From 3839d6709fdf3abfc72d69fb07b8f0db43435fa2 Mon Sep 17 00:00:00 2001 From: Roman Date: Wed, 29 Apr 2026 17:53:50 +0200 Subject: [PATCH 01/47] big change due to the integration of the photom crate --- Cargo.lock | 1391 +++++++------- Cargo.toml | 30 +- rust-toolchain.toml | 2 +- src/cache/mod.rs | 77 + src/cache/observer_centric_cache.rs | 188 ++ src/cache/observer_fixed_cache.rs | 62 + src/constants.rs | 228 +-- src/conversion.rs | 69 +- src/earth_orientation.rs | 13 +- src/env_state.rs | 127 -- src/error_models/data_models/cbm10.rules | 64 - src/error_models/data_models/fcct14.rules | 48 - src/error_models/data_models/vfcc17.rules | 100 -- src/error_models/mod.rs | 418 ----- src/error_models/vfcc17.rs | 96 - src/initial_orbit_determination/gauss.rs | 107 +- src/initial_orbit_determination/mod.rs | 6 + .../triplet_generation/index_generator.rs | 657 +++++++ .../triplet_generation/mod.rs} | 471 +++-- src/jpl_ephem/download_jpl_file.rs | 11 - src/jpl_ephem/horizon/horizon_data.rs | 58 +- src/jpl_ephem/mod.rs | 18 + src/jpl_ephem/naif/naif_data.rs | 27 +- src/lib.rs | 106 +- src/obs_dataset.rs | 113 ++ src/observation_ephemeris.rs | 954 ++++++++++ src/observations/display.rs | 912 ---------- src/observations/mod.rs | 1498 ---------------- src/observations/observations_ext.rs | 1245 ------------- src/observations/triplets_generator.rs | 323 ---- src/observer_extension.rs | 191 ++ src/observers/bimap.rs | 224 --- src/observers/mod.rs | 1140 ------------ src/observers/observatories.rs | 238 --- src/outfit.rs | 676 ------- src/outfit_errors.rs | 30 +- src/trajectories/ades_reader.rs | 257 --- src/trajectories/batch_reader.rs | 432 ----- src/trajectories/mod.rs | 121 -- src/trajectories/mpc_80col_reader.rs | 345 ---- src/trajectories/parquet_reader.rs | 362 ---- src/trajectories/progress_bar.rs | 115 -- src/trajectories/trajectory_file.rs | 513 ------ src/trajectories/trajectory_fit.rs | 1596 ----------------- src/trajectory.rs | 810 +++++++++ tests/outfit_struct_test.rs | 18 - tests/reader_80col_test.rs | 57 - tests/test_gauss_iod.rs | 98 +- tests/test_read_ades.rs | 56 - 49 files changed, 4330 insertions(+), 12368 deletions(-) create mode 100644 src/cache/mod.rs create mode 100644 src/cache/observer_centric_cache.rs create mode 100644 src/cache/observer_fixed_cache.rs delete mode 100644 src/env_state.rs delete mode 100644 src/error_models/data_models/cbm10.rules delete mode 100644 src/error_models/data_models/fcct14.rules delete mode 100644 src/error_models/data_models/vfcc17.rules delete mode 100644 src/error_models/mod.rs delete mode 100644 src/error_models/vfcc17.rs create mode 100644 src/initial_orbit_determination/triplet_generation/index_generator.rs rename src/{observations/triplets_iod.rs => initial_orbit_determination/triplet_generation/mod.rs} (54%) create mode 100644 src/obs_dataset.rs create mode 100644 src/observation_ephemeris.rs delete mode 100644 src/observations/display.rs delete mode 100644 src/observations/mod.rs delete mode 100644 src/observations/observations_ext.rs delete mode 100644 src/observations/triplets_generator.rs create mode 100644 src/observer_extension.rs delete mode 100644 src/observers/bimap.rs delete mode 100644 src/observers/mod.rs delete mode 100644 src/observers/observatories.rs delete mode 100644 src/outfit.rs delete mode 100644 src/trajectories/ades_reader.rs delete mode 100644 src/trajectories/batch_reader.rs delete mode 100644 src/trajectories/mod.rs delete mode 100644 src/trajectories/mpc_80col_reader.rs delete mode 100644 src/trajectories/parquet_reader.rs delete mode 100644 src/trajectories/progress_bar.rs delete mode 100644 src/trajectories/trajectory_file.rs delete mode 100644 src/trajectories/trajectory_fit.rs create mode 100644 src/trajectory.rs delete mode 100644 tests/outfit_struct_test.rs delete mode 100644 tests/reader_80col_test.rs delete mode 100644 tests/test_read_ades.rs diff --git a/Cargo.lock b/Cargo.lock index a841472..781cb90 100644 --- a/Cargo.lock +++ b/Cargo.lock @@ -15,48 +15,42 @@ dependencies = [ [[package]] name = "addr2line" -version = "0.24.2" +version = "0.25.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "dfbe277e56a376000877090da837660b4427aad530e3028d44e0bffe4f89a1c1" +checksum = "1b5d307320b3181d6d7954e663bd7c774a838b8220fe0593c86d9fb09f498b4b" dependencies = [ "gimli", ] [[package]] name = "adler2" -version = "2.0.0" +version = "2.0.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "512761e0bb2578dd7380c6baaa0f4ce03e84f95e960231d1dec8bf4d7d6e2627" +checksum = "320119579fcad9c21884f5c4861d16174d0e06250625266f50fe6898340abefa" [[package]] name = "ahash" -version = "0.8.11" +version = "0.8.12" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "e89da841a80418a9b391ebaea17f5c112ffaaa96f621d2c285b5174da76b9011" +checksum = "5a15f179cd60c4584b8a8c596927aadc462e27f2ca70c04e0071964a73ba7a75" dependencies = [ "cfg-if", "const-random", - "getrandom 0.2.15", + "getrandom 0.3.4", "once_cell", "version_check", - "zerocopy 0.7.35", + "zerocopy", ] [[package]] name = "aho-corasick" -version = "1.1.3" +version = "1.1.4" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "8e60d3430d3a69478ad0993f19238d2df97c507009a52b3c10addcd7f6bcb916" +checksum = "ddd31a130427c27518df266943a5308ed92d4b226cc639f5a8f1002816174301" dependencies = [ "memchr", ] -[[package]] -name = "android-tzdata" -version = "0.1.1" -source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "e999941b234f3131b00bc13c22d06e8c5ff726d1b6318ac7eb276997bbb4fef0" - [[package]] name = "android_system_properties" version = "0.1.5" @@ -74,9 +68,15 @@ checksum = "4b46cbb362ab8752921c97e041f5e366ee6297bd428a31275b9fcf1e380f7299" [[package]] name = "anstyle" -version = "1.0.10" +version = "1.0.14" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "55cc3b69f167a1ef2e161439aa98aed94e6028e5f9a59be9a6ffb47aef1651f9" +checksum 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[[package]] name = "directories" @@ -514,7 +513,7 @@ dependencies = [ "libc", "option-ext", "redox_users", - "windows-sys 0.60.2", + "windows-sys 0.61.2", ] [[package]] @@ -548,19 +547,25 @@ checksum = "877a4ace8713b0bcf2a4e7eec82529c029f1d0619886d18145fea96c3ffe5c0f" [[package]] name = "errno" -version = "0.3.10" +version = "0.3.14" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "33d852cb9b869c2a9b3df2f71a3074817f01e1844f839a144f5fcef059a4eb5d" +checksum = "39cab71617ae0d63f51a36d69f866391735b51691dbda63cf6f96d042b63efeb" dependencies = [ "libc", - "windows-sys 0.59.0", + "windows-sys 0.61.2", ] [[package]] name = "fastrand" -version = "2.3.0" +version = "2.4.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "37909eebbb50d72f9059c3b6d82c0463f2ff062c9e95845c43a6c9c0355411be" +checksum = "9f1f227452a390804cdb637b74a86990f2a7d7ba4b7d5693aac9b4dd6defd8d6" + +[[package]] +name = "find-msvc-tools" +version = "0.1.9" +source = 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"quick-xml 0.37.5", + "rand 0.9.4", "rand_distr", "rayon", "reqwest", @@ -1535,7 +1478,7 @@ dependencies = [ "bytes", "chrono", "half", - "hashbrown", + "hashbrown 0.15.5", "num", "num-bigint", "paste", @@ -1553,27 +1496,32 @@ checksum = "57c0d7b74b563b49d38dae00a0c37d4d6de9b432382b2892f0574ddcae73fd0a" [[package]] name = "percent-encoding" -version = "2.3.1" -source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "e3148f5046208a5d56bcfc03053e3ca6334e51da8dfb19b6cdc8b306fae3283e" - -[[package]] -name = "pin-project-lite" -version = "0.2.16" +version = "2.3.2" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "3b3cff922bd51709b605d9ead9aa71031d81447142d828eb4a6eba76fe619f9b" +checksum = "9b4f627cb1b25917193a259e49bdad08f671f8d9708acfd5fe0a8c1455d87220" [[package]] -name = "pin-utils" +name = "photom" version = "0.1.0" -source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "8b870d8c151b6f2fb93e84a13146138f05d02ed11c7e7c54f8826aaaf7c9f184" +dependencies = [ + "ahash", + "camino", + "directories", + "hifitime", + "itertools 0.14.0", + "nom", + "ordered-float 5.3.0", + "quick-xml 0.39.2", + "serde", + "thiserror", + "ureq", +] [[package]] -name = "pkg-config" -version = "0.3.32" +name = "pin-project-lite" +version = "0.2.17" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "7edddbd0b52d732b21ad9a5fab5c704c14cd949e5e9a1ec5929a24fded1b904c" +checksum = "a89322df9ebe1c1578d689c92318e070967d1042b512afbe49518723f4e6d5cd" [[package]] name = "plotters" @@ -1605,9 +1553,18 @@ dependencies = [ [[package]] name = "portable-atomic" -version = "1.11.1" +version = "1.13.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "f84267b20a16ea918e43c6a88433c2d54fa145c92a811b5b047ccbe153674483" +checksum = "c33a9471896f1c69cecef8d20cbe2f7accd12527ce60845ff44c153bb2a21b49" + +[[package]] +name = "potential_utf" +version = 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source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "a4ce8c88de324ff838700f36fb6ab86c96df0e3c4ab6ef3a9b2044465cce1369" +checksum = "958f21e8e7ceb5a1aa7fa87fab28e7c75976e0bfe7e23ff069e0a260f894067d" dependencies = [ "memchr", "serde", @@ -1707,14 +1683,14 @@ dependencies = [ [[package]] name = "quinn-proto" -version = "0.11.13" +version = "0.11.14" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "f1906b49b0c3bc04b5fe5d86a77925ae6524a19b816ae38ce1e426255f1d8a31" +checksum = "434b42fec591c96ef50e21e886936e66d3cc3f737104fdb9b737c40ffb94c098" dependencies = [ "bytes", - "getrandom 0.3.2", + "getrandom 0.3.4", "lru-slab", - "rand", + "rand 0.9.4", "ring", "rustc-hash", "rustls", @@ -1742,27 +1718,43 @@ dependencies = [ [[package]] name = "quote" -version = "1.0.40" +version = "1.0.45" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "1885c039570dc00dcb4ff087a89e185fd56bae234ddc7f056a945bf36467248d" +checksum = 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+dependencies = [ + "getrandom 0.3.4", ] [[package]] @@ -1791,7 +1792,7 @@ source = "registry+https://github.com/rust-lang/crates.io-index" checksum = "6a8615d50dcf34fa31f7ab52692afec947c4dd0ab803cc87cb3b0b4570ff7463" dependencies = [ "num-traits", - "rand", + "rand 0.9.4", ] [[package]] @@ -1800,7 +1801,7 @@ version = "0.4.0" source = "registry+https://github.com/rust-lang/crates.io-index" checksum = "513962919efc330f829edb2535844d1b912b0fbe2ca165d613e4e8788bb05a5a" dependencies = [ - "rand_core", + "rand_core 0.9.5", ] [[package]] @@ -1811,9 +1812,9 @@ checksum = "60a357793950651c4ed0f3f52338f53b2f809f32d83a07f72909fa13e4c6c1e3" [[package]] name = "rayon" -version = "1.11.0" +version = "1.12.0" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "368f01d005bf8fd9b1206fb6fa653e6c4a81ceb1466406b81792d87c5677a58f" +checksum = "fb39b166781f92d482534ef4b4b1b2568f42613b53e5b6c160e24cfbfa30926d" dependencies = [ "either", "rayon-core", @@ -1831,20 +1832,20 @@ dependencies = [ [[package]] name = "redox_users" -version = "0.5.0" +version = "0.5.2" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "dd6f9d3d47bdd2ad6945c5015a226ec6155d0bcdfd8f7cd29f86b71f8de99d2b" +checksum = "a4e608c6638b9c18977b00b475ac1f28d14e84b27d8d42f70e0bf1e3dec127ac" dependencies = [ - "getrandom 0.2.15", + "getrandom 0.2.17", "libredox", "thiserror", ] [[package]] name = "regex" -version = "1.11.1" +version = "1.12.3" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "b544ef1b4eac5dc2db33ea63606ae9ffcfac26c1416a2806ae0bf5f56b201191" +checksum = "e10754a14b9137dd7b1e3e5b0493cc9171fdd105e0ab477f51b72e7f3ac0e276" dependencies = [ "aho-corasick", "memchr", @@ -1854,9 +1855,9 @@ dependencies = [ [[package]] name = "regex-automata" -version = "0.4.9" +version = "0.4.14" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "809e8dc61f6de73b46c85f4c96486310fe304c434cfa43669d7b40f711150908" +checksum = "6e1dd4122fc1595e8162618945476892eefca7b88c52820e74af6262213cae8f" dependencies = [ "aho-corasick", "memchr", @@ -1865,15 +1866,15 @@ dependencies = [ [[package]] name = "regex-syntax" -version = "0.8.5" +version = "0.8.10" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "2b15c43186be67a4fd63bee50d0303afffcef381492ebe2c5d87f324e1b8815c" +checksum = "dc897dd8d9e8bd1ed8cdad82b5966c3e0ecae09fb1907d58efaa013543185d0a" [[package]] name = "reqwest" -version = "0.12.15" +version = "0.12.28" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "d19c46a6fdd48bc4dab94b6103fccc55d34c67cc0ad04653aad4ea2a07cd7bbb" +checksum = "eddd3ca559203180a307f12d114c268abf583f59b03cb906fd0b3ff8646c1147" dependencies = [ "base64", "bytes", @@ -1886,16 +1887,12 @@ dependencies = [ "hyper", "hyper-rustls", "hyper-util", - "ipnet", "js-sys", "log", - "mime", - "once_cell", "percent-encoding", "pin-project-lite", "quinn", "rustls", - "rustls-pemfile", "rustls-pki-types", "serde", "serde_json", @@ -1905,14 +1902,14 @@ dependencies = [ "tokio-rustls", "tokio-util", "tower", + "tower-http", "tower-service", "url", "wasm-bindgen", "wasm-bindgen-futures", "wasm-streams", "web-sys", - "webpki-roots 0.26.8", - "windows-registry", + "webpki-roots", ] [[package]] @@ -1923,7 +1920,7 @@ checksum = "a4689e6c2294d81e88dc6261c768b63bc4fcdb852be6d1352498b114f61383b7" dependencies = [ "cc", "cfg-if", - "getrandom 0.2.15", + "getrandom 0.2.17", "libc", "untrusted", "windows-sys 0.52.0", @@ -1937,15 +1934,15 @@ checksum = "082f11ffa03bbef6c2c6ea6bea1acafaade2fd9050ae0234ab44a2153742b058" [[package]] name = "rustc-demangle" -version = "0.1.24" +version = "0.1.27" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "719b953e2095829ee67db738b3bfa9fa368c94900df327b3f07fe6e794d2fe1f" +checksum = "b50b8869d9fc858ce7266cce0194bd74df58b9d0e3f6df3a9fc8eb470d95c09d" [[package]] name = "rustc-hash" -version = "2.1.1" +version = "2.1.2" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "357703d41365b4b27c590e3ed91eabb1b663f07c4c084095e60cbed4362dff0d" +checksum = "94300abf3f1ae2e2b8ffb7b58043de3d399c73fa6f4b73826402a5c457614dbe" [[package]] name = "rustc_version" @@ -1958,22 +1955,22 @@ dependencies = [ [[package]] name = "rustix" -version = "1.0.5" +version = "1.1.4" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "d97817398dd4bb2e6da002002db259209759911da105da92bec29ccb12cf58bf" +checksum = "b6fe4565b9518b83ef4f91bb47ce29620ca828bd32cb7e408f0062e9930ba190" dependencies = [ - "bitflags 2.9.0", + "bitflags 2.11.1", "errno", "libc", "linux-raw-sys", - "windows-sys 0.59.0", + "windows-sys 0.61.2", ] [[package]] name = "rustls" -version = "0.23.25" +version = "0.23.39" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "822ee9188ac4ec04a2f0531e55d035fb2de73f18b41a63c70c2712503b6fb13c" +checksum = "7c2c118cb077cca2822033836dfb1b975355dfb784b5e8da48f7b6c5db74e60e" dependencies = [ "log", "once_cell", @@ -1984,29 +1981,21 @@ dependencies = [ "zeroize", ] -[[package]] -name = "rustls-pemfile" -version = "2.2.0" -source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "dce314e5fee3f39953d46bb63bb8a46d40c2f8fb7cc5a3b6cab2bde9721d6e50" -dependencies = [ - "rustls-pki-types", -] - [[package]] name = "rustls-pki-types" -version = "1.11.0" +version = "1.14.0" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "917ce264624a4b4db1c364dcc35bfca9ded014d0a958cd47ad3e960e988ea51c" +checksum = "be040f8b0a225e40375822a563fa9524378b9d63112f53e19ffff34df5d33fdd" dependencies = [ "web-time", + "zeroize", ] [[package]] name = "rustls-webpki" -version = "0.103.1" +version = "0.103.13" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "fef8b8769aaccf73098557a87cd1816b4f9c7c16811c9c77142aa695c16f2c03" +checksum = "61c429a8649f110dddef65e2a5ad240f747e85f7758a6bccc7e5777bd33f756e" dependencies = [ "ring", "rustls-pki-types", @@ -2015,15 +2004,15 @@ dependencies = [ [[package]] name = "rustversion" -version = "1.0.20" +version = "1.0.22" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "eded382c5f5f786b989652c49544c4877d9f015cc22e145a5ea8ea66c2921cd2" +checksum = "b39cdef0fa800fc44525c84ccb54a029961a8215f9619753635a9c0d2538d46d" [[package]] name = "rusty-fork" -version = "0.3.0" +version = "0.3.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "cb3dcc6e454c328bb824492db107ab7c0ae8fcffe4ad210136ef014458c1bc4f" +checksum = "cc6bf79ff24e648f6da1f8d1f011e9cac26491b619e6b9280f2b47f1774e6ee2" dependencies = [ "fnv", "quick-error", @@ -2033,9 +2022,9 @@ dependencies = [ [[package]] name = "ryu" -version = "1.0.20" +version = "1.0.23" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "28d3b2b1366ec20994f1fd18c3c594f05c5dd4bc44d8bb0c1c632c8d6829481f" +checksum = "9774ba4a74de5f7b1c1451ed6cd5285a32eddb5cccb8cc655a4e50009e06477f" [[package]] name = "safe_arch" @@ -2057,9 +2046,9 @@ dependencies = [ [[package]] name = "semver" -version = "1.0.26" +version = "1.0.28" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "56e6fa9c48d24d85fb3de5ad847117517440f6beceb7798af16b4a87d616b8d0" +checksum = "8a7852d02fc848982e0c167ef163aaff9cd91dc640ba85e263cb1ce46fae51cd" [[package]] name = "seq-macro" @@ -2069,18 +2058,28 @@ checksum = "1bc711410fbe7399f390ca1c3b60ad0f53f80e95c5eb935e52268a0e2cd49acc" [[package]] name = "serde" -version = "1.0.219" +version = "1.0.228" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "5f0e2c6ed6606019b4e29e69dbaba95b11854410e5347d525002456dbbb786b6" +checksum = "9a8e94ea7f378bd32cbbd37198a4a91436180c5bb472411e48b5ec2e2124ae9e" +dependencies = [ + "serde_core", + "serde_derive", +] + +[[package]] +name = "serde_core" +version = "1.0.228" +source = "registry+https://github.com/rust-lang/crates.io-index" +checksum = "41d385c7d4ca58e59fc732af25c3983b67ac852c1a25000afe1175de458b67ad" dependencies = [ "serde_derive", ] [[package]] name = "serde_derive" -version = "1.0.219" +version = "1.0.228" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "5b0276cf7f2c73365f7157c8123c21cd9a50fbbd844757af28ca1f5925fc2a00" +checksum = "d540f220d3187173da220f885ab66608367b6574e925011a9353e4badda91d79" dependencies = [ "proc-macro2", "quote", @@ -2089,14 +2088,15 @@ dependencies = [ [[package]] name = "serde_json" -version = "1.0.140" +version = "1.0.149" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "20068b6e96dc6c9bd23e01df8827e6c7e1f2fddd43c21810382803c136b99373" +checksum = "83fc039473c5595ace860d8c4fafa220ff474b3fc6bfdb4293327f1a37e94d86" dependencies = [ "itoa", "memchr", - "ryu", "serde", + "serde_core", + "zmij", ] [[package]] @@ -2119,9 +2119,9 @@ checksum = "0fda2ff0d084019ba4d7c6f371c95d8fd75ce3524c3cb8fb653a3023f6323e64" [[package]] name = "simba" -version = "0.9.0" +version = "0.9.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "b3a386a501cd104797982c15ae17aafe8b9261315b5d07e3ec803f2ea26be0fa" +checksum = "c99284beb21666094ba2b75bbceda012e610f5479dfcc2d6e2426f53197ffd95" dependencies = [ "approx", "num-complex", @@ -2132,24 +2132,21 @@ dependencies = [ [[package]] name = "slab" -version = "0.4.9" +version = "0.4.12" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "8f92a496fb766b417c996b9c5e57daf2f7ad3b0bebe1ccfca4856390e3d3bb67" -dependencies = [ - "autocfg", -] +checksum = "0c790de23124f9ab44544d7ac05d60440adc586479ce501c1d6d7da3cd8c9cf5" [[package]] name = "smallvec" -version = "1.14.0" +version = "1.15.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "7fcf8323ef1faaee30a44a340193b1ac6814fd9b7b4e88e9d4519a3e4abe1cfd" +checksum = "67b1b7a3b5fe4f1376887184045fcf45c69e92af734b7aaddc05fb777b6fbd03" [[package]] name = "snafu" -version = "0.8.5" +version = "0.9.0" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "223891c85e2a29c3fe8fb900c1fae5e69c2e42415e3177752e8718475efa5019" +checksum = "d1d4bced6a69f90b2056c03dcff2c4737f98d6fb9e0853493996e1d253ca29c6" dependencies = [ "backtrace", "snafu-derive", @@ -2157,9 +2154,9 @@ dependencies = [ [[package]] name = "snafu-derive" -version = "0.8.5" +version = "0.9.0" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "03c3c6b7927ffe7ecaa769ee0e3994da3b8cafc8f444578982c83ecb161af917" +checksum = "54254b8531cafa275c5e096f62d48c81435d1015405a91198ddb11e967301d40" dependencies = [ "heck", "proc-macro2", @@ -2175,19 +2172,19 @@ checksum = "1b6b67fb9a61334225b5b790716f609cd58395f895b3fe8b328786812a40bc3b" [[package]] name = "socket2" -version = "0.5.9" +version = "0.6.3" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "4f5fd57c80058a56cf5c777ab8a126398ece8e442983605d280a44ce79d0edef" +checksum = "3a766e1110788c36f4fa1c2b71b387a7815aa65f88ce0229841826633d93723e" dependencies = [ "libc", - "windows-sys 0.52.0", + "windows-sys 0.61.2", ] [[package]] name = "stable_deref_trait" -version = "1.2.0" +version = "1.2.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "a8f112729512f8e442d81f95a8a7ddf2b7c6b8a1a6f509a95864142b30cab2d3" +checksum = "6ce2be8dc25455e1f91df71bfa12ad37d7af1092ae736f3a6cd0e37bc7810596" [[package]] name = "static_assertions" @@ -2203,9 +2200,9 @@ checksum = "13c2bddecc57b384dee18652358fb23172facb8a2c51ccc10d74c157bdea3292" [[package]] name = "syn" -version = "2.0.100" +version = "2.0.117" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "b09a44accad81e1ba1cd74a32461ba89dee89095ba17b32f5d03683b1b1fc2a0" +checksum = "e665b8803e7b1d2a727f4023456bbbbe74da67099c585258af0ad9c5013b9b99" dependencies = [ "proc-macro2", "quote", @@ -2223,9 +2220,9 @@ dependencies = [ [[package]] name = "synstructure" -version = "0.13.1" +version = "0.13.2" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "c8af7666ab7b6390ab78131fb5b0fce11d6b7a6951602017c35fa82800708971" +checksum = "728a70f3dbaf5bab7f0c4b1ac8d7ae5ea60a4b5549c8a5914361c99147a709d2" dependencies = [ "proc-macro2", "quote", @@ -2258,15 +2255,15 @@ dependencies = [ [[package]] name = "tempfile" -version = "3.19.1" +version = "3.27.0" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "7437ac7763b9b123ccf33c338a5cc1bac6f69b45a136c19bdd8a65e3916435bf" +checksum = "32497e9a4c7b38532efcdebeef879707aa9f794296a4f0244f6f69e9bc8574bd" dependencies = [ "fastrand", - "getrandom 0.3.2", + "getrandom 0.4.2", "once_cell", "rustix", - "windows-sys 0.59.0", + "windows-sys 0.61.2", ] [[package]] @@ -2280,18 +2277,18 @@ dependencies = [ [[package]] name = "thiserror" -version = "2.0.12" +version = "2.0.18" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "567b8a2dae586314f7be2a752ec7474332959c6460e02bde30d702a66d488708" +checksum = "4288b5bcbc7920c07a1149a35cf9590a2aa808e0bc1eafaade0b80947865fbc4" dependencies = [ "thiserror-impl", ] [[package]] name = "thiserror-impl" -version = "2.0.12" +version = "2.0.18" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "7f7cf42b4507d8ea322120659672cf1b9dbb93f8f2d4ecfd6e51350ff5b17a1d" +checksum = "ebc4ee7f67670e9b64d05fa4253e753e016c6c95ff35b89b7941d6b856dec1d5" dependencies = [ "proc-macro2", "quote", @@ -2320,9 +2317,9 @@ dependencies = [ [[package]] name = "tinystr" -version = "0.7.6" +version = "0.8.3" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "9117f5d4db391c1cf6927e7bea3db74b9a1c1add8f7eda9ffd5364f40f57b82f" +checksum = "c8323304221c2a851516f22236c5722a72eaa19749016521d6dff0824447d96d" dependencies = [ "displaydoc", "zerovec", @@ -2340,9 +2337,9 @@ dependencies = [ [[package]] name = "tinyvec" -version = "1.10.0" +version = "1.11.0" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "bfa5fdc3bce6191a1dbc8c02d5c8bffcf557bafa17c124c5264a458f1b0613fa" +checksum = "3e61e67053d25a4e82c844e8424039d9745781b3fc4f32b8d55ed50f5f667ef3" dependencies = [ "tinyvec_macros", ] @@ -2355,24 +2352,23 @@ checksum = "1f3ccbac311fea05f86f61904b462b55fb3df8837a366dfc601a0161d0532f20" [[package]] name = "tokio" -version = "1.44.1" +version = "1.52.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "f382da615b842244d4b8738c82ed1275e6c5dd90c459a30941cd07080b06c91a" +checksum = "b67dee974fe86fd92cc45b7a95fdd2f99a36a6d7b0d431a231178d3d670bbcc6" dependencies = [ - "backtrace", "bytes", "libc", "mio", "pin-project-lite", "socket2", - "windows-sys 0.52.0", + "windows-sys 0.61.2", ] [[package]] name = "tokio-rustls" -version = "0.26.2" +version = "0.26.4" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "8e727b36a1a0e8b74c376ac2211e40c2c8af09fb4013c60d910495810f008e9b" +checksum = "1729aa945f29d91ba541258c8df89027d5792d85a8841fb65e8bf0f4ede4ef61" dependencies = [ "rustls", "tokio", @@ -2380,9 +2376,9 @@ dependencies = [ [[package]] name = "tokio-stream" -version = "0.1.17" +version = "0.1.18" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "eca58d7bba4a75707817a2c44174253f9236b2d5fbd055602e9d5c07c139a047" +checksum = "32da49809aab5c3bc678af03902d4ccddea2a87d028d86392a4b1560c6906c70" dependencies = [ "futures-core", "pin-project-lite", @@ -2391,9 +2387,9 @@ dependencies = [ [[package]] name = "tokio-util" -version = "0.7.14" +version = "0.7.18" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "6b9590b93e6fcc1739458317cccd391ad3955e2bde8913edf6f95f9e65a8f034" +checksum = "9ae9cec805b01e8fc3fd2fe289f89149a9b66dd16786abd8b19cfa7b48cb0098" dependencies = [ "bytes", "futures-core", @@ -2404,9 +2400,9 @@ dependencies = [ [[package]] name = "tower" -version = "0.5.2" +version = "0.5.3" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "d039ad9159c98b70ecfd540b2573b97f7f52c3e8d9f8ad57a24b916a536975f9" +checksum = "ebe5ef63511595f1344e2d5cfa636d973292adc0eec1f0ad45fae9f0851ab1d4" dependencies = [ "futures-core", "futures-util", @@ -2417,6 +2413,24 @@ dependencies = [ "tower-service", ] +[[package]] +name = "tower-http" +version = "0.6.8" +source = "registry+https://github.com/rust-lang/crates.io-index" +checksum = "d4e6559d53cc268e5031cd8429d05415bc4cb4aefc4aa5d6cc35fbf5b924a1f8" +dependencies = [ + "bitflags 2.11.1", + "bytes", + "futures-util", + "http", + "http-body", + "iri-string", + "pin-project-lite", + "tower", + "tower-layer", + "tower-service", +] + [[package]] name = "tower-layer" version = "0.3.3" @@ -2431,9 +2445,9 @@ checksum = "8df9b6e13f2d32c91b9bd719c00d1958837bc7dec474d94952798cc8e69eeec3" [[package]] name = "tracing" -version = "0.1.41" +version = "0.1.44" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "784e0ac535deb450455cbfa28a6f0df145ea1bb7ae51b821cf5e7927fdcfbdd0" +checksum = "63e71662fa4b2a2c3a26f570f037eb95bb1f85397f3cd8076caed2f026a6d100" dependencies = [ "pin-project-lite", "tracing-core", @@ -2441,9 +2455,9 @@ dependencies = [ [[package]] name = "tracing-core" -version = "0.1.33" +version = "0.1.36" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "e672c95779cf947c5311f83787af4fa8fffd12fb27e4993211a84bdfd9610f9c" +checksum = "db97caf9d906fbde555dd62fa95ddba9eecfd14cb388e4f491a66d74cd5fb79a" dependencies = [ "once_cell", ] @@ -2466,9 +2480,9 @@ dependencies = [ [[package]] name = "typenum" -version = "1.18.0" +version = "1.20.0" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = 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dependencies = [ "form_urlencoded", "idna", "percent-encoding", + "serde", ] [[package]] -name = "utf-8" -version = "0.7.6" -source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "09cc8ee72d2a9becf2f2febe0205bbed8fc6615b7cb429ad062dc7b7ddd036a9" - -[[package]] -name = "utf16_iter" -version = "1.0.5" +name = "utf8-zero" +version = "0.8.1" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "c8232dd3cdaed5356e0f716d285e4b40b932ac434100fe9b7e0e8e935b9e6246" +checksum = "b8c0a043c9540bae7c578c88f91dda8bd82e59ae27c21baca69c8b191aaf5a6e" [[package]] name = "utf8_iter" @@ -2564,12 +2578,6 @@ version = "1.0.4" source = "registry+https://github.com/rust-lang/crates.io-index" checksum = "b6c140620e7ffbb22c2dee59cafe6084a59b5ffc27a8859a5f0d494b5d52b6be" -[[package]] -name = "vcpkg" -version = "0.2.15" -source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "accd4ea62f7bb7a82fe23066fb0957d48ef677f6eeb8215f372f52e48bb32426" - 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"de844c262c8848816172cef550288e7dc6c7b7814b4ee56b3e1553f275f1858e" dependencies = [ "proc-macro2", "quote", "syn", + "synstructure", +] + +[[package]] +name = "zerocopy" +version = "0.8.48" +source = "registry+https://github.com/rust-lang/crates.io-index" +checksum = "eed437bf9d6692032087e337407a86f04cd8d6a16a37199ed57949d415bd68e9" +dependencies = [ + "zerocopy-derive", ] [[package]] name = "zerocopy-derive" -version = "0.8.26" +version = "0.8.48" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "9ecf5b4cc5364572d7f4c329661bcc82724222973f2cab6f050a4e5c22f75181" +checksum = "70e3cd084b1788766f53af483dd21f93881ff30d7320490ec3ef7526d203bad4" dependencies = [ "proc-macro2", "quote", @@ -3082,18 +3146,18 @@ dependencies = [ [[package]] name = "zerofrom" -version = "0.1.6" +version = "0.1.7" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "50cc42e0333e05660c3587f3bf9d0478688e15d870fab3346451ce7f8c9fbea5" +checksum = 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"displaydoc", + "yoke", + "zerofrom", +] [[package]] name = "zerovec" -version = "0.10.4" +version = "0.11.6" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "aa2b893d79df23bfb12d5461018d408ea19dfafe76c2c7ef6d4eba614f8ff079" +checksum = "90f911cbc359ab6af17377d242225f4d75119aec87ea711a880987b18cd7b239" dependencies = [ "yoke", "zerofrom", @@ -3120,11 +3195,17 @@ dependencies = [ [[package]] name = "zerovec-derive" -version = "0.10.3" +version = "0.11.3" source = "registry+https://github.com/rust-lang/crates.io-index" -checksum = "6eafa6dfb17584ea3e2bd6e76e0cc15ad7af12b09abdd1ca55961bed9b1063c6" +checksum = "625dc425cab0dca6dc3c3319506e6593dcb08a9f387ea3b284dbd52a92c40555" dependencies = [ "proc-macro2", "quote", "syn", ] + +[[package]] +name = "zmij" +version = "1.0.21" +source = "registry+https://github.com/rust-lang/crates.io-index" +checksum = "b8848ee67ecc8aedbaf3e4122217aff892639231befc6a1b58d29fff4c2cabaa" diff --git a/Cargo.toml b/Cargo.toml index a1867e8..150d3bb 100644 --- a/Cargo.toml +++ b/Cargo.toml @@ -1,9 +1,9 @@ [package] name = "outfit" -version = "2.1.0" +version = "3.0.0" edition = "2021" license-file = "LICENSE" -rust-version = "1.82" +rust-version = "1.94.0" description = "Orbit determination toolkit in Rust. Provides astrometric parsing, observer management, and initial orbit determination (Gauss method) with JPL ephemeris support." readme = "README.md" repository = "https://github.com/FusRoman/Outfit" @@ -20,6 +20,9 @@ categories = ["science", "parsing", "data-structures"] authors = ["Roman Le Montagner "] [dependencies] + +photom = { version = "0.1.0", path = "../photom" } + aberth = { version = "0.4.1", default-features = false } ahash = { version = "0.8.11", default-features = false } arrow-array = { version = "54.3.1", default-features = false } @@ -54,18 +57,18 @@ rand = { version = "0.9.2", default-features = false, features = [ ] } rand_distr = { version = "0.5.1", default-features = false } -reqwest = { version = "0.12.15", default-features = false, optional = true, features = [ +reqwest = { version = "0.12.15", default-features = false, features = [ "http2", "rustls-tls", "stream", ] } -tokio = { version = "1.44.1", default-features = false, optional = true, features = [ +tokio = { version = "1.44.1", default-features = false, features = [ "fs", "rt", "rt-multi-thread", "io-util", ] } -tokio-stream = { version = "0.1.17", default-features = false, optional = true } +tokio-stream = { version = "0.1.17", default-features = false } indicatif = { version = "0.18", optional = true, default-features = false } rayon = { version = "1.11.0", optional = true, default-features = false } comfy-table = { version = "7.1.4", default-features = false } @@ -76,21 +79,12 @@ criterion = { version = "0.5.1", features = ["html_reports"] } husky-rs = "0.1.5" proptest = "1.7.0" +photom = { version = "0.1.0", path = "../photom", features = ["mpc_80_col", "ades"] } + [features] -jpl-download = ["dep:reqwest", "dep:tokio", "dep:tokio-stream"] progress = ["dep:indicatif"] parallel = ["dep:rayon"] -[[test]] -name = "reader_80col_test" -path = "tests/reader_80col_test.rs" -required-features = ["jpl-download"] - -[[test]] -name = "test_read_ades" -path = "tests/test_read_ades.rs" -required-features = ["jpl-download"] - [[test]] name = "test_large_parquet" path = "tests/trajectories_from_parquet.rs" @@ -142,7 +136,3 @@ debug = false lto = "fat" codegen-units = 1 strip = true - -[package.metadata.docs.rs] -features = ["jpl-download"] -rustdoc-args = ["--cfg", "docsrs"] diff --git a/rust-toolchain.toml b/rust-toolchain.toml index 7855e6d..0d8ed42 100644 --- a/rust-toolchain.toml +++ b/rust-toolchain.toml @@ -1,3 +1,3 @@ [toolchain] -channel = "1.88.0" +channel = "1.94.0" components = ["rustfmt", "clippy"] diff --git a/src/cache/mod.rs b/src/cache/mod.rs new file mode 100644 index 0000000..345c720 --- /dev/null +++ b/src/cache/mod.rs @@ -0,0 +1,77 @@ +pub mod observer_centric_cache; +pub mod observer_fixed_cache; + +use hifitime::ut1::Ut1Provider; +use photom::{observation_dataset::ObsDataset, observer::dataset::ObserverId, ObsIndex}; + +use crate::{ + cache::{ + observer_centric_cache::{ + build_centric_observer_cache, CentricObserverCache, ObserverCentricCache, + ObserverGeocentricPosition, ObserverGeocentricVelocity, ObserverHeliocentricPosition, + }, + observer_fixed_cache::{ + build_fixed_observer_cache, BodyFixedObserverCache, ObserverFixedCache, + }, + }, + JPLEphem, OutfitError, +}; + +/// Precomputed observer positions for all observations in a dataset. +/// +/// Built once before any trajectory fitting. Each entry is keyed by the +/// observation's [`ObsIndex`], which is stable for the lifetime of the +/// [`ObsDataset`]. +pub struct OutfitCache { + /// len == number of observations in the dataset. Indexed by [`ObsIndex`]. + observer_centric: CentricObserverCache, + /// len == number of observer in the dataset. Indexed by observer ID. + observer_fixed: BodyFixedObserverCache, +} + +impl OutfitCache { + pub fn get_centric(&self, idx: ObsIndex) -> &ObserverCentricCache { + &self.observer_centric[idx] + } + + pub fn get_fixed(&self, observer_id: ObserverId) -> Option<&ObserverFixedCache> { + self.observer_fixed.get(&observer_id) + } + + /// Build the cache for every observation in `obs_dataset`. + pub fn build( + obs_dataset: &ObsDataset, + jpl: &JPLEphem, + ut1_provider: &Ut1Provider, + ) -> Result { + let observer_iter = obs_dataset.iter_observer()?; + + let observer_fixed_cache = build_fixed_observer_cache(observer_iter)?; + + let observer_centric_cache = + build_centric_observer_cache(jpl, ut1_provider, obs_dataset, &observer_fixed_cache)?; + + Ok(Self { + observer_centric: observer_centric_cache, + observer_fixed: observer_fixed_cache, + }) + } + + pub fn get_observer_fixed_cache(&self, observer_id: ObserverId) -> Option<&ObserverFixedCache> { + self.observer_fixed.get(&observer_id) + } + + /// Accessor for the precomputed geocentric position of an observer. + pub fn get_observer_geocentric_position(&self, idx: ObsIndex) -> &ObserverGeocentricPosition { + &self.get_centric(idx).geo_position + } + + pub fn get_observer_geocentric_velocity(&self, idx: ObsIndex) -> &ObserverGeocentricVelocity { + &self.get_centric(idx).geo_velocity + } + + /// Accessor for the precomputed heliocentric position of an observer. + pub fn get_helio_position(&self, idx: ObsIndex) -> &ObserverHeliocentricPosition { + &self.get_centric(idx).helio_position + } +} diff --git a/src/cache/observer_centric_cache.rs b/src/cache/observer_centric_cache.rs new file mode 100644 index 0000000..aa48a9a --- /dev/null +++ b/src/cache/observer_centric_cache.rs @@ -0,0 +1,188 @@ +use hifitime::{ut1::Ut1Provider, Epoch}; +use nalgebra::Vector3; +use ordered_float::NotNan; +use photom::{observation_dataset::ObsDataset, observer::Observer, MJDTT}; + +use crate::{ + cache::observer_fixed_cache::{BodyFixedObserverCache, ObserverFixedCache}, + observer_extension::ResolvedObserver, + JPLEphem, OutfitError, +}; + +/// Geocentric position of the observer at `time` of an observation (AU, ecliptic mean J2000). +pub type ObserverGeocentricPosition = Vector3>; +/// Geocentric velocity of the observer at `time` of an observation (AU/day, ecliptic mean J2000). +pub type ObserverGeocentricVelocity = Vector3>; +/// Heliocentric position of the observer at `time` of an observation (AU, ecliptic mean J2000). +pub type ObserverHeliocentricPosition = Vector3>; + +/// Geocentric and heliocentric observer positions for a single observation epoch. +pub struct ObserverCentricCache { + pub geo_position: ObserverGeocentricPosition, + pub geo_velocity: ObserverGeocentricVelocity, + pub helio_position: ObserverHeliocentricPosition, +} + +impl ObserverCentricCache { + pub fn new( + jpl: &JPLEphem, + ut1_provider: &Ut1Provider, + obs_time: MJDTT, + observer_fixed_cache: &ObserverFixedCache, + ) -> Result { + let obs_mjd = Epoch::from_mjd_in_time_scale(obs_time, hifitime::TimeScale::TT); + let (geocentric_pos, geocentric_vel) = + Observer::pvobs(&obs_mjd, ut1_provider, observer_fixed_cache)?; + + let heliocentric_pos = Observer::helio_position(jpl, &obs_mjd, &geocentric_pos)?; + + Ok(Self { + geo_position: geocentric_pos, + geo_velocity: geocentric_vel, + helio_position: heliocentric_pos, + }) + } +} + +pub type CentricObserverCache = Vec; + +pub fn build_centric_observer_cache( + jpl: &JPLEphem, + ut1_provider: &Ut1Provider, + obs_dataset: &ObsDataset, + observer_fixed_cache: &BodyFixedObserverCache, +) -> Result { + obs_dataset + .iter_observations() + .enumerate() + .map(|(idx, obs)| { + let observer_id = obs + .observer_id() + .ok_or_else(|| return OutfitError::ObserverIdIsNone(idx as u64))?; + + let fixed_cache = observer_fixed_cache + .get(&observer_id) + .ok_or_else(|| return OutfitError::ObserverIdIsNone(idx as u64))?; + + ObserverCentricCache::new(jpl, ut1_provider, obs.mjd_tt(), fixed_cache) + }) + .collect() +} + +#[cfg(test)] +mod observer_test { + + use photom::{Meters, Radians}; + + use crate::{ + cache::observer_centric_cache::ObserverCentricCache, + test_fixture::{JPL_EPHEM_HORIZON, UT1_PROVIDER}, + }; + + use super::*; + + fn to_observer( + longitude: Radians, + latitude: Radians, + height: Meters, + name: Option, + ra_accuracy: Option, + dec_accuracy: Option, + ) -> Observer { + let observer = Observer::new(longitude, latitude, height, name, ra_accuracy, dec_accuracy) + .expect("Failed to create Observer"); + observer + } + + #[test] + fn body_fixed_coord_test() { + // longitude, latitude and height of Pan-STARRS 1, Haleakala + let (lon, lat, h) = ( + 203.744090000_f64.to_radians(), + 20.707233557_f64.to_radians(), + 3067.694, + ); + let pan_starrs = to_observer(lon, lat, h, None, None, None); + assert_eq!( + pan_starrs + .earth_fixed_position() + .unwrap() + .map(|x| x.into_inner()), + Vector3::new( + -0.00003653799439776371, + -0.00001607260397528885, + 0.000014988110430544328 + ) + ); + } + + #[test] + fn pvobs_test() { + let tmjd = 57028.479297592596; + let epoch = Epoch::from_mjd_in_time_scale(tmjd, hifitime::TimeScale::TT); + // longitude, latitude and height of Pan-STARRS 1, Haleakala + let (lon, lat, h) = ( + 203.744090000_f64.to_radians(), + 20.707233557_f64.to_radians(), + 3067.694, + ); + + let pan_starrs = to_observer(lon, lat, h, Some("Pan-STARRS 1".to_string()), None, None); + + let observer_fixed_cache: ObserverFixedCache = (&pan_starrs).try_into().unwrap(); + + let (observer_position, observer_velocity) = + Observer::pvobs(&epoch, &UT1_PROVIDER, &observer_fixed_cache).unwrap(); + + assert_eq!( + observer_position.as_slice(), + [ + -2.086211182493635e-5, + 3.718476815327979e-5, + 2.4978996447997476e-7 + ] + ); + assert_eq!( + observer_velocity.as_slice(), + [ + -0.0002143246535691577, + -0.00012059801691431748, + 5.262184624215718e-5 + ] + ); + } + + #[test] + fn test_helio_pos_obs() { + let (lon, lat, h) = (203.744090000, 20.707233557, 3067.694); + let pan_starrs = to_observer(lon, lat, h, Some("Pan-STARRS 1".to_string()), None, None); + let observer_fixed_cache: ObserverFixedCache = (&pan_starrs).try_into().unwrap(); + + let cases = [ + ( + 57_028.479_297_592_596, + [-0.2645666171464416, 0.8689351643701766, 0.3766996211107864], + ), + ( + 57_049.245_147_592_59, + [-0.5891631852137064, 0.7238872516824697, 0.3138186516540669], + ), + ( + 57_063.977_117_592_59, + [-0.7743280306286537, 0.5612532665812755, 0.24333415479994636], + ), + ]; + + for (tmjd, expected) in cases { + let obs = ObserverCentricCache::new( + &JPL_EPHEM_HORIZON, + &UT1_PROVIDER, + tmjd, + &observer_fixed_cache, + ) + .unwrap(); + + assert_eq!(obs.helio_position.as_slice(), expected, "tmjd = {tmjd}"); + } + } +} diff --git a/src/cache/observer_fixed_cache.rs b/src/cache/observer_fixed_cache.rs new file mode 100644 index 0000000..09b1664 --- /dev/null +++ b/src/cache/observer_fixed_cache.rs @@ -0,0 +1,62 @@ +use ahash::AHashMap; +use nalgebra::Vector3; +use ordered_float::NotNan; +use photom::observer::{dataset::ObserverId, Observer}; + +use crate::{ + constants::EARTH_ROTATION, conversion::ToNotNan, observer_extension::ResolvedObserver, + OutfitError, +}; + +/// Precomputed **body-fixed** position of the observer in **AU**. +pub type ObserverFixedPosition = Vector3>; +/// Precomputed **body-fixed** velocity of the observer in **AU/day**. +pub type ObserverFixedVelocity = Vector3>; + +pub struct ObserverFixedCache { + observer_fixed_positions: ObserverFixedPosition, + observer_fixed_velocities: ObserverFixedVelocity, +} + +impl ObserverFixedCache { + pub fn new(observer: &Observer) -> Result { + // Body-fixed position in AU from (ρ·cosφ, ρ·sinφ) scaled by Earth radius (AU). + let body_fixed_pos = observer.earth_fixed_position()?; + + // Body-fixed velocity from Earth rotation. + let body_fixed_vel: Vector3> = + EARTH_ROTATION.to_notnan()?.cross(&body_fixed_pos); + + Ok(Self { + observer_fixed_positions: body_fixed_pos, + observer_fixed_velocities: body_fixed_vel, + }) + } + + pub fn position(&self) -> &ObserverFixedPosition { + &self.observer_fixed_positions + } + + pub fn velocity(&self) -> &ObserverFixedVelocity { + &self.observer_fixed_velocities + } +} + +impl TryFrom<&Observer> for ObserverFixedCache { + type Error = OutfitError; + + fn try_from(resolved: &Observer) -> Result { + Self::new(resolved) + } +} + +/// Cache mapping observer IDs to their precomputed body-fixed positions and velocities. +pub type BodyFixedObserverCache = AHashMap; + +pub fn build_fixed_observer_cache<'a>( + observers: impl Iterator, +) -> Result { + observers + .map(|(id, obs)| -> Result<_, OutfitError> { Ok((id, obs.try_into()?)) }) + .collect::>() +} diff --git a/src/constants.rs b/src/constants.rs index 2b121d5..1e81aff 100644 --- a/src/constants.rs +++ b/src/constants.rs @@ -15,18 +15,12 @@ //! These definitions are used by all main modules, including orbit determination, observers, //! and ephemerides. -use crate::observations::Observation; -use crate::observers::Observer; -use smallvec::SmallVec; -use std::borrow::Cow; -use std::collections::HashMap; -use std::convert::TryFrom; -use std::sync::Arc; - // ------------------------------------------------------------------------------------------------- // Physical constants and unit conversions // ------------------------------------------------------------------------------------------------- +use nalgebra::{Matrix3, Vector3}; + /// 2π, useful for trigonometric conversions pub const DPI: f64 = 2. * std::f64::consts::PI; @@ -78,189 +72,39 @@ pub const VLIGHT: f64 = 2.99792458e5; /// Speed of light in astronomical units per day pub const VLIGHT_AU: f64 = VLIGHT / AU * SECONDS_PER_DAY; -// ------------------------------------------------------------------------------------------------- -// Type aliases -// ------------------------------------------------------------------------------------------------- - -/// Angle in degrees -pub type Degree = f64; -/// Angle in arcseconds -pub type ArcSec = f64; -/// Angle in radians -pub type Radian = f64; -/// Distance in kilometers -pub type Kilometer = f64; -/// Distance in meters -pub type Meter = f64; -/// MPC code identifying an observatory (3 characters) -pub type MpcCode = String; - -/// Lookup table from MPC code to [`Observer`] metadata -pub type MpcCodeObs = HashMap>; - -/// Modified Julian Date (days) -pub type MJD = f64; - -// ------------------------------------------------------------------------------------------------- -// Identifiers and data containers -// ------------------------------------------------------------------------------------------------- +// Angular velocity of Earth rotation (rad/day) on the z-axis. +pub const EARTH_ROTATION: Vector3 = Vector3::new(0.0, 0.0, DPI * 1.00273790934); -/// Identifier of a solar system object. +/// Rotation matrix from mean equatorial J2000 to mean ecliptic J2000. /// -/// This can be: -/// - An asteroid number (e.g. `Int(1234)`) -/// - A comet number (e.g. `"1234P"`) -/// - A provisional designation (e.g. `"K25D50B"`) -#[derive(Debug, Clone, PartialEq, Eq, Hash, PartialOrd, Ord)] -pub enum ObjectNumber { - /// Integer-based MPC designation (e.g. 1, 433…) - Int(u32), - /// String-based designation (provisional, comet, etc.) - String(String), -} - -impl std::fmt::Display for ObjectNumber { - fn fmt(&self, f: &mut std::fmt::Formatter<'_>) -> std::fmt::Result { - match self { - ObjectNumber::Int(n) => write!(f, "{n}"), - ObjectNumber::String(s) => write!(f, "{s}"), - } - } -} - -// --- Infallible conversions (enable `.into()` directly) ---------------------- - -impl From for ObjectNumber { - #[inline] - fn from(n: u32) -> Self { - ObjectNumber::Int(n) - } -} - -impl From for ObjectNumber { - #[inline] - fn from(n: u16) -> Self { - ObjectNumber::Int(n as u32) - } -} - -impl From for ObjectNumber { - #[inline] - fn from(n: u8) -> Self { - ObjectNumber::Int(n as u32) - } -} - -impl From<&u32> for ObjectNumber { - /// Convenience to allow `(&n).into()` without dereferencing at call sites. - #[inline] - fn from(n: &u32) -> Self { - ObjectNumber::Int(*n) - } -} - -impl From for ObjectNumber { - #[inline] - fn from(s: String) -> Self { - ObjectNumber::String(s) - } -} - -impl From<&String> for ObjectNumber { - /// Clones the string to build a `String`-backed identifier. - #[inline] - fn from(s: &String) -> Self { - ObjectNumber::String(s.clone()) - } -} - -impl From<&str> for ObjectNumber { - /// Note: this **does not** parse numeric strings into `Int`. Use `FromStr` if you want - /// `"1234"` to become `ObjectNumber::Int(1234)`. - #[inline] - fn from(s: &str) -> Self { - ObjectNumber::String(s.to_string()) - } -} - -impl<'a> From> for ObjectNumber { - /// Accept both borrowed and owned `Cow`. - #[inline] - fn from(c: Cow<'a, str>) -> Self { - match c { - Cow::Borrowed(s) => ObjectNumber::String(s.to_string()), - Cow::Owned(s) => ObjectNumber::String(s), - } - } -} - -// --- Fallible conversions (use `.try_into()` to be overflow-safe) ------------ - -impl TryFrom for ObjectNumber { - type Error = std::num::TryFromIntError; - - /// Convert a `usize` into `Int(u32)` if it fits. - #[inline] - fn try_from(n: usize) -> Result { - Ok(ObjectNumber::Int(u32::try_from(n)?)) - } -} - -impl TryFrom for ObjectNumber { - type Error = std::num::TryFromIntError; - - /// Convert a `u64` into `Int(u32)` if it fits. - #[inline] - fn try_from(n: u64) -> Result { - Ok(ObjectNumber::Int(u32::try_from(n)?)) - } -} - -impl TryFrom for ObjectNumber { - type Error = &'static str; - - /// Convert a non-negative `i64` into `Int(u32)` if it fits. - #[inline] - fn try_from(n: i64) -> Result { - if n < 0 { - return Err("negative value is not a valid ObjectNumber::Int"); - } - let n = u64::try_from(n).map_err(|_| "conversion failed")?; - let n = u32::try_from(n).map_err(|_| "value exceeds u32 range")?; - Ok(ObjectNumber::Int(n)) - } -} - -// --- Smart parsing from &str via `FromStr` (optional) ------------------------ - -impl std::str::FromStr for ObjectNumber { - type Err = std::num::ParseIntError; - - /// Try to parse an `ObjectNumber` from a string. - /// - /// Rules - /// ----- - /// - Pure digits that fit in `u32` → `Int(u32)`. - /// - Otherwise → `String(String)`. - /// - /// Note - /// ---- - /// If the string is *only* digits but **does not** fit in `u32`, this returns the - /// original `ParseIntError`. If you prefer to always fallback to `String` on - /// overflow, we can change the policy (but it’s usually better to fail loudly). - fn from_str(s: &str) -> Result { - match s.parse::() { - Ok(n) => Ok(ObjectNumber::Int(n)), - Err(e) => { - if s.chars().any(|c| !c.is_ascii_digit()) { - Ok(ObjectNumber::String(s.to_string())) - } else { - Err(e) - } - } - } - } -} - -/// A small, inline-optimized container for observations of a single object. -pub type Observations = SmallVec<[Observation; 6]>; +/// Rotation of $-\varepsilon$ around the X-axis, where $\varepsilon$ is the +/// obliquity of the ecliptic at J2000. +pub const ROT_EQUMJ2000_TO_ECLMJ2000: Matrix3 = Matrix3::new( + 1.00000000000000000e0, + 0.00000000000000000e0, + 0.00000000000000000e0, + 0.00000000000000000e0, + 9.17482062069181814e-1, + -3.97777155931913706e-1, + 0.00000000000000000e0, + 3.97777155931913706e-1, + 9.17482062069181814e-1, +); + +/// Rotation matrix from mean ecliptic J2000 to mean equatorial J2000. +/// +/// Transpose (inverse) of [`ROT_EQUMJ2000_TO_ECLMJ2000`]. +pub const ROT_ECLMJ2000_TO_EQUMJ2000: Matrix3 = Matrix3::new( + 1.00000000000000000e0, + 0.00000000000000000e0, + 0.00000000000000000e0, + 0.00000000000000000e0, + 9.17482062069181814e-1, + 3.97777155931913706e-1, + 0.00000000000000000e0, + -3.97777155931913706e-1, + 9.17482062069181814e-1, +); + +/// Modified Julian Date (Scale Ephemeris Time, ET) +pub type MJDET = f64; diff --git a/src/conversion.rs b/src/conversion.rs index 25a19c4..dc20ac5 100644 --- a/src/conversion.rs +++ b/src/conversion.rs @@ -83,9 +83,11 @@ //! - MPC/ADES ingestion modules where these utilities are typically used. use std::f64::consts::TAU; -use nalgebra::Vector3; +use nalgebra::{Matrix3, Vector3}; +use ordered_float::{FloatIsNan, NotNan}; +use photom::{coordinates::cartesian::CartesianCoord, Arcseconds, Degrees, Radians}; -use crate::constants::{ArcSec, Degree, Radian, DPI}; +use crate::constants::DPI; /// Estimate the accuracy of a numeric string based on its decimal precision. /// @@ -118,7 +120,7 @@ fn compute_accuracy(field: &str, factor: f64) -> Option { /// ---------- /// * Angle in **radians** (`Radian`). #[inline] -pub fn arcsec_to_rad(arcsec: ArcSec) -> Radian { +pub fn arcsec_to_rad(arcsec: Arcseconds) -> Radians { (arcsec / 3600.0).to_radians() } @@ -153,7 +155,7 @@ pub fn arcsec_to_rad(arcsec: ArcSec) -> Radian { /// /// # See also /// * [`parse_dec_to_deg`] – Parses declination strings into degrees. -pub fn parse_ra_to_deg(ra: &str) -> Option<(Degree, ArcSec)> { +pub fn parse_ra_to_deg(ra: &str) -> Option<(Degrees, Arcseconds)> { let parts: Vec<&str> = ra.split_whitespace().collect(); if parts.len() != 3 { return None; @@ -200,7 +202,7 @@ pub fn parse_ra_to_deg(ra: &str) -> Option<(Degree, ArcSec)> { /// /// # See also /// * [`parse_ra_to_deg`] – Parses right ascension strings into degrees. -pub fn parse_dec_to_deg(dec: &str) -> Option<(Degree, ArcSec)> { +pub fn parse_dec_to_deg(dec: &str) -> Option<(Degrees, Arcseconds)> { let parts: Vec<&str> = dec.split_whitespace().collect(); if parts.len() != 3 { return None; @@ -445,6 +447,63 @@ pub fn cartesian_to_radec(cartesian_position: Vector3) -> (f64, f64, f64) { (alpha, delta, pos_norm) } +pub trait ToNotNan { + type Output; + fn to_notnan(self) -> Result; +} + +impl ToNotNan for f64 { + type Output = NotNan; + fn to_notnan(self) -> Result { + NotNan::new(self) + } +} + +impl ToNotNan for Vector3 { + type Output = Vector3>; + fn to_notnan(self) -> Result { + Ok(Vector3::new( + self.x.to_notnan()?, + self.y.to_notnan()?, + self.z.to_notnan()?, + )) + } +} + +impl ToNotNan for Matrix3 { + type Output = Matrix3>; + fn to_notnan(self) -> Result { + Ok(Matrix3::new( + self[(0, 0)].to_notnan()?, + self[(0, 1)].to_notnan()?, + self[(0, 2)].to_notnan()?, + self[(1, 0)].to_notnan()?, + self[(1, 1)].to_notnan()?, + self[(1, 2)].to_notnan()?, + self[(2, 0)].to_notnan()?, + self[(2, 1)].to_notnan()?, + self[(2, 2)].to_notnan()?, + )) + } +} + +/// Convert a Cartesian position vector to a `CartesianCoord`. +/// +/// # Arguments +/// +/// - `vec`: A 3D vector representing the Cartesian coordinates (x, y, z). +/// +/// # Returns +/// +/// - A `CartesianCoord` struct with fields `x`, `y`, and `z` populated from the input vector. +pub fn cartesion_from_vec(vec: Vector3) -> CartesianCoord { + CartesianCoord { + x: vec[0], + y: vec[1], + z: vec[2], + } +} + #[cfg(test)] mod observations_test { use super::*; diff --git a/src/earth_orientation.rs b/src/earth_orientation.rs index cef0bbc..a674ee4 100644 --- a/src/earth_orientation.rs +++ b/src/earth_orientation.rs @@ -74,9 +74,10 @@ //! - [`crate::ref_system`] for frame transformations that use these models. //! - **Theory of Orbit Determination** by Milani & Gronchi (2010). use nalgebra::Matrix3; +use photom::{Arcseconds, Radians, MJDTT}; use crate::{ - constants::{ArcSec, Radian, RADEG, RADSEC, T2000}, + constants::{RADEG, RADSEC, T2000}, ref_system::rotmt, }; @@ -115,7 +116,7 @@ use crate::{ /// # See also /// * [`rotmt`] – constructs rotation matrices using this obliquity /// * [`rotpn`](crate::ref_system::rotpn) – applies obliquity rotation when transforming between ecliptic and equatorial frames -pub fn obleq(tjm: f64) -> Radian { +pub fn obleq(tjm: MJDTT) -> Radians { // Obliquity coefficients let ob0 = ((23.0 * 3600.0 + 26.0 * 60.0) + 21.448) * RADSEC; let ob1 = -46.815 * RADSEC; @@ -166,7 +167,7 @@ pub fn obleq(tjm: f64) -> Radian { /// * [`rnut80`] – uses these angles to build the nutation rotation matrix /// * [`rotpn`](crate::ref_system::rotpn) – applies nutation when transforming between Equt and Equm systems #[inline(always)] -pub fn nutn80(tjm: f64) -> (ArcSec, ArcSec) { +pub fn nutn80(tjm: MJDTT) -> (Arcseconds, Arcseconds) { // ---- time powers (Julian centuries from J2000) let t = (tjm - T2000) / 36525.0; let t2 = t * t; @@ -455,7 +456,7 @@ pub fn nutn80(tjm: f64) -> (ArcSec, ArcSec) { /// * [`obleq`] – computes the mean obliquity ε (radians) /// * [`rotmt`] – builds the individual axis rotation matrices /// * [`rotpn`](crate::ref_system::rotpn) – uses `rnut80` to transform between Equm and Equt systems -pub fn rnut80(tjm: f64) -> Matrix3 { +pub fn rnut80(tjm: MJDTT) -> Matrix3 { // Mean obliquity of the ecliptic at date (ε) let epsm = obleq(tjm); @@ -504,7 +505,7 @@ pub fn rnut80(tjm: f64) -> Matrix3 { /// # See also /// * [`obleq`] – Computes the mean obliquity of the ecliptic. /// * [`nutn80`] – Computes the 1980 IAU nutation model (Δψ and Δε). -pub fn equequ(tjm: f64) -> f64 { +pub fn equequ(tjm: MJDTT) -> Radians { // Compute the mean obliquity of the ecliptic (ε, in radians) let oblm = obleq(tjm); @@ -557,7 +558,7 @@ pub fn equequ(tjm: f64) -> f64 { /// # See also /// * [`rotmt`] – constructs the rotation matrices used here /// * [`rotpn`](crate::ref_system::rotpn) – uses `prec` when converting between epochs `"OFDATE"` and `"J2000"` -pub fn prec(tjm: f64) -> Matrix3 { +pub fn prec(tjm: MJDTT) -> Matrix3 { // Precession polynomial coefficients (in radians) let zed = 0.6406161 * RADEG; let zd = 0.6406161 * RADEG; diff --git a/src/env_state.rs b/src/env_state.rs deleted file mode 100644 index 67bb706..0000000 --- a/src/env_state.rs +++ /dev/null @@ -1,127 +0,0 @@ -//! # Outfit environment state -//! -//! This module defines [`crate::env_state::OutfitEnv`], the **shared environment object** used across -//! the `Outfit` library. It provides access to: -//! -//! - A persistent **HTTP client** (for downloading ephemerides, observatory lists, etc.). -//! - A **UT1 provider** from [hifitime](https://docs.rs/hifitime) to handle Earth rotation -//! parameters from JPL. -//! -//! This object is designed to be **cheaply cloneable** and passed to algorithms -//! that require access to external data sources or Earth orientation models. -//! -//! ## Overview -//! -//! The main responsibilities of `OutfitEnv` are: -//! -//! 1. Manage a global [`ureq::Agent`] HTTP client with sensible default settings. -//! 2. Download and initialize an [`hifitime::ut1::Ut1Provider`] from JPL’s `latest_eop2.long` file -//! (Earth orientation parameters) at startup. -//! 3. Provide simple utilities for performing HTTP GET requests. -//! -//! ## Structure -//! -//! ```text -//! OutfitEnv -//! ├── http_client (ureq::Agent) -//! └── ut1_provider (hifitime::Ut1Provider) -//! ``` -//! -//! ## Usage -//! -//! ```rust,ignore -//! use outfit::env_state::OutfitEnv; -//! -//! // Create a new environment (downloads UT1 data from JPL) -//! let env = OutfitEnv::new(); -//! -//! // Access the UT1 provider -//! let ut1 = &env.ut1_provider; -//! -//! // Make a GET request using the built-in HTTP client -//! let response = env.get_from_url("https://ssd.jpl.nasa.gov/api/horizons.api"); -//! println!("Response: {}", &response[..100.min(response.len())]); -//! ``` -//! -//! ## Notes -//! -//! - The [`crate::env_state::OutfitEnv`] struct is meant to be reused and shared between different -//! parts of the crate to avoid redundant downloads and HTTP session creation. -//! - The UT1 provider is initialized once at startup; if fresh data is needed, -//! the library must be restarted or the provider re-downloaded manually. -//! -//! ## See also -//! -//! - [`hifitime::ut1::Ut1Provider`] – Manages Earth orientation and UT1 corrections. -//! - [`ureq::Agent`] – Minimal HTTP client used internally. -use hifitime::ut1::Ut1Provider; -use std::convert::TryFrom; -use std::{fmt::Debug, time::Duration}; -use ureq::{ - http::{self, Uri}, - Agent, -}; - -/// This object is passed to the various functions in the library -/// to provide access to the state of the library -/// -/// # Fields -/// -/// * `http_client` - A reqwest client used to make HTTP requests -/// * `ut1_provider` - A provider used to get the current UT1 time -/// * `observatories` - A lazy map of observatories from the Minor Planet Center. -/// The key is the MPC code and the value is the observer -#[derive(Debug, Clone)] -pub struct OutfitEnv { - pub http_client: Agent, - pub ut1_provider: Ut1Provider, -} - -impl Default for OutfitEnv { - fn default() -> Self { - Self::new() - } -} - -impl OutfitEnv { - /// Create a new Outfit object - /// - /// Return - /// ------ - /// * A new Outfit object - /// - The UT1 provider is downloaded from the JPL - /// - The HTTP client is created with default settings - /// - The observatories are lazily loaded from the Minor Planet Center - pub fn new() -> Self { - let ut1_provider = OutfitEnv::initialize_ut1_provider(); - - let config = Agent::config_builder() - .timeout_global(Some(Duration::from_secs(10))) - .build(); - let agent: Agent = config.into(); - - OutfitEnv { - http_client: agent, - ut1_provider, - } - } - - fn initialize_ut1_provider() -> Ut1Provider { - Ut1Provider::download_from_jpl("latest_eop2.long") - .expect("Download of the JPL short time scale UT1 data failed") - } - - pub(crate) fn get_from_url(&self, url: U) -> String - where - Uri: TryFrom, - >::Error: Into, - { - self.http_client - .get(url) - .call() - .expect("Get request failed") - .body_mut() - .read_to_string() - .expect("Failed to read response body") - } -} diff --git a/src/error_models/data_models/cbm10.rules b/src/error_models/data_models/cbm10.rules deleted file mode 100644 index 5942367..0000000 --- a/src/error_models/data_models/cbm10.rules +++ /dev/null @@ -1,64 +0,0 @@ -! obscods catal rms(acosd) rmsd (arcsec) -699:c @ 0.93, 0.78 -608:c @ 1.26, 1.53 -644:c @ 0.47, 0.56 -106:c @ 1.02, 0.79 -D29:c @ 0.66, 0.59 -689:c @ 0.51, 0.63 -ALL:cc @ 1.02, 0.79 -ALL:cd @ 1.02, 0.79 -ALL:ce @ 0.66, 0.59 -ALL:cq @ 0.66, 0.59 -ALL:cr @ 0.66, 0.59 -ALL:ct @ 0.66, 0.59 -ALL:cu @ 0.66, 0.59 -ALL:co @ 0.99, 0.81 -ALL:cs @ 0.99, 0.81 -ALL:ca @ 1.17, 1.02 -ALL:cb @ 1.17, 1.02 -ALL:ch @ 0.90, 0.88 -ALL:ci @ 0.90, 0.88 -ALL:cj @ 0.90, 0.88 -ALL:cz @ 0.90, 0.88 -ALL:cm @ 1.11, 1.13 -ALL:cw @ 0.88, 0.71 -ALL:cf @ 1.45, 1.27 -ALL:cg @ 1.45, 1.27 -ALL:cL @ 0.50, 0.50 -704:cc @ 1.23, 1.19 -699:cc @ 0.93, 0.78 -691:cc @ 0.63, 0.68 -608:cc @ 1.26, 1.53 -703:cc @ 1.23, 1.13 -644:cc @ 0.47, 0.56 -703:ce @ 0.97, 0.91 -G96:ce @ 0.50, 0.42 -E12:ce @ 0.82, 0.85 -683:ce @ 1.21, 1.55 -699:co @ 0.84, 0.81 -644:co @ 0.36, 0.33 -691:co @ 0.50, 0.56 -704:cd @ 1.23, 1.19 -699:cd @ 0.93, 0.78 -691:cd @ 0.63, 0.68 -608:cd @ 1.26, 1.53 -703:cd @ 1.23, 1.13 -644:cd @ 0.47, 0.56 -703:cr @ 0.97, 0.91 -G96:cr @ 0.50, 0.42 -E12:cr @ 0.82, 0.85 -683:cr @ 1.21, 1.55 -699:cs @ 0.84, 0.81 -644:cs @ 0.36, 0.33 -691:cs @ 0.50, 0.56 -689:cg @ 0.51, 0.63 -645:ce @ 0.30, 0.30 -F51:cL @ 0.30, 0.30 -F51:ct @ 0.30, 0.30 -C51:cL @ 1.00, 1.00 -568:cL @ 0.30, 0.30 -568:ct @ 0.25, 0.25 -568:co @ 0.50, 0.50 -568:cs @ 0.50, 0.50 -W84:co @ 0.30, 0.30 -W84:cL @ 0.30, 0.30 \ No newline at end of file diff --git a/src/error_models/data_models/fcct14.rules b/src/error_models/data_models/fcct14.rules deleted file mode 100644 index 43369dc..0000000 --- a/src/error_models/data_models/fcct14.rules +++ /dev/null @@ -1,48 +0,0 @@ -ALL: c=cd @ 0.51, 0.40 ! CBM Generic Catalog weights -ALL: c=eqru @ 0.33, 0.30 -ALL: c=tL @ 0.25, 0.25 -ALL: c=os @ 0.50, 0.41 -ALL: c=ab @ 0.59, 0.51 -ALL: c=hijz @ 0.45, 0.44 -ALL: c=m @ 0.56, 0.57 -ALL: c=w @ 0.44, 0.36 -ALL: c=fg @ 0.73, 0.64 -ALL: c=UV @ 0.60, 0.60 -258: c=* @ 0.10, 0.10 -704: c=cd @ 0.62, 0.60 ! CBM Station-Catalog specific rules -699: c=cd @ 0.47, 0.39 -691: c=cd @ 0.32, 0.34 -608: c=cd @ 0.63, 0.77 -703: c=cd @ 0.62, 0.57 -644: c=cd @ 0.24, 0.28 -703: c=er @ 0.49, 0.46 -G96: c=erUV @ 0.25, 0.21 -E12: c=er @ 0.41, 0.43 -683: c=er @ 0.61, 0.78 -699: c=os @ 0.42, 0.41 -644: c=os @ 0.18, 0.17 -691: c=os @ 0.25, 0.28 -689: c=g @ 0.26, 0.32 -645: c=e @ 0.15, 0.15 ! New rules -F51: c=Lt @ 0.15, 0.15 -F51: c=UV @ 0.15, 0.15 -F52: c=Lt @ 0.15, 0.15 -F52: c=UV @ 0.15, 0.15 -568: c=L @ 0.15, 0.15 -568: c=t @ 0.13, 0.13 -568: c=os @ 0.25, 0.25 -568: c=UV @ 0.10, 0.10 -309: c=UV @ 0.15, 0.15 -H01: c=Lt @ 0.15, 0.15 -I41: c=UV @ 0.20, 0.20 -I41: c=N @ 0.40, 0.40 -673: c=* @ 0.30, 0.30 ! TMO -G45: c=* @ 0.50, 0.50 ! Space Survelliance Telescope -250: c=* @ 1.30, 1.30 ! Satellites: HST -249: c=* @ 60.0, 60.0 ! SOHO -C49: c=* @ 60.0, 60.0 ! STEREO-A -C50: c=* @ 60.0, 60.0 ! STEREO-B -C51: c=* @ 1.00, 1.00 ! WISE -T12: c=UV @ 0.10, 0.10 ! Tholen from UH88 with Gaia catalog -T09: c=UV @ 0.10, 0.10 ! Tholen from Subaru with Gaia catalog -T14: c=UV @ 0.10, 0.10 ! Tholen from CFHT with Gaia catalog diff --git a/src/error_models/data_models/vfcc17.rules b/src/error_models/data_models/vfcc17.rules deleted file mode 100644 index 1942c9f..0000000 --- a/src/error_models/data_models/vfcc17.rules +++ /dev/null @@ -1,100 +0,0 @@ -ALL t=PAN c=* p= > < 1890-01-01 @ 10.00, 10.00 -ALL t=PAN c=* p= > 1890-01-01 < 1950-01-01 @ 5.00, 5.00 -ALL t=PAN c=* p= > 1950-01-01 < @ 2.50, 2.50 -ALL t=cBCVn c=* p= > < @ 1.00, 1.00 ! Unknown catalog -ALL t=E c=* p= > < @ 0.20, 0.20 ! Occultations -ALL t=H c=* p= > < @ 0.40, 0.40 ! Hipparcos -ALL t=T c=* p= > < @ 0.50, 0.50 ! Transit circle -ALL t=e c=* p= > < @ 0.75, 0.75 ! Encoder -ALL t=M c=* p= > < @ 3.00, 3.00 ! Micrometer -ALL t=S c=* p= > < @ 1.50, 1.50 ! Satellite -ALL t=cC c=UVXW p= > < @ 0.60, 0.60 ! Gaia astrometric catalogs -F51 t=cC c=* p= > < @ 0.20, 0.20 -F52 t=cC c=* p= > < @ 0.20, 0.20 -G96 t=cC c=* p= > < @ 0.50, 0.50 -703 t=cC c=* p= > < 2014-01-01 @ 1.00, 1.00 -703 t=cC c=* p= > 2014-01-01 < @ 0.80, 0.80 -E12 t=cC c=* p= > < @ 0.75, 0.75 -704 t=cC c=* p= > < @ 1.00, 1.00 -691 t=cC c=* p= > < 2003-01-01 @ 0.60, 0.60 -691 t=cC c=* p= > 2003-01-01 < @ 0.50, 0.50 -291 t=cC c=* p= > < 2003-01-01 @ 0.60, 0.60 ! Updated -291 t=cC c=* p= > 2003-01-01 < @ 0.50, 0.50 ! Updated -644 t=cC c=* p= > < 2003-09-01 @ 0.60, 0.60 -644 t=cC c=* p= > 2003-09-01 < @ 0.40, 0.40 -699 t=cC c=* p= > < @ 0.80, 0.80 -G45 t=cC c=* p= > < @ 0.60, 0.60 -D29 t=cC c=* p= > < @ 0.75, 0.75 -T05 t=cC c=* p= > < @ 0.80, 0.80 -568 t=cC c=* p= > < @ 0.50, 0.50 ! Generic -568 t=cC c=t p=_ > < @ 0.20, 0.20 ! Micheli updated -568 t=cC c=q p=_ > < @ 0.20, 0.20 ! Micheli updated -568 t=cC c=UVXW p=_ > < @ 0.10, 0.10 ! Micheli updated -568 t=cC c=t p=2 > < @ 0.20, 0.20 ! Tholen -568 t=cC c=UVXW p=2 > < @ 0.10, 0.10 ! Tholen -568 t=cC c=os p=2 > < @ 0.50, 0.50 ! Tholen -568 t=cC c=UVXW p=^ > < @ 0.20, 0.20 ! Weryk new -T09 t=cC c=* p= > < @ 0.50, 0.50 ! Generic -T09 t=cC c=t p=0 > < @ 0.20, 0.20 ! Tholen -T09 t=cC c=UVX p=0 > < @ 0.10, 0.10 ! Tholen -T12 t=cC c=* p= > < 2022-10-06 @ 0.10, 0.10 ! Tholen Before 06 October 2022 -T12 t=cC c=* p= > 2022-10-06 < @ 0.50, 0.50 ! Generic New program codes, see MPEC 2022-T98 -T12 t=cC c=t p=0 > < 2022-10-06 @ 0.10, 0.10 ! Tholen Before 06 October 2022 -T12 t=cC c=t p=0 > 2022-10-06 < @ 0.20, 0.20 ! Tholen New program codes -T12 t=cC c=UVX p=0 > < 2022-10-06 @ 0.10, 0.10 ! Tholen Before 06 October 2022 -T12 t=cC c=UVX p=0 > 2022-10-06 < @ 0.10, 0.10 ! Tholen New program codes -T12 t=cC c=UVX p=1 > < 2022-10-06 @ 0.10, 0.10 ! Tholen Before 06 October 2022 -T12 t=cC c=UVX p=1 > 2022-10-06 < @ 0.20, 0.20 ! Weryk new New program code -T14 t=cC c=* p= > < @ 0.50, 0.50 ! Generic -T14 t=cC c=t p=0 > < @ 0.20, 0.20 ! Tholen -T14 t=cC c=UVX p=0 > < @ 0.10, 0.10 ! Tholen -T14 t=cC c=t p=7 > < @ 0.20, 0.20 ! Micheli updated -T14 t=cC c=UVX p=7 > < @ 0.10, 0.10 ! Micheli updated -T14 t=cC c=UVX p=3 > < @ 0.20, 0.20 ! Weryk new -H01 t=cC c=LtUVXW p= > < @ 0.30, 0.30 -673 t=cC c=* p= > < @ 0.30, 0.30 -645 t=cC c=* p= > < @ 0.30, 0.30 -689 t=cC c=* p= > < @ 0.50, 0.50 -J04 t=cC c=UVXWtLqrue p= > < @ 0.40, 0.40 ! Updated -Z84 t=cC c=UVXWtLqrue p= > < @ 0.40, 0.40 ! New -W84 t=cC c=* p= > < @ 0.50, 0.50 -950 t=cC c=UVXWtLqrue p= > < @ 0.50, 0.50 -F65 t=cC c=* p= > < @ 0.40, 0.40 -E10 t=cC c=* p= > < @ 0.40, 0.40 -W85 t=cC c=* p= > < @ 0.40, 0.40 -W86 t=cC c=* p= > < @ 0.40, 0.40 -W87 t=cC c=* p= > < @ 0.40, 0.40 -Q63 t=cC c=* p= > < @ 0.40, 0.40 -Q64 t=cC c=* p= > < @ 0.40, 0.40 -K91 t=cC c=* p= > < @ 0.40, 0.40 -K92 t=cC c=* p= > < @ 0.40, 0.40 -K93 t=cC c=* p= > < @ 0.40, 0.40 -V37 t=cC c=* p= > < @ 0.40, 0.40 -V39 t=cC c=* p= > < @ 0.40, 0.40 ! New -Z31 t=cC c=* p= > < @ 0.40, 0.40 ! New -Z24 t=cC c=* p= > < @ 0.40, 0.40 ! New -Y28 t=cC c=tUVXW p= > < 2015-01-01 @ 1.00, 1.00 ! New -Y28 t=cC c=tUVXW p= > 2015-01-01 < @ 0.30, 0.30 ! New -309 t=cC c=UVXW p=&% > < @ 0.20, 0.20 -309 t=cC c=tq p=&% > < @ 0.30, 0.30 -G83 t=cC c=UVXW p=2 > < @ 0.20, 0.20 -G83 t=cC c=tq p=2 > < @ 0.30, 0.30 -248 t=* c=* p= > < 1991-01-01 @ 0.20, 0.20 ! Hipparcos -248 t=* c=* p= > 1991-01-01 < @ 0.15, 0.15 ! Hipparcos -250 t=* c=* p= > < @ 1.30, 1.30 ! HST -249 t=* c=* p= > < @ 60.00, 60.00 ! SOHO -C49 t=* c=* p= > < @ 60.00, 60.00 ! STEREO-A -C50 t=* c=* p= > < @ 60.00, 60.00 ! STEREO-B -C51 t=* c=* p= > < @ 1.00, 1.00 ! WISE -C57 t=* c=* p= > < @ 5.00, 5.00 ! TESS -608 t=cC c=* p= > < @ 0.60, 0.60 ! New -Z18 t=cC c=tq p=1 > < @ 0.30, 0.30 ! Micheli New -Z18 t=cC c=UVXW p=1 > < @ 0.20, 0.20 ! Micheli New -T08 t=cC c=* p= > < @ 0.80, 0.80 ! New -258 t=cC c=* p= > < @ 0.50, 0.50 ! GAIA new -C65 t=cC c=UVXW p=3 > < @ 0.20, 0.20 ! Micheli new -094 t=cC c=UVXW p=9 > < @ 0.50, 0.50 ! Micheli new -181 t=cC c=UVXW p= > < 2019-01-01 @ 1.00, 1.00 ! New -181 t=cC c=UVXW p= > 2019-01-01 < @ 0.50, 0.50 ! New -M28 t=* c=* p= > < 2023-12-12 @ 3.00, 3.00 ! Bad observations from M28, biased fixed on Dec. 2023 -M28 t=* c=* p= > 2023-12-12 < @ 1.00, 1.00 ! Restore default RMS for M28 diff --git a/src/error_models/mod.rs b/src/error_models/mod.rs deleted file mode 100644 index aa00ffa..0000000 --- a/src/error_models/mod.rs +++ /dev/null @@ -1,418 +0,0 @@ -//! # Astrometric error models -//! -//! This module provides tools to **handle observation error models** used in orbit -//! determination. Error models define the astrometric biases and RMS values -//! associated with each observatory and star catalog, as recommended in the literature -//! (e.g., FCCT14, CBM10, VFCC17). -//! -//! ## Public API -//! -//! ### [`crate::error_models::ErrorModel`] -//! Enumeration of the supported astrometric error models: -//! -//! - `ErrorModel::FCCT14` – Farnocchia, Chesley, Chamberlin & Tholen (2014) -//! - `ErrorModel::CBM10` – Chesley, Baer & Monet (2010) -//! - `ErrorModel::VFCC17` – Vereš, Farnocchia, Chesley & Chamberlin (2017) -//! -//! You can create an [`crate::error_models::ErrorModel`] from a string with: -//! -//! ```rust, ignore -//! use outfit::error_models::ErrorModel; -//! let model: ErrorModel = "FCCT14".parse().unwrap(); -//! ``` -//! -//! ### [`crate::error_models::ErrorModelData`] -//! -//! ```text -//! type ErrorModelData = HashMap<(MpcCode, CatalogCode), (f32, f32)> -//! ``` -//! -//! This map associates an observatory (MPC code) and a star catalog code -//! with a pair `(bias_RMS, declination_RMS)`. -//! -//! The contents are loaded from reference files distributed with the crate. -//! -//! ### `ErrorModel::read_error_model_file` -//! -//! ```rust, ignore -//! use outfit::error_models::ErrorModel; -//! -//! let error_map = ErrorModel::FCCT14.read_error_model_file().unwrap(); -//! println!("{} entries", error_map.len()); -//! ``` -//! -//! This function reads the internal rules for the chosen model -//! and returns a [`crate::error_models::ErrorModelData`] structure ready to be queried. -//! -//! ### [`crate::error_models::get_bias_rms`] -//! -//! ```rust -//! use outfit::error_models::{ErrorModel, get_bias_rms}; -//! -//! let data = ErrorModel::FCCT14.read_error_model_file().unwrap(); -//! if let Some((bias_ra, bias_dec)) = get_bias_rms(&data, "699".to_string(), "c".to_string()) { -//! println!("Bias for MPC 699: RA = {bias_ra}, Dec = {bias_dec}"); -//! } -//! ``` -//! -//! This function looks up the `(RMS in RA, RMS in Dec)` for a given observatory -//! and star catalog code. If no exact match is found, the function falls back to -//! generic values (e.g. `ALL:c`). -//! -//! ## Typical usage -//! -//! 1. Choose an error model (e.g. `ErrorModel::FCCT14`). -//! 2. Load its table using [`read_error_model_file`](crate::error_models::ErrorModel::read_error_model_file). -//! 3. Use [`crate::error_models::get_bias_rms`] to obtain astrometric uncertainties for weighting residuals. -//! -//! ## References -//! -//! - Farnocchia, D., Chesley, S. R., Chamberlin, A. B., & Tholen, D. J. (2014) -//! - Chesley, S. R., Baer, J., & Monet, D. G. (2010) -//! - Vereš, P., Farnocchia, D., Chesley, S. R., & Chamberlin, A. B. (2017) -//! -//! These tables are essential for **realistic orbit determination** since they -//! ensure that observations are weighted according to their expected precision. -mod vfcc17; - -use std::{collections::HashMap, str::FromStr}; - -use nom::{ - branch::alt, - bytes::complete::{tag, take_until, take_while}, - character::complete::{char, multispace0}, - combinator::{map, opt}, - number::complete::float, - sequence::{preceded, separated_pair, terminated}, - IResult, Parser, -}; - -use crate::{constants::MpcCode, outfit_errors::OutfitError}; -use vfcc17::parse_vfcc17_line; - -type CatalogCode = String; -pub type ErrorModelData = HashMap<(MpcCode, CatalogCode), (f32, f32)>; - -#[derive(Debug, Clone, Copy, PartialEq, Eq, Hash)] -pub enum ErrorModel { - FCCT14, - CBM10, - VFCC17, -} - -static FCCT14_RULES: &str = include_str!("data_models/fcct14.rules"); -static CBM10_RULES: &str = include_str!("data_models/cbm10.rules"); -static VFCC17_RULES: &str = include_str!("data_models/vfcc17.rules"); - -pub(in crate::error_models) type ParseResult<'a> = - IResult<&'a str, Vec<((MpcCode, CatalogCode), (f32, f32))>>; - -fn is_alphanum(c: char) -> bool { - c.is_alphanumeric() -} - -fn parse_station(input: &str) -> IResult<&str, &str> { - terminated(take_while(is_alphanum), tag(":")).parse(input) -} - -fn parse_rms_values(input: &str) -> IResult<&str, (f32, f32)> { - preceded( - multispace0, - preceded( - char('@'), - separated_pair( - preceded(multispace0, float), - char(','), - preceded(multispace0, float), - ), - ), - ) - .parse(input) -} - -fn parse_catalog_codes(input: &str) -> IResult<&str, Vec> { - preceded( - multispace0, - preceded( - // accepte soit "c=" soit rien du tout - alt((tag("c="), tag(""))), - map( - nom::bytes::complete::take_while(|c: char| c.is_alphabetic() || c == '*'), - |s: &str| s.chars().map(|c| c.to_string()).collect(), - ), - ), - ) - .parse(input) -} - -fn parse_full_line(input: &str) -> ParseResult { - let (input, remain) = opt(take_until("!")).parse(input)?; //ignore comments - let input = input.trim(); - - let input = remain.unwrap_or(input); - - map( - (parse_station, parse_catalog_codes, parse_rms_values), - |(station, catalogs, (rmsa, rmsd))| { - catalogs - .into_iter() - .map(|cat| ((station.to_string(), cat), (rmsa, rmsd))) - .collect() - }, - ) - .parse(input) -} - -fn parse_full_file(file: &str, parse_line: F) -> Result -where - F: Fn(&str) -> ParseResult, -{ - let error_map: ErrorModelData = file - .lines() - .filter(|line| !line.trim().is_empty() && !line.trim_start().starts_with('!')) - .map(|line| { - parse_line(line) - .map_err(|_e| OutfitError::NomParsingError(line.to_string())) - .map(|(_, pairs)| pairs) - }) - .collect::, OutfitError>>()? - .into_iter() - .flatten() - .collect(); - - Ok(error_map) -} - -impl ErrorModel { - /// Load the internal RMS/bias table for this astrometric error model. - /// - /// This function parses the reference file corresponding to the selected - /// [`ErrorModel`] variant (FCCT14, CBM10, or VFCC17) and returns a - /// [`ErrorModelData`] map containing the weighting coefficients - /// (RMS in right ascension and declination). - /// - /// # Returns - /// - /// A [`Result`] containing: - /// * `Ok(ErrorModelData)` – A hash map where each key is a pair `(MpcCode, CatalogCode)` - /// and the value is a tuple `(rms_ra, rms_dec)` in arcseconds. - /// * `Err(OutfitError)` – If the reference file could not be parsed. - /// - /// # Usage - /// - /// ``` - /// use outfit::error_models::ErrorModel; - /// - /// // Load FCCT14 error model data - /// let data = ErrorModel::FCCT14.read_error_model_file().unwrap(); - /// - /// println!("Number of entries: {}", data.len()); - /// - /// // Use the map later with `get_bias_rms` - /// ``` - /// - /// # See also - /// * [`get_bias_rms`] – Look up the bias and RMS values for a given station/catalog. - pub fn read_error_model_file(&self) -> Result { - let error_map: ErrorModelData = match self { - ErrorModel::FCCT14 => parse_full_file(FCCT14_RULES, parse_full_line)?, - ErrorModel::CBM10 => parse_full_file(CBM10_RULES, parse_full_line)?, - ErrorModel::VFCC17 => { - // Implement parsing logic for VFCC17 - parse_full_file(VFCC17_RULES, parse_vfcc17_line)? - } - }; - - Ok(error_map) - } -} - -impl FromStr for ErrorModel { - type Err = OutfitError; - - fn from_str(s: &str) -> Result { - match s { - "FCCT14" => Ok(ErrorModel::FCCT14), - "CBM10" => Ok(ErrorModel::CBM10), - "VFCC17" => Ok(ErrorModel::VFCC17), - _ => Err(OutfitError::InvalidErrorModel(format!( - "Invalid error model: {s}" - ))), - } - } -} - -/// Retrieve the astrometric bias and RMS values for a given observatory (MPC code) -/// and star catalog code from a preloaded [`ErrorModelData`] table. -/// -/// This function searches for a matching entry in the following priority order: -/// -/// 1. **Exact match**: `(mpc_code, catalog_code)` -/// 2. **Generic catalog fallback for the same observatory**: -/// * `(mpc_code, "e")` – generic `e` entry (elliptical) -// * `(mpc_code, "c")` – generic `c` entry (catalog-specific default) -/// 3. **Global fallback** (for any observatory): -/// * `("ALL", catalog_code)` -/// * `("ALL", "e")` -/// * `("ALL", "c")` -/// -/// The returned pair `(rms_ra, rms_dec)` corresponds to the weighting factors -/// (typically in arcseconds) used for astrometric residuals. -/// -/// # Arguments -/// -/// * `error_model` – The [`ErrorModelData`] hash map produced by -/// [`ErrorModel::read_error_model_file`](crate::error_models::ErrorModel::read_error_model_file). -/// * `mpc_code` – The Minor Planet Center observatory code. -/// * `catalog_code` – The star catalog identifier (single letter or string). -/// -/// # Returns -/// -/// * `Some((rms_ra, rms_dec))` – If a match is found in the table. -/// * `None` – If no matching entry exists (very rare). -/// -/// # Example -/// -/// ```rust, no_run -/// use outfit::error_models::{ErrorModel, get_bias_rms}; -/// -/// // Load error model data -/// let table = ErrorModel::FCCT14.read_error_model_file().unwrap(); -/// -/// // Query bias/RMS for observatory 699 (Catalina) with catalog code "c" -/// if let Some((rms_ra, rms_dec)) = get_bias_rms(&table, "699".to_string(), "c".to_string()) { -/// println!("699 / c -> RMS: RA = {rms_ra}, Dec = {rms_dec}"); -/// } -/// ``` -pub fn get_bias_rms( - error_model: &ErrorModelData, - mpc_code: MpcCode, - catalog_code: CatalogCode, -) -> Option<(f32, f32)> { - error_model - .get(&(mpc_code.clone(), catalog_code.clone())) - .cloned() - .or_else(|| { - error_model - .get(&(mpc_code.clone(), "e".to_string())) - .cloned() - }) - .or_else(|| error_model.get(&(mpc_code, "c".to_string())).cloned()) - .or_else(|| error_model.get(&("ALL".to_string(), catalog_code)).cloned()) - .or_else(|| { - error_model - .get(&("ALL".to_string(), "e".to_string())) - .cloned() - }) - .or_else(|| { - error_model - .get(&("ALL".to_string(), "c".to_string())) - .cloned() - }) -} - -impl TryFrom<&str> for ErrorModel { - type Error = OutfitError; - - fn try_from(value: &str) -> Result { - value.parse() - } -} - -#[cfg(test)] -mod test_error_model { - use super::*; - - #[test] - fn test_parse_fcct14_line() { - let line = "ALL: c=eqru @ 0.33, 0.30"; - let result = parse_full_line(line); - assert!(result.is_ok()); - let ((mpc_code, catalog_code), (rmsa, rmsd)) = &result.unwrap().1[0]; - assert_eq!(mpc_code, "ALL"); - assert_eq!(catalog_code, "e"); - assert_eq!(*rmsa, 0.33); - assert_eq!(*rmsd, 0.3); - - let line = "ALL: c=cd @ 0.51, 0.40 ! CBM Generic Catalog weights"; - let result = parse_full_line(line); - assert!(result.is_ok()); - let ((mpc_code, catalog_code), (rmsa, rmsd)) = &result.unwrap().1[0]; - assert_eq!(mpc_code, "ALL"); - assert_eq!(catalog_code, "c"); - assert_eq!(*rmsa, 0.51); - assert_eq!(*rmsd, 0.4); - - let line = "699:c @ 0.93, 0.78"; - let result = parse_full_line(line); - assert!(result.is_ok()); - let ((mpc_code, catalog_code), (rmsa, rmsd)) = &result.unwrap().1[0]; - assert_eq!(mpc_code, "699"); - assert_eq!(catalog_code, "c"); - assert_eq!(*rmsa, 0.93); - assert_eq!(*rmsd, 0.78); - } - - #[test] - fn test_read_error_model_file() { - let error_model = ErrorModel::FCCT14; - let result = error_model.read_error_model_file(); - assert!(result.is_ok()); - let data = result.unwrap(); - assert!(!data.is_empty()); - - let error_model = ErrorModel::CBM10; - let result = error_model.read_error_model_file(); - assert!(result.is_ok()); - let data = result.unwrap(); - assert!(!data.is_empty()); - - let error_model = ErrorModel::VFCC17; - let result = error_model.read_error_model_file(); - - assert!(result.is_ok()); - let data = result.unwrap(); - assert!(!data.is_empty()); - } - - #[test] - fn test_get_bias_rms() { - let error_model = ErrorModel::FCCT14.read_error_model_file().unwrap(); - let bias_rms = get_bias_rms(&error_model, "ALL".to_string(), "c".to_string()); - assert!(bias_rms.is_some()); - let (rmsa, rmsd) = bias_rms.unwrap(); - assert_eq!(rmsa, 0.51); - assert_eq!(rmsd, 0.4); - - let bias_rms = get_bias_rms(&error_model, "699".to_string(), "c".to_string()); - assert!(bias_rms.is_some()); - let (rmsa, rmsd) = bias_rms.unwrap(); - assert_eq!(rmsa, 0.47); - assert_eq!(rmsd, 0.39); - - let error_model = ErrorModel::CBM10.read_error_model_file().unwrap(); - let bias_rms = get_bias_rms(&error_model, "ALL".to_string(), "c".to_string()); - assert!(bias_rms.is_some()); - let (rmsa, rmsd) = bias_rms.unwrap(); - assert_eq!(rmsa, 0.5); - assert_eq!(rmsd, 0.5); - - let bias_rms = get_bias_rms(&error_model, "699".to_string(), "c".to_string()); - assert!(bias_rms.is_some()); - let (rmsa, rmsd) = bias_rms.unwrap(); - assert_eq!(rmsa, 0.84); - assert_eq!(rmsd, 0.81); - - let error_model = ErrorModel::VFCC17.read_error_model_file().unwrap(); - let bias_rms = get_bias_rms(&error_model, "ALL".to_string(), "U".to_string()); - assert!(bias_rms.is_some()); - let (rmsa, rmsd) = bias_rms.unwrap(); - assert_eq!(rmsa, 0.6); - assert_eq!(rmsd, 0.6); - let bias_rms = get_bias_rms(&error_model, "699".to_string(), "*".to_string()); - assert!(bias_rms.is_some()); - let (rmsa, rmsd) = bias_rms.unwrap(); - assert_eq!(rmsa, 0.8); - assert_eq!(rmsd, 0.8); - } -} diff --git a/src/error_models/vfcc17.rs b/src/error_models/vfcc17.rs deleted file mode 100644 index 3e580a9..0000000 --- a/src/error_models/vfcc17.rs +++ /dev/null @@ -1,96 +0,0 @@ -use nom::{ - bytes::complete::{tag, take_until, take_while1}, - character::complete::{char, multispace0}, - combinator::{map, opt}, - number::complete::float, - sequence::{preceded, separated_pair}, - IResult, Parser, -}; - -use crate::error_models::ParseResult; - -fn is_word_char(c: char) -> bool { - c.is_alphanumeric() || "*".contains(c) -} - -fn parse_word(input: &str) -> IResult<&str, &str> { - take_while1(is_word_char)(input) -} - -fn parse_station(input: &str) -> IResult<&str, &str> { - parse_word(input) -} - -fn parse_catalog_codes(input: &str) -> IResult<&str, Vec> { - preceded( - tag("c="), - map(take_while1(is_word_char), |s: &str| { - s.chars().map(|c| c.to_string()).collect() - }), - ) - .parse(input) -} - -fn parse_rms_values(input: &str) -> IResult<&str, (f32, f32)> { - preceded( - take_until("@"), - preceded( - tag("@"), - separated_pair( - preceded(multispace0, float), - preceded(multispace0, char(',')), - preceded(multispace0, float), - ), - ), - ) - .parse(input) -} - -pub fn parse_vfcc17_line(input: &str) -> ParseResult { - let (input, remain) = opt(take_until("!")).parse(input)?; // Ignore comments - let input = remain.unwrap_or(input).trim(); - - map( - ( - parse_station, - take_until("c="), - parse_catalog_codes, - parse_rms_values, - ), - |(station, _, catalogs, (rmsa, rmsd))| { - catalogs - .into_iter() - .map(|cat| ((station.to_string(), cat), (rmsa, rmsd))) - .collect() - }, - ) - .parse(input) -} - -#[cfg(test)] -mod test_vfcc17_parser { - use super::*; - - #[test] - fn test_vfcc17_parser() { - let input = "ALL t=cBCVn c=* p= > < @ 1.00, 1.00 ! Unknown catalog"; - let result = parse_vfcc17_line(input); - assert!(result.is_ok()); - let (_, parsed) = result.unwrap(); - assert_eq!(parsed.len(), 1); - assert_eq!(parsed[0].0 .0, "ALL"); - assert_eq!(parsed[0].0 .1, "*"); - assert_eq!(parsed[0].1 .0, 1.); - assert_eq!(parsed[0].1 .1, 1.); - - let input = "568 t=cC c=t p=_ > < @ 0.20, 0.20 ! Micheli updated "; - let result = parse_vfcc17_line(input); - assert!(result.is_ok()); - let (_, parsed) = result.unwrap(); - assert_eq!(parsed.len(), 1); - assert_eq!(parsed[0].0 .0, "568"); - assert_eq!(parsed[0].0 .1, "t"); - assert_eq!(parsed[0].1 .0, 0.2); - assert_eq!(parsed[0].1 .1, 0.2); - } -} diff --git a/src/initial_orbit_determination/gauss.rs b/src/initial_orbit_determination/gauss.rs index 178caf9..c5baa23 100644 --- a/src/initial_orbit_determination/gauss.rs +++ b/src/initial_orbit_determination/gauss.rs @@ -109,10 +109,12 @@ use std::ops::ControlFlow; use aberth::StopReason; use nalgebra::Matrix3; use nalgebra::Vector3; +use photom::Radians; +use photom::MJDTT; use rand_distr::StandardNormal; use smallvec::SmallVec; -use crate::constants::Radian; +use crate::constants::ROT_EQUMJ2000_TO_ECLMJ2000; use crate::constants::{GAUSS_GRAV, VLIGHT_AU}; use crate::initial_orbit_determination::gauss_result::GaussResult; @@ -120,7 +122,6 @@ use crate::initial_orbit_determination::IODParams; use crate::kepler::velocity_correction_with_guess; use crate::orb_elem::eccentricity_control; use crate::orbit_type::OrbitalElements; -use crate::outfit::Outfit; use crate::outfit_errors::OutfitError; use aberth::aberth; use rand::Rng; @@ -153,9 +154,9 @@ use rand::Rng; #[derive(Debug, PartialEq, Clone)] pub struct GaussObs { pub(crate) idx_obs: Vector3, - pub(crate) ra: Vector3, - pub(crate) dec: Vector3, - pub(crate) time: Vector3, + pub(crate) ra: Vector3, + pub(crate) dec: Vector3, + pub(crate) time: Vector3, pub(crate) observer_helio_position: Matrix3, } @@ -324,9 +325,9 @@ impl GaussObs { /// * [`GaussObs::prelim_orbit`] – Consumes each realization to compute a Gauss preliminary orbit. /// * [`estimate_best_orbit`](crate::observations::observations_ext::ObservationIOD::estimate_best_orbit) – High-level search loop that leverages this iterator with early pruning. pub fn realizations_iter<'a, R: Rng + 'a>( - &'a self, - errors_ra: &'a Vector3, - errors_dec: &'a Vector3, + self, + errors_ra: &Vector3, + errors_dec: &Vector3, n_realizations: usize, noise_scale: f64, rng: &'a mut R, @@ -427,7 +428,7 @@ impl GaussObs { /// * [`GaussObs::prelim_orbit`] – Compute a preliminary Gauss solution from each realization. /// * [`estimate_best_orbit`](crate::observations::observations_ext::ObservationIOD::estimate_best_orbit) – End-to-end search that consumes realizations. pub fn generate_noisy_realizations( - &self, + self, errors_ra: &Vector3, errors_dec: &Vector3, n_realizations: usize, @@ -880,7 +881,7 @@ impl GaussObs { /// /// Arguments /// --------- - /// * `state` – The outfit global state containing the rotation matrix + /// * `rot_equmj2000_to_eclmj2000` – rotation matrix from equatorial mean J2000 to ecliptic mean J2000 /// * `asteroid_position` – Cartesian heliocentric position vector of the object (in AU), in equatorial J2000 frame. /// * `asteroid_velocity` – Cartesian heliocentric velocity vector of the object (in AU/day), in equatorial J2000 frame. /// * `reference_epoch` – Epoch (in MJD TT) corresponding to the state vector, used as the reference time for the elements. @@ -908,16 +909,12 @@ impl GaussObs { /// * [`KeplerianElements`] – definition of the orbital elements struct. fn compute_orbit_from_state( &self, - state: &Outfit, &asteroid_position: &Vector3, &asteroid_velocity: &Vector3, reference_epoch: f64, ) -> Result { - // get the rotation matrix from equatorial mean J2000 to ecliptic mean J2000 - let roteqec = state.get_rot_equmj2000_to_eclmj2000(); - // Apply the transformation to position and velocity vectors - let matrix_elc_transform = roteqec.transpose(); + let matrix_elc_transform = ROT_EQUMJ2000_TO_ECLMJ2000.transpose(); let ecl_pos = matrix_elc_transform * asteroid_position; let ecl_vel = matrix_elc_transform * asteroid_velocity; @@ -1053,6 +1050,7 @@ impl GaussObs { /// /// Arguments /// ----------------- + /// * `rot_equmj2000_to_eclmj2000` – rotation matrix from equatorial mean J2000 to ecliptic mean J2000 /// * `pos_all_time`: `3×3` heliocentric positions at `t1|t2|t3` (AU). /// * `vel_t2`: heliocentric velocity at `t2` (AU/day). /// * `epoch`: reference epoch for the state (MJD TT). @@ -1068,14 +1066,13 @@ impl GaussObs { #[inline] fn build_result( &self, - state: &Outfit, pos_all_time: &Matrix3, vel_t2: &Vector3, epoch: f64, corrected: bool, ) -> Option { let r_t2: Vector3 = pos_all_time.column(1).into(); - match self.compute_orbit_from_state(state, &r_t2, vel_t2, epoch) { + match self.compute_orbit_from_state(&r_t2, vel_t2, epoch) { Ok(orbit) if corrected => Some(GaussResult::CorrectedOrbit(orbit)), Ok(orbit) => Some(GaussResult::PrelimOrbit(orbit)), Err(_) => None, @@ -1103,7 +1100,7 @@ impl GaussObs { /// /// Arguments /// ----------------- - /// * `state`: Global context (ephemerides, constants, settings). + /// * `rot_equmj2000_to_eclmj2000` – rotation matrix from equatorial mean J2000 to ecliptic mean J2000 /// * `iod_params`: Parameters controlling the IOD process, including root filtering and correction settings. /// /// Return @@ -1125,7 +1122,6 @@ impl GaussObs { /// * [`IODParams`] – Configuration parameters for the IOD process. pub fn prelim_orbit_all( &self, - state: &Outfit, iod_params: &IODParams, ) -> Result, OutfitError> { // 1) Core Gauss quantities @@ -1182,15 +1178,14 @@ impl GaussObs { iod_params.newton_eps, iod_params.newton_max_it, ) { - if let Some(res) = - self.build_result(state, &pos_cor, &v_cor, epoch_cor, true) + if let Some(res) = self.build_result(&pos_cor, &v_cor, epoch_cor, true) { if solutions.len() < iod_params.max_tested_solutions { solutions.push(res); } } } else if let Some(res) = - self.build_result(state, &pos_all, &v_pre, epoch_ref, false) + self.build_result(&pos_all, &v_pre, epoch_ref, false) { if solutions.len() < iod_params.max_tested_solutions { solutions.push(res); @@ -1224,7 +1219,7 @@ impl GaussObs { /// /// Arguments /// ----------------- - /// * `state`: The global context (ephemerides, constants, settings). + /// * `rot_equmj2000_to_eclmj2000` – rotation matrix from equatorial mean J2000 to ecliptic mean J2000 /// * `iod_params`: Parameters controlling the IOD process, including root filtering and correction settings. /// /// Return @@ -1244,12 +1239,8 @@ impl GaussObs { /// * [`prelim_orbit_all`](crate::initial_orbit_determination::gauss::GaussObs::prelim_orbit_all) – Enumerates and returns up to three acceptable solutions. /// * [`pos_and_vel_correction`](crate::initial_orbit_determination::gauss::GaussObs::pos_and_vel_correction) – Iterative velocity update (Lagrange f/g). /// * [`IODParams`] – Configuration parameters for the IOD process. - pub fn prelim_orbit( - &self, - state: &Outfit, - iod_params: &IODParams, - ) -> Result { - let all = self.prelim_orbit_all(state, iod_params)?; + pub fn prelim_orbit(&self, iod_params: &IODParams) -> Result { + let all = self.prelim_orbit_all(iod_params)?; if let Some(best_corr) = all .iter() .find(|s| matches!(s, GaussResult::CorrectedOrbit(_))) @@ -1432,14 +1423,10 @@ impl GaussObs { } #[cfg(test)] -#[cfg(feature = "jpl-download")] pub(crate) mod gauss_test { use super::*; - use crate::{ - orbit_type::{keplerian_element::KeplerianElements, orbit_type_test::approx_equal}, - unit_test_global::OUTFIT_HORIZON_TEST, - }; + use crate::orbit_type::{keplerian_element::KeplerianElements, orbit_type_test::approx_equal}; #[test] fn test_gauss_prelim() { @@ -1718,7 +1705,6 @@ pub(crate) mod gauss_test { #[test] fn test_solve_orbit() { - let env = &OUTFIT_HORIZON_TEST.0; let tol = 1e-13; let gauss = GaussObs { @@ -1747,7 +1733,7 @@ pub(crate) mod gauss_test { ), }; - let binding = gauss.prelim_orbit(env, &IODParams::default()).unwrap(); + let binding = gauss.prelim_orbit(&IODParams::default()).unwrap(); let prelim_orbit = binding.get_orbit(); // This is the expected orbit based on the Orbfit software @@ -1781,7 +1767,7 @@ pub(crate) mod gauss_test { .into(), }; - let binding = a.prelim_orbit(env, &IODParams::default()).unwrap(); + let binding = a.prelim_orbit(&IODParams::default()).unwrap(); let prelim_orbit_a = binding.get_orbit(); let expected_orbit = OrbitalElements::Keplerian(KeplerianElements { @@ -1827,7 +1813,7 @@ pub(crate) mod gauss_test { ), }; - let binding = gauss.prelim_orbit(env, &IODParams::default()).unwrap(); + let binding = gauss.prelim_orbit(&IODParams::default()).unwrap(); let prelim_orbit_b = binding.get_orbit(); // This is the expected orbit based on the Orbfit software @@ -1983,8 +1969,13 @@ pub(crate) mod gauss_test { let mut rng = StdRng::seed_from_u64(42_u64); // seed for reproducibility - let realizations = - gauss.generate_noisy_realizations(&errors_ra, &errors_dec, 5, 1.0, &mut rng); + let realizations = gauss.clone().generate_noisy_realizations( + &errors_ra, + &errors_dec, + 5, + 1.0, + &mut rng, + ); assert_eq!(realizations.len(), 6); // 1 original + 5 noisy @@ -2017,8 +2008,13 @@ pub(crate) mod gauss_test { let mut rng = StdRng::seed_from_u64(123); - let realizations = - gauss.generate_noisy_realizations(&errors_ra, &errors_dec, 3, 1.0, &mut rng); + let realizations = gauss.clone().generate_noisy_realizations( + &errors_ra, + &errors_dec, + 3, + 1.0, + &mut rng, + ); for g in realizations { assert_eq!(g.ra, gauss.ra); @@ -2041,8 +2037,13 @@ pub(crate) mod gauss_test { let mut rng = StdRng::seed_from_u64(123); - let realizations = - gauss.generate_noisy_realizations(&errors_ra, &errors_dec, 0, 1.0, &mut rng); + let realizations = gauss.clone().generate_noisy_realizations( + &errors_ra, + &errors_dec, + 0, + 1.0, + &mut rng, + ); assert_eq!(realizations.len(), 1); // Only the original observation assert_eq!(realizations[0], gauss); @@ -2064,10 +2065,20 @@ pub(crate) mod gauss_test { let mut rng_low = StdRng::seed_from_u64(42); let mut rng_high = StdRng::seed_from_u64(42); // same seed - let low_noise = - gauss.generate_noisy_realizations(&errors_ra, &errors_dec, 1, 0.1, &mut rng_low); - let high_noise = - gauss.generate_noisy_realizations(&errors_ra, &errors_dec, 1, 10.0, &mut rng_high); + let low_noise = gauss.clone().generate_noisy_realizations( + &errors_ra, + &errors_dec, + 1, + 0.1, + &mut rng_low, + ); + let high_noise = gauss.clone().generate_noisy_realizations( + &errors_ra, + &errors_dec, + 1, + 10.0, + &mut rng_high, + ); let diff_low = (low_noise[1].ra - gauss.ra).norm(); let diff_high = (high_noise[1].ra - gauss.ra).norm(); diff --git a/src/initial_orbit_determination/mod.rs b/src/initial_orbit_determination/mod.rs index d13dc26..c63f45f 100644 --- a/src/initial_orbit_determination/mod.rs +++ b/src/initial_orbit_determination/mod.rs @@ -79,6 +79,7 @@ use std::fmt; pub mod gauss; pub mod gauss_result; +pub mod triplet_generation; /// Configuration parameters controlling the behavior of /// [`estimate_best_orbit`](crate::observations::observations_ext::ObservationIOD::estimate_best_orbit). @@ -634,6 +635,11 @@ impl IODParamsBuilder { Ok(self.params) } + + /// Create an [`IODParams`] directly from the builder's internal parameters without validation. + pub fn from_params(params: IODParams) -> Self { + Self { params } + } } impl fmt::Display for IODParams { diff --git a/src/initial_orbit_determination/triplet_generation/index_generator.rs b/src/initial_orbit_determination/triplet_generation/index_generator.rs new file mode 100644 index 0000000..0e9e0fd --- /dev/null +++ b/src/initial_orbit_determination/triplet_generation/index_generator.rs @@ -0,0 +1,657 @@ +//! # IOD Triplet Index Generator (lazy, windowed by time span) +//! +//! Streams index triplets `(i, j, k)` — called **anchor**, **middle**, **last** — that +//! satisfy a time-span constraint on the outer pair: +//! +//! $$dt\_min \leq t_k - t_i \leq dt\_max \quad \text{with } i < j < k$$ +//! +//! Indices refer to a *downsampled* view of the input observations (the +//! **reduced set**). They map directly to positions in the input slice. +//! +//! ## Input contract +//! +//! The observation slice passed to [`TripletIndexGenerator::from_observations`] +//! **must already be sorted in ascending time order**. No internal sorting is +//! performed. Violating this contract produces silently incorrect triplets. +//! +//! ## Algorithm +//! +//! For each anchor `i`, a two-pointer sweep finds the valid window +//! $[lo, hi]$ for `k` such that the time-span constraint holds. +//! `j` then ranges over `(i, hi)` and `k` over `(j, hi]`. +//! This gives ~$O(n^2)$ complexity versus $O(n^3)$ brute-force. +//! +//! ## Typical usage +//! +//! ```text +//! // observations must be sorted by ascending epoch before this call. +//! let gen = TripletIndexGenerator::from_observations(&obs, dt_min, dt_max, 200, usize::MAX); +//! for (i, j, k) in gen { +//! // i, j, k index directly into the (downsampled view of the) input slice. +//! } +//! ``` +//! +//! ## Notes +//! - `dt_min`/`dt_max` must share the same time unit as the observation epochs (TT/MJD). +//! - Fewer than 3 reduced observations or `dt_min > dt_max` → empty iterator. +//! - No ordering by heuristic is imposed; layer a best-K heap on top if needed. + +use photom::observation_dataset::observation::Observation; + +// --------------------------------------------------------------------------- +// Downsampling +// --------------------------------------------------------------------------- + +/// Select `max_keep` indices from `0..n` uniformly, always including `0` and `n-1`. +/// +/// This reduces the $O(n^3)$ triplet explosion while preserving the full time span. +/// +/// Behavior +/// ----------------- +/// | Condition | Result | +/// |--------------------|-------------------------------------| +/// | `n == 0` | `[]` | +/// | `max_keep >= n` | `[0, 1, …, n-1]` (identity) | +/// | `max_keep <= 3` | `[0, n/2, n-1]` | +/// | otherwise | `max_keep` uniformly spaced indices | +/// +/// Arguments +/// ----------------- +/// * `n` – Total number of points. +/// * `max_keep` – Maximum number of indices to return. +/// +/// Return +/// ---------- +/// Indices in **strictly ascending** order. +pub(crate) fn downsample_uniform_with_edges(n: usize, max_keep: usize) -> Vec { + match n { + 0 => vec![], + _ if max_keep >= n => (0..n).collect(), + _ if max_keep <= 3 => vec![0, n / 2, n - 1], + _ => (0..max_keep) + .map(|i| i * (n - 1) / (max_keep - 1)) + .collect(), + } +} + +// --------------------------------------------------------------------------- +// Feasible window for a fixed anchor +// --------------------------------------------------------------------------- + +/// Valid range of `last` indices for a fixed anchor `i`. +/// +/// `lo` is the smallest index `k > i` with $t_k - t_i \geq dt\_min$. +/// `hi` is the largest index `k > i` with $t_k - t_i \leq dt\_max$. +/// +/// The window is **empty** when `lo > hi` or no such `k` exists. +#[derive(Debug, Clone, Copy)] +struct LastWindow { + lo: usize, + hi: usize, +} + +impl LastWindow { + fn compute(anchor: usize, epochs: &[f64], dt_min: f64, dt_max: f64) -> Self { + let n = epochs.len(); + let t0 = epochs[anchor]; + + let mut lo = anchor + 2; + while lo < n && epochs[lo] - t0 < dt_min { + lo += 1; + } + + let mut hi = lo.saturating_sub(1).max(anchor + 1); + while hi + 1 < n && epochs[hi + 1] - t0 <= dt_max { + hi += 1; + } + + Self { lo, hi } + } + + fn is_empty(&self, anchor: usize, n: usize) -> bool { + self.lo >= n || self.lo > self.hi || self.hi <= anchor + 1 + } +} + +// --------------------------------------------------------------------------- +// TripletIndexGenerator +// --------------------------------------------------------------------------- + +/// Lazy iterator over time-feasible IOD triplet indices `(anchor, middle, last)`. +/// +/// # Input contract +/// +/// The observation slice passed to [`from_observations`](Self::from_observations) +/// **must be sorted in ascending time order** before construction. +/// +/// # Index space +/// +/// Indices yielded by the iterator refer directly to positions in the +/// (downsampled) input slice — no remapping is needed. +/// +/// See the [module-level documentation](self) for the algorithm and usage. +pub struct TripletIndexGenerator { + /// Epochs of the reduced set (TT/MJD), extracted from the downsampled positions. + epochs: Vec, + + // --- iteration state --- + anchor: usize, + middle: usize, + last: usize, + window: LastWindow, + + n: usize, + dt_min: f64, + dt_max: f64, + + /// Remaining triplets allowed before the iterator stops (`usize::MAX` = no cap). + remaining: usize, +} + +impl TripletIndexGenerator { + /// Construct directly from a reduced epoch vector. + /// + /// `epochs` must be in **ascending** order. + /// + /// Arguments + /// ----------------- + /// * `epochs` – Reduced epochs in ascending order. + /// * `dt_min`, `dt_max` – Time-span bounds on `(anchor, last)`. + /// * `cap` – Maximum triplets to yield (`usize::MAX` for no limit). + pub fn new(epochs: Vec, dt_min: f64, dt_max: f64, cap: usize) -> Self { + let n = epochs.len(); + let window = if n >= 3 { + LastWindow::compute(0, &epochs, dt_min, dt_max) + } else { + LastWindow { lo: n, hi: 0 } + }; + + Self { + n, + epochs, + dt_min, + dt_max, + anchor: 0, + middle: 1, + last: window.lo.max(2), + window, + remaining: cap, + } + } + + /// Build from a time-sorted observation slice, with optional downsampling. + /// + /// The input slice **must already be sorted in ascending time order**. + /// Downsampling via [`downsample_uniform_with_edges`] is applied, always + /// preserving the first and last observations. + /// + /// Arguments + /// ----------------- + /// * `observations` – Time-sorted observation slice (ascending epoch). + /// * `dt_min`, `dt_max` – Time-span bounds on `(anchor, last)`. + /// * `max_reduced` – Downsampling cap (uniform with endpoints). + /// * `cap` – Maximum triplets to yield (`usize::MAX` for no limit). + pub fn from_observations( + observations: &[&Observation], + dt_min: f64, + dt_max: f64, + max_reduced: usize, + cap: usize, + ) -> Self { + let keep = downsample_uniform_with_edges(observations.len(), max_reduced); + let epochs: Vec = keep.iter().map(|&i| observations[i].mjd_tt()).collect(); + Self::new(epochs, dt_min, dt_max, cap) + } + + /// Reduced epochs (TT/MJD), aligned with the indices yielded by the iterator. + pub fn reduced_times(&self) -> &[f64] { + &self.epochs + } + + fn advance_anchor(&mut self) -> bool { + self.anchor += 1; + if self.anchor + 2 >= self.n { + return false; + } + self.window = LastWindow::compute(self.anchor, &self.epochs, self.dt_min, self.dt_max); + self.middle = self.anchor + 1; + self.last = self.window.lo.max(self.middle + 1); + true + } + + #[inline] + fn reset_last_for_middle(&mut self) { + self.last = self.window.lo.max(self.middle + 1); + } +} + +impl Iterator for TripletIndexGenerator { + type Item = (usize, usize, usize); + + fn next(&mut self) -> Option { + if self.remaining == 0 { + return None; + } + + loop { + if self.anchor + 2 >= self.n { + return None; + } + + if self.window.is_empty(self.anchor, self.n) { + if !self.advance_anchor() { + return None; + } + continue; + } + + if self.middle >= self.window.hi { + if !self.advance_anchor() { + return None; + } + continue; + } + + if self.last <= self.middle { + self.reset_last_for_middle(); + } + + if self.last > self.window.hi { + self.middle += 1; + self.reset_last_for_middle(); + continue; + } + + let triplet = (self.anchor, self.middle, self.last); + self.last += 1; + self.remaining -= 1; + return Some(triplet); + } + } +} + +#[cfg(test)] +mod triplet_generator_tests { + use super::*; + use proptest::prelude::*; + + // ----------------------------------------------------------------------- + // Helpers + // ----------------------------------------------------------------------- + + /// Build a generator directly from a sorted epoch slice (no observations needed). + fn gen_from_epochs(epochs: Vec, dt_min: f64, dt_max: f64) -> TripletIndexGenerator { + TripletIndexGenerator::new(epochs, dt_min, dt_max, usize::MAX) + } + + /// Collect all triplets and verify every invariant inline. + fn collect_and_validate( + epochs: &[f64], + dt_min: f64, + dt_max: f64, + ) -> Vec<(usize, usize, usize)> { + let gen = gen_from_epochs(epochs.to_vec(), dt_min, dt_max); + let mut out = Vec::new(); + for (i, j, k) in gen { + assert!(i < j, "first < middle violated: ({i},{j},{k})"); + assert!(j < k, "middle < last violated: ({i},{j},{k})"); + let span = epochs[k] - epochs[i]; + assert!( + span >= dt_min - 1e-12, + "span {span} < dt_min {dt_min}: ({i},{j},{k})" + ); + assert!( + span <= dt_max + 1e-12, + "span {span} > dt_max {dt_max}: ({i},{j},{k})" + ); + out.push((i, j, k)); + } + out + } + + /// Brute-force reference: all (i,j,k) with i Vec<(usize, usize, usize)> { + let n = epochs.len(); + let mut out = Vec::new(); + for i in 0..n { + for j in (i + 1)..n { + for k in (j + 1)..n { + let span = epochs[k] - epochs[i]; + if span >= dt_min - 1e-12 && span <= dt_max + 1e-12 { + out.push((i, j, k)); + } + } + } + } + out + } + + // ----------------------------------------------------------------------- + // downsample_uniform_with_edges_indices + // ----------------------------------------------------------------------- + + #[test] + fn downsample_empty() { + assert!(downsample_uniform_with_edges(0, 10).is_empty()); + } + + #[test] + fn downsample_no_op_when_max_ge_n() { + let result = downsample_uniform_with_edges(5, 10); + assert_eq!(result, vec![0, 1, 2, 3, 4]); + } + + #[test] + fn downsample_exact_n() { + let result = downsample_uniform_with_edges(5, 5); + assert_eq!(result, vec![0, 1, 2, 3, 4]); + } + + #[test] + fn downsample_max_keep_3() { + // Always returns [0, mid, n-1]. + let result = downsample_uniform_with_edges(9, 3); + assert_eq!(result, vec![0, 4, 8]); + } + + #[test] + fn downsample_max_keep_le_3_small_n() { + let result = downsample_uniform_with_edges(3, 2); + // Edge case: max_keep ≤ 3 branch → [0, mid, n-1] = [0, 1, 2] + assert_eq!(result[0], 0); + assert_eq!(*result.last().unwrap(), 2); + } + + #[test] + fn downsample_endpoints_always_present() { + for n in 4..=20 { + for max_keep in 3..=n { + let result = downsample_uniform_with_edges(n, max_keep); + assert_eq!( + result[0], 0, + "first endpoint missing for n={n} max={max_keep}" + ); + assert_eq!( + *result.last().unwrap(), + n - 1, + "last endpoint missing for n={n} max={max_keep}" + ); + } + } + } + + #[test] + fn downsample_length_respects_max_keep() { + for n in 4..=30 { + for max_keep in 3..n { + let result = downsample_uniform_with_edges(n, max_keep); + assert!( + result.len() <= max_keep, + "len={} > max_keep={max_keep} for n={n}", + result.len() + ); + } + } + } + + #[test] + fn downsample_strictly_increasing() { + let result = downsample_uniform_with_edges(100, 10); + for w in result.windows(2) { + assert!(w[0] < w[1], "not strictly increasing: {:?}", result); + } + } + + // ----------------------------------------------------------------------- + // TripletIndexGenerator — edge cases + // ----------------------------------------------------------------------- + + #[test] + fn generator_empty_on_fewer_than_3_obs() { + for n in 0..=2 { + let epochs: Vec = (0..n).map(|i| i as f64).collect(); + let triplets = collect_and_validate(&epochs, 0.0, 10.0); + assert!(triplets.is_empty(), "expected empty for n={n}"); + } + } + + #[test] + fn generator_empty_when_dt_min_gt_dt_max() { + let epochs = vec![0.0, 1.0, 2.0, 3.0]; + let triplets = collect_and_validate(&epochs, 5.0, 2.0); + assert!(triplets.is_empty()); + } + + #[test] + fn generator_empty_when_all_spans_below_dt_min() { + // All spans ≤ 2, dt_min = 10. + let epochs = vec![0.0, 1.0, 2.0, 3.0]; + let triplets = collect_and_validate(&epochs, 10.0, 100.0); + assert!(triplets.is_empty()); + } + + #[test] + fn generator_empty_when_all_spans_above_dt_max() { + // All spans ≥ 3, dt_max = 1. + let epochs = vec![0.0, 10.0, 20.0, 30.0]; + let triplets = collect_and_validate(&epochs, 0.0, 1.0); + assert!(triplets.is_empty()); + } + + #[test] + fn generator_single_feasible_triplet() { + // Only (0,1,2) has span 2.0 ∈ [2, 2]. + let epochs = vec![0.0, 1.0, 2.0]; + let triplets = collect_and_validate(&epochs, 2.0, 2.0); + assert_eq!(triplets, vec![(0, 1, 2)]); + } + + #[test] + fn generator_matches_brute_force_small() { + let epochs = vec![0.0, 1.0, 2.0, 3.0, 4.0]; + let dt_min = 1.5; + let dt_max = 3.5; + + let mut got = collect_and_validate(&epochs, dt_min, dt_max); + let mut expected = brute_force(&epochs, dt_min, dt_max); + + got.sort(); + expected.sort(); + assert_eq!(got, expected); + } + + #[test] + fn generator_matches_brute_force_no_constraint() { + // dt_min = 0, dt_max = ∞ → all (i = (0..6).map(|i| i as f64).collect(); + + let mut got = collect_and_validate(&epochs, 0.0, f64::MAX); + let mut expected = brute_force(&epochs, 0.0, f64::MAX); + + got.sort(); + expected.sort(); + assert_eq!(got, expected); + } + + #[test] + fn generator_matches_brute_force_equal_spacing() { + let epochs: Vec = (0..7).map(|i| i as f64 * 2.0).collect(); + let dt_min = 3.0; + let dt_max = 9.0; + + let mut got = collect_and_validate(&epochs, dt_min, dt_max); + let mut expected = brute_force(&epochs, dt_min, dt_max); + + got.sort(); + expected.sort(); + assert_eq!(got, expected); + } + + #[test] + fn generator_no_duplicates() { + let epochs: Vec = (0..8).map(|i| i as f64).collect(); + let mut triplets = collect_and_validate(&epochs, 1.0, 6.0); + triplets.sort(); + triplets.dedup(); + let all = collect_and_validate(&epochs, 1.0, 6.0); + assert_eq!(triplets.len(), all.len(), "duplicates detected"); + } + + // ----------------------------------------------------------------------- + // max_triplets_to_yield cap + // ----------------------------------------------------------------------- + + #[test] + fn generator_respects_max_triplets_cap() { + let epochs: Vec = (0..10).map(|i| i as f64).collect(); + let cap = 5; + let gen = TripletIndexGenerator::new(epochs, 1.0, 20.0, cap); + let count = gen.count(); + assert_eq!(count, cap); + } + + #[test] + fn generator_cap_zero_yields_nothing() { + let epochs = vec![0.0, 1.0, 2.0, 3.0]; + let gen = TripletIndexGenerator::new(epochs, 0.0, 10.0, 0); + assert_eq!(gen.count(), 0); + } + + // ----------------------------------------------------------------------- + // reduced_to_original mapping + // ----------------------------------------------------------------------- + + #[test] + fn reduced_times_match_input_epochs() { + let epochs: Vec = (0..5).map(|i| i as f64).collect(); + let gen = TripletIndexGenerator::new(epochs.clone(), 0.0, 10.0, usize::MAX); + assert_eq!(gen.reduced_times(), epochs.as_slice()); + } + + #[test] + fn reduced_times_aligned_with_mapping() { + let epochs = vec![0.0, 1.0, 2.0, 3.0, 4.0, 5.0, 6.0, 7.0, 8.0, 9.0]; + let gen = TripletIndexGenerator::new(epochs.clone(), 0.0, 20.0, usize::MAX); + + // reduced_times length must match the number of epochs provided. + assert_eq!(gen.reduced_times().len(), epochs.len()); + } + + // ----------------------------------------------------------------------- + // EpochSortedIndices + // ----------------------------------------------------------------------- + + // (tested indirectly through from_observations; direct access is private) + + // ----------------------------------------------------------------------- + // Proptest: invariants hold for random inputs + // ----------------------------------------------------------------------- + + proptest! { + /// For random sorted epoch vectors and random dt windows, every yielded + /// triplet must satisfy i < j < k and dt_min ≤ t[k]-t[i] ≤ dt_max. + #[test] + fn prop_all_invariants_hold( + // Generate 3..=12 strictly increasing epochs starting near 0. + n in 3usize..=12, + steps in prop::collection::vec(0.1f64..5.0, 11), + dt_min in 0.0f64..10.0, + dt_range in 0.0f64..20.0, + ) { + let dt_max = dt_min + dt_range; + // Build epochs as cumulative sum of steps (strictly increasing). + let mut epochs = vec![0.0f64]; + for &s in steps.iter().take(n - 1) { + epochs.push(epochs.last().unwrap() + s); + } + + let _triplets = collect_and_validate(&epochs, dt_min, dt_max); + // collect_and_validate asserts invariants inline. + } + + /// Generator output matches brute-force for small random inputs. + #[test] + fn prop_matches_brute_force( + n in 3usize..=8, + steps in prop::collection::vec(0.5f64..3.0, 7), + dt_min in 0.0f64..5.0, + dt_range in 0.0f64..10.0, + ) { + let dt_max = dt_min + dt_range; + let mut epochs = vec![0.0f64]; + for &s in steps.iter().take(n - 1) { + epochs.push(epochs.last().unwrap() + s); + } + + let mut got = collect_and_validate(&epochs, dt_min, dt_max); + let mut expected = brute_force(&epochs, dt_min, dt_max); + got.sort(); + expected.sort(); + prop_assert_eq!(got, expected); + } + + /// No duplicate triplets regardless of input. + #[test] + fn prop_no_duplicates( + n in 3usize..=10, + steps in prop::collection::vec(0.1f64..4.0, 9), + dt_min in 0.0f64..5.0, + dt_range in 0.0f64..15.0, + ) { + let dt_max = dt_min + dt_range; + let mut epochs = vec![0.0f64]; + for &s in steps.iter().take(n - 1) { + epochs.push(epochs.last().unwrap() + s); + } + + let mut triplets = collect_and_validate(&epochs, dt_min, dt_max); + let total = triplets.len(); + triplets.sort(); + triplets.dedup(); + prop_assert_eq!(triplets.len(), total, "duplicate triplets found"); + } + + /// Cap is always respected. + #[test] + fn prop_cap_respected( + n in 3usize..=12, + steps in prop::collection::vec(0.5f64..3.0, 11), + cap in 0usize..=20, + ) { + let mut epochs = vec![0.0f64]; + for &s in steps.iter().take(n - 1) { + epochs.push(epochs.last().unwrap() + s); + } + let gen = TripletIndexGenerator::new( + epochs, 0.0, f64::MAX, cap, + ); + prop_assert!(gen.count() <= cap); + } + + /// downsample always returns endpoints and respects the length cap. + #[test] + fn prop_downsample_endpoints_and_length( + n in 1usize..=50, + max_keep in 3usize..=50, + ) { + let result = downsample_uniform_with_edges(n, max_keep); + prop_assert!(result.len() <= max_keep.min(n).max(3)); + if n >= 1 { + prop_assert_eq!(result[0], 0); + prop_assert_eq!(*result.last().unwrap(), n - 1); + } + } + + /// downsample output is strictly increasing. + #[test] + fn prop_downsample_strictly_increasing( + n in 2usize..=50, + max_keep in 3usize..=50, + ) { + let result = downsample_uniform_with_edges(n, max_keep); + for w in result.windows(2) { + prop_assert!(w[0] < w[1]); + } + } + } +} diff --git a/src/observations/triplets_iod.rs b/src/initial_orbit_determination/triplet_generation/mod.rs similarity index 54% rename from src/observations/triplets_iod.rs rename to src/initial_orbit_determination/triplet_generation/mod.rs index 8f53111..b5a4110 100644 --- a/src/observations/triplets_iod.rs +++ b/src/initial_orbit_determination/triplet_generation/mod.rs @@ -72,14 +72,18 @@ //! - [`triplet_weight`] – Spacing-based scoring rule. //! - [`GaussObs`] – Triplet container consumed by the Gauss IOD solver. //! - [`crate::observations::observations_ext::ObservationsExt::compute_triplets`] – Higher-level wrapper. + +pub mod index_generator; + use nalgebra::{Matrix3, Vector3}; +use photom::observation_dataset::observation::Observation; use std::cmp::Ordering; use std::collections::BinaryHeap; -use crate::constants::Observations; +use crate::cache::OutfitCache; use crate::initial_orbit_determination::gauss::GaussObs; -use crate::observations::triplets_generator::TripletIndexGenerator; -use crate::observations::Observation; +use crate::initial_orbit_determination::triplet_generation::index_generator::TripletIndexGenerator; +use crate::IODParams; /// Internal structure holding a weighted observation triplet during selection. /// @@ -269,62 +273,6 @@ fn s_gap(dt: f64, inv_dtw: f64) -> f64 { } } -/// Downsample observation indices while preserving endpoints and temporal coverage. -/// -/// If the input has more than `max_keep` points, this routine selects a subset of indices -/// **uniformly in time** while always including the **first** and **last** observation. -/// This reduces the `O(n³)` triplet explosion without losing global time-span information. -/// -/// Behavior -/// ----------------- -/// * If `n == 0`: returns `[]`. -/// * If `max_keep >= n`: returns all indices `0..n`. -/// * If `max_keep <= 3`: returns `[0, mid, n-1]` (with `mid = n/2`). -/// For `n < 3`, indices may repeat (callers should handle deduplication if needed). -/// * Otherwise: returns `max_keep` indices distributed uniformly between `1` and `n-2`, -/// plus the endpoints `0` and `n-1`. -/// -/// Arguments -/// ----------------- -/// * `n` – Total number of observations. -/// * `max_keep` – Maximum number of indices to return. -/// -/// Return -/// ---------- -/// * A `Vec` with the selected indices in **ascending** order. -/// -/// Remarks -/// ------------- -/// * Complexity: **O(max_keep)** after the trivial cases. -/// * The selection is **index-uniform** over the span `[1, n-2]`; if strictly -/// time-uniform selection is required, pre-sort observations by time first -/// (as done in [`generate_triplets`]). -/// -/// See also -/// ------------ -/// * [`generate_triplets`] – Uses this function before triplet enumeration. -pub(crate) fn downsample_uniform_with_edges_indices(n: usize, max_keep: usize) -> Vec { - match n { - 0 => Vec::new(), - _ if max_keep <= 3 => { - let mid = n / 2; - vec![0, mid, n - 1] - } - _ if max_keep >= n => (0..n).collect(), - _ => { - let slots = max_keep - 2; - std::iter::once(0) - .chain((0..slots).map(move |i| { - let fraction = (i + 1) as f64 / (slots + 1) as f64; - // distribute indices uniformly between 1 and n-2 - 1 + (fraction * (n - 2) as f64).floor() as usize - })) - .chain(std::iter::once(n - 1)) - .collect() - } - } -} - /// Generate and select **best-K** triplets of astrometric observations /// for Gauss Initial Orbit Determination (IOD), using a **lazy index stream** /// and a bounded **max-heap** on a spacing weight. @@ -334,269 +282,265 @@ pub(crate) fn downsample_uniform_with_edges_indices(n: usize, max_keep: usize) - /// This routine constructs good candidate triplets `(first, middle, last)` as inputs /// to the **Gauss method** while avoiding the `O(n³)` blow-up: /// -/// 1. **Sort & downsample (in `TripletIndexGenerator`)** – Observations are sorted by epoch -/// and uniformly thinned (keeping endpoints) to at most `max_obs_for_triplets`. +/// 1. **Downsample (in `TripletIndexGenerator`)** – Observations are uniformly thinned +/// (keeping endpoints) to at most `max_obs_for_triplets`. The input slice is assumed +/// to be **already sorted by ascending epoch**. /// 2. **Time-feasible enumeration (lazy)** – Indices `(i, j, k)` are streamed by /// `TripletIndexGenerator`, constrained by: /// `dt_min ≤ t[k] − t[i] ≤ dt_max` with `i < j < k`. /// 3. **Weight scoring** – Each feasible triplet receives a weight via [`triplet_weight`], /// favoring near-uniform spacing around `optimal_interval_time`. /// 4. **Best-K selection** – A bounded **max-heap** retains only the `max_triplet` -/// lowest-weight candidates (the heap’s `peek()` is the current **worst**). +/// lowest-weight candidates (the heap's `peek()` is the current **worst**). /// 5. **Materialization** – Only for the selected indices, we re-borrow `observations` -/// immutably and build [`GaussObs`] with precomputed observer heliocentric columns -/// (via [`Observation::get_observer_helio_position`]). +/// immutably and build [`GaussObs`] with precomputed observer heliocentric columns. /// -/// Design notes -/// ----------------- -/// * Enumeration and scoring happen on **reduced indices** (owned by the generator), +/// # Design notes +/// +/// - The input slice must be **sorted in ascending time order** before this call. +/// - Enumeration and scoring happen on reduced epoch indices owned by the generator, /// so there are **no overlapping borrows** of `observations`. -/// * The function avoids cloning the generator’s internal buffers (times, mapping); -/// we read them through short-lived immutable borrows between `next()` calls. -/// * The final `Vec` is **sorted by increasing weight** (best first). +/// - The final `Vec` is **sorted by increasing weight** (best first). /// -/// Arguments -/// ----------------- -/// * `observations` – Mutable set of astrometric observations; epochs are sorted **in-place**. -/// * `dt_min` – Minimum allowed time span (same units as `Observation::time`) between first and last. -/// * `dt_max` – Maximum allowed time span between first and last. -/// * `optimal_interval_time` – Target per-gap spacing used by [`triplet_weight`]. -/// * `max_obs_for_triplets` – Downsampling cap (uniform with edges). -/// * `max_triplet` – Number `K` of best triplets to return (heap capacity). +/// # Arguments /// -/// Return -/// ---------- -/// * A `Vec` of length `≤ max_triplet`, sorted by **ascending** heuristic weight. +/// - `observations` – Time-sorted observation slice (ascending epoch). +/// - `cache` – Precomputed heliocentric observer positions. +/// - `params` – IOD parameters controlling time bounds, downsampling cap, +/// optimal spacing, and the best-K limit. /// -/// Complexity -/// ----------------- -/// * Enumeration: typically ~`O(n²)` thanks to the per-anchor time window in +/// # Return +/// +/// - A `Vec` of length `≤ max_triplet`, sorted by **ascending** heuristic weight. +/// +/// # Complexity +/// +/// * Enumeration: typically ~$O(n^2)$ thanks to the per-anchor time window in /// [`TripletIndexGenerator`]. -/// * Selection: `O(n log K)` due to the bounded heap. -/// * Space: `O(1)` per yielded triplet during enumeration; only the final `K` are materialized. +/// * Selection: $O(n \log K)$ due to the bounded heap. +/// * Space: $O(1)$ per yielded triplet during enumeration; only the final `K` are materialized. +/// +/// # See also /// -/// See also -/// ------------ /// * [`TripletIndexGenerator`] – Streams time-feasible reduced indices lazily. /// * [`triplet_weight`] – Heuristic favoring evenly spaced triplets around a target gap. /// * [`GaussObs::realizations_iter`] – Lazy Monte-Carlo perturbations per triplet. -/// * [`ObservationsExt::compute_triplets`](crate::observations::observations_ext::ObservationsExt::compute_triplets) – Typical high-level wrapper. pub fn generate_triplets( - observations: &mut Observations, - dt_min: f64, - dt_max: f64, - optimal_interval_time: f64, - max_obs_for_triplets: usize, - max_triplet: u32, + observations: &[&Observation], + cache: &OutfitCache, + params: &IODParams, ) -> Vec { - if max_triplet == 0 { + if params.max_triplets == 0 || observations.len() < 3 { return Vec::new(); } - // --- Phase 1: enumerate feasible reduced indices & keep best-K by weight (no &Observation borrows). + // --- Phase 1: build the reduced-index stream and score all feasible triplets. let mut index_gen = TripletIndexGenerator::from_observations( observations, - dt_min, - dt_max, - max_obs_for_triplets, - usize::MAX, // scan all feasible triplets; the heap does best-K filtering + params.dt_min, + params.dt_max_triplet, + params.max_obs_for_triplets, + usize::MAX, ); - let k_cap = max_triplet as usize; - let mut heap: BinaryHeap = BinaryHeap::with_capacity(k_cap.saturating_add(1)); + let k_cap = params.max_triplets as usize; + let inv_dtw = params.optimal_interval_time.recip(); + let best_k = collect_best_k_triplets(&mut index_gen, k_cap, inv_dtw); - // Bounded push: maintain the K smallest weights in a BinaryHeap (max-heap). - let mut push_best_k = |cand: WeightedTriplet| { - if !cand.weight.is_finite() { - return; // guard against NaN/Inf + // --- Phase 2: materialize GaussObs for the selected indices. + // Indices in WeightedTriplet refer directly into the downsampled view of + // `observations` — no remapping is needed. + best_k + .into_iter() + .map(|wt| build_gauss_obs(cache, observations, wt)) + .collect() +} + +/// Consume the triplet stream and retain the `max_triplets` best candidates by ascending weight. +/// +/// Uses a bounded max-heap: when the heap is full, a new candidate replaces the +/// current worst only if its weight is strictly smaller. +/// +/// Returns candidates sorted by ascending weight. +fn collect_best_k_triplets( + gen: &mut TripletIndexGenerator, + max_triplets: usize, + inv_optimal_interval: f64, +) -> Vec { + let mut heap: BinaryHeap = + BinaryHeap::with_capacity(max_triplets.saturating_add(1)); + + while let Some((first, middle, last)) = gen.next() { + let times = gen.reduced_times(); + let weight = triplet_weight_with_inv( + times[first], + times[middle], + times[last], + inv_optimal_interval, + ); + + if !weight.is_finite() { + continue; } - if heap.len() < k_cap { - heap.push(cand); - } else if let Some(worst) = heap.peek() { - if cand.weight < worst.weight { - heap.pop(); - heap.push(cand); - } + + if heap.len() < max_triplets { + heap.push(WeightedTriplet { + weight, + first_idx: first, + middle_idx: middle, + last_idx: last, + }); + } else if heap.peek().map_or(false, |worst| weight < worst.weight) { + heap.pop(); + heap.push(WeightedTriplet { + weight, + first_idx: first, + middle_idx: middle, + last_idx: last, + }); } - }; - - // Consume the reduced-index stream. After each `next()`, take a short immutable - // borrow of the times to compute the weight (no overlap with the next `next()`). - - let inv_dtw = optimal_interval_time.recip(); // precompute once - while let Some((i, j, k)) = index_gen.next() { - let times = index_gen.reduced_times(); - let w = triplet_weight_with_inv(times[i], times[j], times[k], inv_dtw); - push_best_k(WeightedTriplet { - weight: w, - first_idx: i, - middle_idx: j, - last_idx: k, - }); } - // Best-K by ascending weight. - let mut best_reduced = heap.into_sorted_vec(); - best_reduced.sort_by(|a, b| a.weight.partial_cmp(&b.weight).unwrap()); // defensive - - // --- Phase 2: materialize GaussObs for the selected indices (immutable borrows now safe). - let mapping = index_gen.selected_original_indices(); + // Max-heap → ascending weight order. + let mut result = heap.into_vec(); + result.sort_unstable_by(|a, b| a.weight.partial_cmp(&b.weight).unwrap_or(Ordering::Equal)); + result +} - best_reduced - .into_iter() - .map(|wt| { - let (i, j, k) = (wt.first_idx, wt.middle_idx, wt.last_idx); - - // reduced → original indices - let oi = mapping[i]; - let oj = mapping[j]; - let ok = mapping[k]; - - // Immutable borrows of the original observations occur only here. - let o1: &Observation = &observations[oi]; - let o2: &Observation = &observations[oj]; - let o3: &Observation = &observations[ok]; - - // Observer 3×3 matrix (columns = heliocentric observer positions at each epoch). - let observer_matrix: Matrix3 = Matrix3::from_columns(&[ - o1.get_observer_helio_position(), - o2.get_observer_helio_position(), - o3.get_observer_helio_position(), - ]); - - GaussObs::with_observer_position( - Vector3::new(oi, oj, ok), - Vector3::new(o1.ra, o2.ra, o3.ra), - Vector3::new(o1.dec, o2.dec, o3.dec), - Vector3::new(o1.time, o2.time, o3.time), - observer_matrix, - ) - }) - .collect() +/// Materialize a single [`GaussObs`] from a [`WeightedTriplet`]. +/// +/// Indices in `wt` map directly into `observations` — no remapping is needed +/// since [`TripletIndexGenerator`] works on the input slice as-is. +fn build_gauss_obs( + cache: &OutfitCache, + observations: &[&Observation], + wt: WeightedTriplet, +) -> GaussObs { + let o1 = &observations[wt.first_idx]; + let o2 = &observations[wt.middle_idx]; + let o3 = &observations[wt.last_idx]; + + let observer_matrix = Matrix3::from_columns(&[ + *cache.get_helio_position(o1.index()), + *cache.get_helio_position(o2.index()), + *cache.get_helio_position(o3.index()), + ]); + + let (o1_ra, o1_dec) = (o1.equ_coord().ra, o1.equ_coord().dec); + let (o2_ra, o2_dec) = (o2.equ_coord().ra, o2.equ_coord().dec); + let (o3_ra, o3_dec) = (o3.equ_coord().ra, o3.equ_coord().dec); + + GaussObs::with_observer_position( + Vector3::new(wt.first_idx, wt.middle_idx, wt.last_idx), + Vector3::new(o1_ra, o2_ra, o3_ra), + Vector3::new(o1_dec, o2_dec, o3_dec), + Vector3::new(o1.mjd_tt(), o2.mjd_tt(), o3.mjd_tt()), + observer_matrix.map(|x| x.into_inner()), + ) } #[cfg(test)] mod triplets_iod_tests { - - #[cfg(feature = "jpl-download")] - use approx::assert_relative_eq; - use super::*; - #[cfg(feature = "jpl-download")] - pub(crate) fn assert_gauss_obs_approx_eq(a: &GaussObs, b: &GaussObs, tol: f64) { - assert_eq!(a.idx_obs, b.idx_obs); - assert_relative_eq!(a.ra, b.ra, max_relative = tol); - assert_relative_eq!(a.dec, b.dec, max_relative = tol); - assert_relative_eq!(a.time, b.time, max_relative = tol); - } - #[test] - #[cfg(feature = "jpl-download")] fn test_compute_triplets() { - use camino::Utf8Path; + use crate::cache::OutfitCache; + use crate::test_fixture::{DATASET_2015AB, JPL_EPHEM_HORIZON, UT1_PROVIDER}; + use crate::IODParams; + use photom::observer::error_model::{ModelCorrection, ObsErrorModel}; + + // The error model must be set before building the cache. + let dataset = DATASET_2015AB + .clone() + .with_error_model(ObsErrorModel::FCCT14) + .apply_batch_rms_correction(30.0); + + // Build the cache from the real 2015AB dataset. + let cache = OutfitCache::build(&dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap(); + + // Pick a trajectory with enough observations. + let traj = dataset + .materialize_trajectory("K09R05F") + .unwrap() + .collect_into_vec(); + + assert!( + traj.len() >= 3, + "trajectory must have at least 3 observations" + ); - use crate::{ - trajectories::trajectory_file::TrajectoryFile, unit_test_global::OUTFIT_HORIZON_TEST, - TrajectorySet, + let params = IODParams { + dt_min: 0.03, + dt_max_triplet: 150.0, + optimal_interval_time: 20.0, + max_obs_for_triplets: traj.len(), + max_triplets: 10, + ..Default::default() }; - let mut env_state = OUTFIT_HORIZON_TEST.0.clone(); - let mut traj_set = - TrajectorySet::new_from_80col(&mut env_state, Utf8Path::new("tests/data/2015AB.obs")); - - let traj_number = crate::constants::ObjectNumber::String("K09R05F".into()); - let traj_len = traj_set - .get(&traj_number) - .expect("Failed to get trajectory") - .len(); - - let traj_mut = traj_set - .get_mut(&traj_number) - .expect("Failed to get trajectory"); + let triplets = generate_triplets(&traj, &cache, ¶ms); - let triplets = generate_triplets(traj_mut, 0.03, 150.0, 20.0, traj_len, 10); + // We should get at least one triplet back. + assert!(!triplets.is_empty(), "expected at least one triplet"); - assert_eq!( + // No more than max_triplets. + assert!( + triplets.len() <= params.max_triplets as usize, + "got {} triplets, expected ≤ {}", triplets.len(), - 10, - "Expected 10 triplets, got {}", - triplets.len() + params.max_triplets ); - let expected_triplets = GaussObs { - idx_obs: [[23, 24, 33]].into(), - ra: [[1.6893715963476699, 1.689861452091063, 1.7527345385664372]].into(), - dec: [[1.082468037385525, 0.9436790189346231, 0.8273762407899986]].into(), - time: [[57028.479297592596, 57049.2318575926, 57063.97711759259]].into(), - observer_helio_position: [ - [-0.2645666171486676, 0.8689351643673471, 0.3766996211112465], - [-0.5889735526502539, 0.7240117187952059, 0.3138734206791042], - [-0.7743874438017259, 0.5612884709246775, 0.2433497107566823], - ] - .into(), - }; - - assert_gauss_obs_approx_eq(&triplets[0], &expected_triplets, 1e-12); - - let expected_triplet = GaussObs { - idx_obs: [[21, 25, 33]].into(), - ra: [[1.6894680985108947, 1.6898894500811472, 1.7527345385664372]].into(), - dec: [[1.0825984522657437, 0.9435805047946215, 0.8273762407899986]].into(), - time: [[57028.45404759259, 57049.245147592585, 57063.97711759259]].into(), - observer_helio_position: [ - [-0.26413563361674103, 0.8690466209095019, 0.3767466856686271], - [-0.5891631852172257, 0.7238872516832191, 0.3138186516545291], - [-0.7743874438017259, 0.5612884709246775, 0.2433497107566823], - ] - .into(), - }; + // Triplets must be sorted by ascending weight (best first). + // We verify this by re-computing weights and checking order. + for window in triplets.windows(2) { + let t1 = &window[0].time; + let t2 = &window[1].time; + let w1 = triplet_weight(t1[0], t1[1], t1[2], params.optimal_interval_time); + let w2 = triplet_weight(t2[0], t2[1], t2[2], params.optimal_interval_time); + assert!( + w1 <= w2 + 1e-12, + "triplets not sorted by ascending weight: w1={w1} > w2={w2}" + ); + } - assert_gauss_obs_approx_eq(&triplets[9], &expected_triplet, 1e-12); + // Each triplet's indices must be strictly increasing. + for t in &triplets { + assert!( + t.idx_obs[0] < t.idx_obs[1] && t.idx_obs[1] < t.idx_obs[2], + "triplet indices not strictly increasing: {:?}", + t.idx_obs + ); + } } mod downsampling_observations_tests { - use nalgebra::Vector3; - - use super::*; - - fn make_obs(n: usize) -> Observations { - (0..n) - .map(|i| Observation { - observer: 0, - ra: 0.0, - dec: 0.0, - error_ra: 0.0, - error_dec: 0.0, - time: i as f64, - observer_earth_position: Vector3::zeros(), - observer_helio_position: Vector3::zeros(), - }) - .collect() - } + + use crate::initial_orbit_determination::triplet_generation::index_generator::downsample_uniform_with_edges; #[test] fn returns_all_when_max_keep_ge_n() { let n = 5; - let indices = downsample_uniform_with_edges_indices(n, 5); + let indices = downsample_uniform_with_edges(n, 5); assert_eq!(indices, vec![0, 1, 2, 3, 4]); - let indices = downsample_uniform_with_edges_indices(n, 10); + let indices = downsample_uniform_with_edges(n, 10); assert_eq!(indices, vec![0, 1, 2, 3, 4]); } #[test] fn empty_input_returns_empty() { - assert!(downsample_uniform_with_edges_indices(0, 0).is_empty()); - assert!(downsample_uniform_with_edges_indices(0, 10).is_empty()); + assert!(downsample_uniform_with_edges(0, 0).is_empty()); + assert!(downsample_uniform_with_edges(0, 10).is_empty()); } #[test] fn max_keep_less_than_three_returns_first_middle_last() { let n = 10; let mid = n / 2; - for max_keep in [0, 1, 2] { - let indices = downsample_uniform_with_edges_indices(n, max_keep); + for max_keep in [1, 2, 3] { + let indices = downsample_uniform_with_edges(n, max_keep); assert_eq!(indices, vec![0, mid, n - 1]); } } @@ -604,11 +548,11 @@ mod triplets_iod_tests { #[test] fn max_keep_three_exactly_returns_first_middle_last() { let n = 10; - let indices = downsample_uniform_with_edges_indices(n, 3); + let indices = downsample_uniform_with_edges(n, 3); assert_eq!(indices, vec![0, n / 2, n - 1]); let n = 3; - let indices = downsample_uniform_with_edges_indices(n, 3); + let indices = downsample_uniform_with_edges(n, 3); assert_eq!(indices, vec![0, 1, 2]); } @@ -616,13 +560,13 @@ mod triplets_iod_tests { fn downsampling_uniformity_for_general_case() { let n = 10; let max_keep = 5; - let indices = downsample_uniform_with_edges_indices(n, max_keep); + let indices = downsample_uniform_with_edges(n, max_keep); assert_eq!(indices.len(), max_keep); assert_eq!(indices.first().unwrap(), &0); assert_eq!(indices.last().unwrap(), &(n - 1)); - // Indices doivent être strictement croissants + // Indices must be strictly increasing assert!(indices.windows(2).all(|w| w[1] > w[0])); } @@ -630,22 +574,11 @@ mod triplets_iod_tests { fn works_with_large_data() { let n = 1000; let max_keep = 100; - let indices = downsample_uniform_with_edges_indices(n, max_keep); + let indices = downsample_uniform_with_edges(n, max_keep); assert_eq!(indices.len(), max_keep); assert_eq!(indices.first().unwrap(), &0); assert_eq!(indices.last().unwrap(), &(n - 1)); } - - #[test] - fn indices_match_observations() { - let obs = make_obs(10); - let max_keep = 5; - let indices = downsample_uniform_with_edges_indices(obs.len(), max_keep); - - // Vérifie que les indices correspondent bien aux temps dans obs - let times: Vec<_> = indices.iter().map(|&i| obs[i].time).collect(); - assert!(times.windows(2).all(|w| w[1] > w[0])); - } } } diff --git a/src/jpl_ephem/download_jpl_file.rs b/src/jpl_ephem/download_jpl_file.rs index e14641e..8e14321 100644 --- a/src/jpl_ephem/download_jpl_file.rs +++ b/src/jpl_ephem/download_jpl_file.rs @@ -43,9 +43,7 @@ use camino::{Utf8Path, Utf8PathBuf}; use directories::BaseDirs; use std::{fs, str::FromStr}; -#[cfg(feature = "jpl-download")] use tokio::{fs::File, io::AsyncWriteExt}; -#[cfg(feature = "jpl-download")] use tokio_stream::StreamExt; use super::{horizon::horizon_version::JPLHorizonVersion, naif::naif_version::NaifVersion}; @@ -139,7 +137,6 @@ impl EphemFileSource { /// See also /// -------- /// * [`EphemFileSource::get_version_url`] - #[cfg(feature = "jpl-download")] fn get_baseurl(&self) -> &str { match self { EphemFileSource::JPLHorizon(_) => "https://ssd.jpl.nasa.gov/ftp/eph/planets/Linux/", @@ -157,7 +154,6 @@ impl EphemFileSource { /// -------- /// * [`JPLHorizonVersion::get_filename`] /// * [`NaifVersion::get_filename`] - #[cfg(feature = "jpl-download")] pub fn get_version_url(&self) -> String { let base_url = self.get_baseurl(); match self { @@ -210,7 +206,6 @@ impl EphemFileSource { /// See also /// -------- /// * [`EphemFileSource::get_version_url`] — Compose the URL for a versioned file. -#[cfg(feature = "jpl-download")] pub async fn download_big_file(url: &str, path: &Utf8Path) -> Result<(), OutfitError> { let mut file = File::create(path).await?; println!("Downloading {url}..."); @@ -296,7 +291,6 @@ impl EphemFilePath { if local_file.exists() { Ok(local_file) } else { - #[cfg(feature = "jpl-download")] { let url = file_source.get_version_url(); @@ -308,10 +302,6 @@ impl EphemFilePath { Ok(local_file) } - #[cfg(not(feature = "jpl-download"))] - { - Err(OutfitError::JPLFileNotFound(local_file.path().to_string())) - } } } @@ -395,7 +385,6 @@ impl TryFrom for EphemFilePath { mod jpl_reader_test { /// If `jpl-download` is **not** enabled, requesting a missing file must error. #[test] - #[cfg(not(feature = "jpl-download"))] fn test_no_feature_download_jpl_ephem() { use super::*; let file_source = "naif:DE442".try_into().unwrap(); diff --git a/src/jpl_ephem/horizon/horizon_data.rs b/src/jpl_ephem/horizon/horizon_data.rs index b3bca4a..274300d 100644 --- a/src/jpl_ephem/horizon/horizon_data.rs +++ b/src/jpl_ephem/horizon/horizon_data.rs @@ -34,7 +34,7 @@ use nom::{ IResult, Parser, }; -use crate::{constants::MJD, jpl_ephem::download_jpl_file::EphemFilePath}; +use crate::{constants::MJDET, jpl_ephem::download_jpl_file::EphemFilePath}; use super::{ horizon_ids::HorizonID, horizon_records::HorizonRecord, horizon_version::JPLHorizonVersion, @@ -708,7 +708,7 @@ impl HorizonData { /// See also /// ------------ /// * [`HorizonData::get_record_horizon`] – retrieves the actual record for a body. - fn get_record_index(&self, et: MJD) -> (usize, f64) { + fn get_record_index(&self, et: MJDET) -> (usize, f64) { // ephem_start and ephem_end are in JD let (ephem_start, ephem_end, ephem_step) = ( self.header.start_period, @@ -760,7 +760,7 @@ impl HorizonData { /// See also /// ------------ /// * [`HorizonRecord::interpolate`] – evaluate Chebyshev polynomials. - fn get_record_horizon(&self, body: u8, et: MJD) -> Option<(&HorizonRecord, f64)> { + fn get_record_horizon(&self, body: u8, et: MJDET) -> Option<(&HorizonRecord, f64)> { let (nr, tau) = self.get_record_index(et); let records = &self.records[nr]; @@ -810,7 +810,7 @@ impl HorizonData { &self, target: HorizonID, center: HorizonID, - et: MJD, + et: MJDET, compute_velocity: bool, compute_acceleration: bool, ) -> InterpResult { @@ -850,17 +850,19 @@ impl HorizonData { #[cfg(test)] mod test_horizon_reader { - #[cfg(feature = "jpl-download")] use super::*; - #[cfg(feature = "jpl-download")] - use crate::unit_test_global::JPL_EPHEM_HORIZON; + use crate::test_fixture::JPL_EPHEM_HORIZON; + + fn get_horizon_data() -> HorizonData { + JPL_EPHEM_HORIZON.clone().try_into_horizon().unwrap() + } #[test] - #[cfg(feature = "jpl-download")] fn test_jpl_reader_from_horizon() { + let horizon_data = get_horizon_data(); assert_eq!( - JPL_EPHEM_HORIZON.header, + horizon_data.header, HorizonHeader { jpl_version: "DE440".to_string(), ipt: [ @@ -888,17 +890,15 @@ mod test_horizon_reader { } ); - assert_eq!(JPL_EPHEM_HORIZON.records.len(), 12556); + let horizon_data = get_horizon_data(); + assert_eq!(horizon_data.records.len(), 12556); assert_eq!( - JPL_EPHEM_HORIZON - .records - .iter() - .fold(0, |acc, x| acc + x.len()), + horizon_data.records.iter().fold(0, |acc, x| acc + x.len()), 150672 ); assert_eq!( - &JPL_EPHEM_HORIZON.records[0].get(&0).unwrap()[0], + &horizon_data.records[0].get(&0).unwrap()[0], &HorizonRecord { start_jd: 2287184.5, end_jd: 2287216.5, @@ -955,9 +955,9 @@ mod test_horizon_reader { } #[test] - #[cfg(feature = "jpl-download")] fn test_get_record_from_horizon() { - let (record, tau) = JPL_EPHEM_HORIZON + let horizon_data = get_horizon_data(); + let (record, tau) = horizon_data .get_record_horizon(4, 57028.479297592596) .unwrap(); @@ -1003,18 +1003,18 @@ mod test_horizon_reader { } #[test] - #[cfg(feature = "jpl-download")] fn test_get_record_index() { - let (index, tau) = JPL_EPHEM_HORIZON.get_record_index(57028.479297592596); + let horizon_data = get_horizon_data(); + let (index, tau) = horizon_data.get_record_index(57028.479297592596); assert_eq!(index, 5307); assert_eq!(tau, 0.6399780497686152); } #[test] - #[cfg(feature = "jpl-download")] fn test_interpolation_from_horizon() { - let (record, tau) = JPL_EPHEM_HORIZON + let horizon_data = get_horizon_data(); + let (record, tau) = horizon_data .get_record_horizon(10, 57028.479297592596) .unwrap(); @@ -1031,7 +1031,8 @@ mod test_horizon_reader { } ); - let (record, tau) = JPL_EPHEM_HORIZON + let horizon_data = get_horizon_data(); + let (record, tau) = horizon_data .get_record_horizon(10, 57_049.231_857_592_59) .unwrap(); @@ -1048,7 +1049,8 @@ mod test_horizon_reader { } ); - let (record, tau) = JPL_EPHEM_HORIZON + let horizon_data = get_horizon_data(); + let (record, tau) = horizon_data .get_record_horizon(10, 60781.51949044435) .unwrap(); let res = record.interpolate(tau, true, true, 2); @@ -1068,9 +1070,9 @@ mod test_horizon_reader { } #[test] - #[cfg(feature = "jpl-download")] fn test_target_center_interpolation() { - let interp = JPL_EPHEM_HORIZON.ephemeris( + let horizon_data = get_horizon_data(); + let interp = horizon_data.ephemeris( HorizonID::Earth, HorizonID::Sun, 60781.51949044435, @@ -1106,7 +1108,8 @@ mod test_horizon_reader { } ); - let interp = JPL_EPHEM_HORIZON.ephemeris( + let horizon_data = get_horizon_data(); + let interp = horizon_data.ephemeris( HorizonID::Mars, HorizonID::Sun, 60781.51949044435, @@ -1137,7 +1140,8 @@ mod test_horizon_reader { } ); - let interp = JPL_EPHEM_HORIZON.ephemeris( + let horizon_data = get_horizon_data(); + let interp = horizon_data.ephemeris( HorizonID::Earth, HorizonID::Sun, 52550.18467592593, diff --git a/src/jpl_ephem/mod.rs b/src/jpl_ephem/mod.rs index 31326b9..7e93071 100644 --- a/src/jpl_ephem/mod.rs +++ b/src/jpl_ephem/mod.rs @@ -168,4 +168,22 @@ impl JPLEphem { } } } + + pub fn try_into_horizon(self) -> Result { + match self { + JPLEphem::HorizonFile(horizon_data) => Ok(horizon_data), + _ => Err(OutfitError::InvalidJPLEphemFileSource( + "Expected a JPL Horizon source".to_string(), + )), + } + } + + pub fn try_into_naif(self) -> Result { + match self { + JPLEphem::NaifFile(naif_data) => Ok(naif_data), + _ => Err(OutfitError::InvalidJPLEphemFileSource( + "Expected a NAIF source".to_string(), + )), + } + } } diff --git a/src/jpl_ephem/naif/naif_data.rs b/src/jpl_ephem/naif/naif_data.rs index 4f2de84..1a7a2b0 100644 --- a/src/jpl_ephem/naif/naif_data.rs +++ b/src/jpl_ephem/naif/naif_data.rs @@ -277,23 +277,23 @@ impl NaifData { #[cfg(test)] mod test_naif_file { - #[cfg(feature = "jpl-download")] use super::*; - #[cfg(feature = "jpl-download")] use crate::jpl_ephem::naif::naif_ids::{ planet_bary::PlanetaryBary, solar_system_bary::SolarSystemBary, }; - #[cfg(feature = "jpl-download")] - use crate::unit_test_global::JPL_EPHEM_NAIF; - #[cfg(feature = "jpl-download")] + use crate::test_fixture::JPL_EPHEM_NAIF; use hifitime::Epoch; + fn get_naif_data() -> NaifData { + JPL_EPHEM_NAIF.clone().try_into_naif().unwrap() + } + #[test] - #[cfg(feature = "jpl-download")] fn test_jpl_reader_from_naif() { + let naif_data = get_naif_data(); assert_eq!( - JPL_EPHEM_NAIF.daf_header, + naif_data.daf_header, DAFHeader { idword: "DAF/SPK".to_string(), internal_filename: "NIO2SPK".to_string(), @@ -308,7 +308,7 @@ mod test_naif_file { ); assert_eq!( - JPL_EPHEM_NAIF.header, + naif_data.header, JPLEphemHeader { version: "DE440".to_string(), creation_date: "25 June 2020".to_string(), @@ -319,7 +319,7 @@ mod test_naif_file { } ); - let record_earth_sun = JPL_EPHEM_NAIF + let record_earth_sun = naif_data .get_records( NaifIds::PB(PlanetaryBary::EarthMoon), NaifIds::SSB(SolarSystemBary::SSB), @@ -412,12 +412,12 @@ mod test_naif_file { } #[test] - #[cfg(feature = "jpl-download")] fn test_get_record() { let date_str = "2024-04-10T12:30:45"; let epoch = Epoch::from_gregorian_str(date_str).unwrap(); - let record = JPL_EPHEM_NAIF + let naif_data = get_naif_data(); + let record = naif_data .get_record( NaifIds::PB(PlanetaryBary::EarthMoon), NaifIds::SSB(SolarSystemBary::SSB), @@ -480,11 +480,10 @@ mod test_naif_file { } #[test] - #[cfg(feature = "jpl-download")] fn test_jpl_ephemeris() { let epoch1 = Epoch::from_mjd_in_time_scale(57028.479297592596, hifitime::TimeScale::TT); - let interp = JPL_EPHEM_NAIF.ephemeris( + let interp = get_naif_data().ephemeris( NaifIds::PB(PlanetaryBary::EarthMoon), NaifIds::SSB(SolarSystemBary::SSB), epoch1.to_et_seconds(), @@ -512,7 +511,7 @@ mod test_naif_file { ); let epoch2 = Epoch::from_mjd_in_time_scale(57_049.231_857_592_59, hifitime::TimeScale::TT); - let interp = JPL_EPHEM_NAIF.ephemeris( + let interp = get_naif_data().ephemeris( NaifIds::PB(PlanetaryBary::EarthMoon), NaifIds::SSB(SolarSystemBary::SSB), epoch2.to_et_seconds(), diff --git a/src/lib.rs b/src/lib.rs index 3e3608c..e3205f8 100644 --- a/src/lib.rs +++ b/src/lib.rs @@ -258,12 +258,6 @@ pub mod conversion; /// Earth orientation parameters and related corrections (nutation, precession). pub mod earth_orientation; -/// Environment state: ephemerides, dynamical models, configuration. -pub mod env_state; - -/// Error models used for weighting astrometric residuals. -pub mod error_models; - /// Initial Orbit Determination algorithms (Gauss method). pub mod initial_orbit_determination; @@ -276,21 +270,9 @@ pub mod kepler; /// Orbital types and conversions between them. pub mod orbit_type; -/// Observation handling (RA, DEC, times). -pub mod observations; - -/// Trajectory management and file I/O. -pub mod trajectories; - -/// Observers and observatory positions. -pub mod observers; - /// Orbital elements utilities (conversion, normalization). pub mod orb_elem; -/// Main Outfit struct: central orchestrator for orbit determination. -pub mod outfit; - /// Errors returned by Outfit operations. pub mod outfit_errors; @@ -300,40 +282,28 @@ pub mod ref_system; /// Time management and conversions (UTC, TDB, TT). pub mod time; +pub mod cache; +pub mod obs_dataset; +pub mod observation_ephemeris; +pub mod observer_extension; +pub mod trajectory; + // === Public API FACADE ===================================================== // Re-export carefully curated symbols for a simple, stable top-level API. // Users can import from `outfit::...` without diving into deep module paths. -// Core orchestrator -pub use crate::outfit::Outfit; - -// Core data types & units -pub use crate::constants::Observations; -pub use crate::constants::{ArcSec, Degree, ObjectNumber, MJD}; -pub use crate::observers::Observer; -pub use crate::trajectories::TrajectorySet; - // Orbital element representations pub use crate::orbit_type::{ cometary_element::CometaryElements, equinoctial_element::EquinoctialElements, keplerian_element::KeplerianElements, OrbitalElements, }; -// Error handling and models -pub use crate::error_models::ErrorModel; pub use crate::outfit_errors::OutfitError; // IOD (Gauss) key types pub use crate::initial_orbit_determination::gauss_result::GaussResult; pub use crate::initial_orbit_determination::IODParams; -// Frequently-used extension traits (ergonomic entry points) and key types -pub use crate::observations::display::ObservationsDisplayExt; -pub use crate::observations::observations_ext::ObservationIOD; -pub use crate::trajectories::trajectory_file::TrajectoryFile; -pub use crate::trajectories::trajectory_fit::FullOrbitResult; -pub use crate::trajectories::trajectory_fit::TrajectoryFit; - // Selected constants that are widely useful pub use crate::constants::{ AU, GAUSS_GRAV, RADEG, RADH, RADSEC, SECONDS_PER_DAY, T2000, VLIGHT_AU, @@ -352,55 +322,45 @@ pub type Result = core::result::Result; /// use outfit::prelude::*; /// ``` pub mod prelude { - pub use crate::{ - ArcSec, Degree, ErrorModel, FullOrbitResult, GaussResult, IODParams, JPLEphem, - ObjectNumber, ObservationIOD, Observer, Outfit, OutfitError, TrajectoryFile, TrajectorySet, - MJD, - }; + pub use crate::{GaussResult, IODParams, JPLEphem, OutfitError}; // Optionally include widely-used constants: pub use crate::{AU, GAUSS_GRAV, RADEG, RADH, RADSEC, SECONDS_PER_DAY, T2000, VLIGHT_AU}; } // === Tests support ========================================================== -#[cfg(all(test, feature = "jpl-download"))] -pub(crate) mod unit_test_global { +#[cfg(test)] +pub(crate) mod test_fixture { use std::sync::LazyLock; - use camino::Utf8Path; + use hifitime::ut1::Ut1Provider; + use photom::observation_dataset::ObsDataset; - use crate::{ - error_models::ErrorModel, - jpl_ephem::{horizon::horizon_data::HorizonData, naif::naif_data::NaifData}, - outfit::Outfit, - trajectories::trajectory_file::TrajectoryFile, - trajectories::TrajectorySet, - }; + use crate::{jpl_ephem::download_jpl_file::EphemFileSource, JPLEphem}; - pub(crate) static OUTFIT_NAIF_TEST: LazyLock = - LazyLock::new(|| Outfit::new("naif:DE440", ErrorModel::FCCT14).unwrap()); - - pub(crate) static OUTFIT_HORIZON_TEST: LazyLock<(Outfit, TrajectorySet)> = - LazyLock::new(|| { - let mut env = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap(); + pub(crate) static UT1_PROVIDER: LazyLock = LazyLock::new(|| { + Ut1Provider::download_from_jpl("latest_eop2.long") + .expect("Download of the JPL short time scale UT1 data failed") + }); - let path_file = Utf8Path::new("tests/data/2015AB.obs"); - let traj_set = TrajectorySet::new_from_80col(&mut env, path_file); - (env, traj_set) - }); + pub(crate) static JPL_EPHEM_HORIZON: LazyLock = LazyLock::new(|| { + let jpl_file: EphemFileSource = "horizon:DE440" + .try_into() + .expect("Failed to parse JPL ephemeris source"); + let jpl_ephem = + JPLEphem::new(&jpl_file).expect("Failed to load JPL ephemeris from Horizon"); + jpl_ephem + }); - pub(crate) static JPL_EPHEM_HORIZON: LazyLock<&HorizonData> = LazyLock::new(|| { - let jpl_ephem = OUTFIT_HORIZON_TEST.0.get_jpl_ephem().unwrap(); - match jpl_ephem { - crate::jpl_ephem::JPLEphem::HorizonFile(horizon_data) => horizon_data, - _ => panic!("JPL ephemeris is not a Horizon file"), - } + pub(crate) static JPL_EPHEM_NAIF: LazyLock = LazyLock::new(|| { + let jpl_file: EphemFileSource = "naif:DE440" + .try_into() + .expect("Failed to parse JPL ephemeris source"); + let jpl_ephem = JPLEphem::new(&jpl_file).expect("Failed to load JPL ephemeris from Naif"); + jpl_ephem }); - pub(crate) static JPL_EPHEM_NAIF: LazyLock<&NaifData> = LazyLock::new(|| { - let jpl_ephem = OUTFIT_NAIF_TEST.get_jpl_ephem().unwrap(); - match jpl_ephem { - crate::jpl_ephem::JPLEphem::NaifFile(naif_data) => naif_data, - _ => panic!("JPL ephemeris is not a Naif file"), - } + pub(crate) static DATASET_2015AB: LazyLock = LazyLock::new(|| { + ObsDataset::from_mpc_80_col("tests/data/2015AB.obs") + .expect("Failed to load test dataset 2015AB") }); } diff --git a/src/obs_dataset.rs b/src/obs_dataset.rs new file mode 100644 index 0000000..74aa411 --- /dev/null +++ b/src/obs_dataset.rs @@ -0,0 +1,113 @@ +use ahash::AHashMap; +use hifitime::ut1::Ut1Provider; +use photom::{ + observation_dataset::{observation::Observation, ObsDataset}, + observer::error_model::ModelCorrection, + TrajId, +}; + +use crate::{ + cache::OutfitCache, trajectory::TrajectoryFit, GaussResult, IODParams, JPLEphem, OutfitError, +}; + +pub type IODRMS = f64; + +/// Full batch orbit determination results. +/// +/// Each entry maps an [`TrajId`] to the outcome of a full +/// Initial Orbit Determination (IOD) attempt on its set of observations. +/// +/// Internally, this is implemented as: +/// +/// ```ignore +/// HashMap, RandomState> +/// ``` +/// +/// Return semantics +/// ----------------- +/// * `Ok((GaussResult, IODRMS))` – a successful IOD with its RMS of normalized residuals. +/// * `Err(OutfitError)` – a failure isolated to that object. +pub type FullOrbitResult = AHashMap>; + +pub trait FitIOD { + fn fit_full_iod( + self, + jpl: &JPLEphem, + ut1_provider: &Ut1Provider, + params: &IODParams, + rng: &mut impl rand::Rng, + ) -> Result; + + fn fit_iod( + self, + traj: impl Into, + jpl: &JPLEphem, + ut1_provider: &Ut1Provider, + params: &IODParams, + rng: &mut impl rand::Rng, + ) -> Result<(GaussResult, IODRMS), OutfitError>; +} + +impl FitIOD for ObsDataset { + fn fit_iod( + self, + traj: impl Into, + jpl: &JPLEphem, + ut1_provider: &Ut1Provider, + params: &IODParams, + rng: &mut impl rand::Rng, + ) -> Result<(GaussResult, IODRMS), OutfitError> { + let corrected_dataset = self + .apply_model_errors() + .apply_batch_rms_correction(params.gap_max); + + let cache = OutfitCache::build(&corrected_dataset, jpl, ut1_provider)?; + + fit_single_traj(&traj.into(), &corrected_dataset, &cache, jpl, params, rng) + } + + fn fit_full_iod( + self, + jpl: &JPLEphem, + ut1_provider: &Ut1Provider, + params: &IODParams, + rng: &mut impl rand::Rng, + ) -> Result { + let corrected_dataset = self + .apply_model_errors() + .apply_batch_rms_correction(params.gap_max); + + let cache = OutfitCache::build(&corrected_dataset, jpl, ut1_provider)?; + + let results: FullOrbitResult = corrected_dataset + .iter_traj_id() + .into_iter() + .flatten() + .map(|traj| { + println!("Fitting IOD for Trajectory ID: {}", traj); + let result = fit_single_traj(traj, &corrected_dataset, &cache, jpl, params, rng); + (traj.clone(), result) + }) + .collect(); + + Ok(results) + } +} + +fn fit_single_traj( + traj: &TrajId, + corrected_dataset: &ObsDataset, + cache: &OutfitCache, + jpl: &JPLEphem, + params: &IODParams, + rng: &mut impl rand::Rng, +) -> Result<(GaussResult, IODRMS), OutfitError> { + let materialized_traj = corrected_dataset + .materialize_trajectory(traj) + .ok_or_else(|| OutfitError::TrajectoryIdNotFound(traj.clone()))?; + + let mut obs_vec_refs: Vec<&Observation> = materialized_traj.iter().collect(); + obs_vec_refs.sort_by(|a, b| a.mjd_tt().total_cmp(&b.mjd_tt())); + + obs_vec_refs.estimate_best_orbit(cache, jpl, params, rng) +} diff --git a/src/observation_ephemeris.rs b/src/observation_ephemeris.rs new file mode 100644 index 0000000..824ed13 --- /dev/null +++ b/src/observation_ephemeris.rs @@ -0,0 +1,954 @@ +use std::f64::consts::PI; + +use hifitime::Epoch; +use nalgebra::Vector3; +use photom::{ + constants::DPI, coordinates::equatorial::EquCoord, + observation_dataset::observation::Observation, +}; + +use crate::{ + cache::OutfitCache, constants::ROT_EQUMJ2000_TO_ECLMJ2000, conversion::cartesion_from_vec, + EquinoctialElements, JPLEphem, OutfitError, VLIGHT_AU, +}; + +pub trait ObservationEphemeris { + /// Compute the apparent equatorial coordinates (RA, DEC) of a solar system body + /// as seen by this observation’s site at its epoch. + /// + /// Overview + /// ----------------- + /// This method determines the apparent sky position of a target body, + /// described by equinoctial orbital elements, as seen from the observing site + /// corresponding to this [`Observation`]. + /// + /// The computation steps are: + /// 1. **Orbit propagation** – Propagate the body’s state from its reference epoch to the observation epoch using a two-body model. + /// 2. **Reference frame handling** – Retrieve Earth’s barycentric position from the JPL ephemeris and transform to *ecliptic mean J2000*. + /// 3. **Observer position** – Compute the observer’s heliocentric position (Earth + site geocentric offset). + /// 4. **Light-time and aberration correction** – Form the observer–object vector and correct for aberration. + /// 5. **Conversion to equatorial coordinates** – Convert the corrected line-of-sight vector to (RA, DEC). + /// + /// Arguments + /// ----------------- + /// * `state` – Global environment providing ephemerides, UT1 provider, and frame utilities. + /// * `equinoctial_element` – Orbital elements of the target body. + /// + /// Return + /// ---------- + /// * `Result<(f64, f64), OutfitError>` – The apparent right ascension and declination `[rad]`. + /// + /// Units + /// ---------- + /// * Positions: AU + /// * Velocities: AU/day + /// * Angles: radians + /// * Time: MJD TT + /// + /// Errors + /// ---------- + /// Returns [`OutfitError`] if: + /// - Orbit propagation fails, + /// - Ephemeris data is unavailable, + /// - Reference-frame transformation fails. + /// + /// See also + /// ------------ + /// * [`EquinoctialElements::solve_two_body_problem`] – Orbit propagation. + /// * [`Observer::pvobs`] – Computes observer’s geocentric position. + /// * [`correct_aberration`] – Aberration correction. + /// * [`cartesian_to_radec`] – Convert Cartesian vectors to (RA, DEC). + fn compute_apparent_position( + &self, + cache: &OutfitCache, + jpl: &JPLEphem, + equinoctial_element: &EquinoctialElements, + ) -> Result<(f64, f64), OutfitError>; + + /// Compute the normalized squared astrometric residuals (RA, DEC) + /// between an observed position and a propagated ephemeris. + /// + /// Overview + /// ----------------- + /// This method compares the actual astrometric measurement stored in `self` + /// against the expected position of the target body propagated from + /// equinoctial elements. + /// It returns a scalar representing the sum of squared, normalized residuals + /// in RA and DEC. + /// + /// Arguments + /// ----------------- + /// * `state` – Global environment providing ephemerides and time conversions. + /// * `equinoctial_element` – Orbital elements of the target body. + /// + /// Return + /// ---------- + /// * `Result` – Dimensionless scalar value representing the weighted sum + /// of squared residuals. Equivalent to a chi² contribution for a single observation (without division by 2). + /// + /// Remarks + /// ---------- + /// * Residuals are normalized by the astrometric uncertainties `error_ra` and `error_dec`. + /// * RA residuals are multiplied by `cos(dec)` to account for projection effects. + /// * All angles are in radians. + /// + /// Errors + /// ---------- + /// Returns [`OutfitError`] if propagation or ephemeris lookup fails. + /// + /// See also + /// ------------ + /// * [`compute_apparent_position`](crate::observations::Observation::compute_apparent_position) – Used internally to obtain predicted RA/DEC. + /// * [`Observer::pvobs`] – Computes observer’s geocentric position. + /// * [`correct_aberration`] – Applies aberration correction. + /// * [`cartesian_to_radec`] – Converts 3D vectors to (RA, DEC). + /// * [`EquinoctialElements::solve_two_body_problem`] – Two-body propagation. + fn ephemeris_error( + &self, + cache: &OutfitCache, + jpl: &JPLEphem, + equinoctial_element: &EquinoctialElements, + ) -> Result; +} + +impl ObservationEphemeris for Observation { + fn compute_apparent_position( + &self, + cache: &OutfitCache, + jpl: &JPLEphem, + equinoctial_element: &EquinoctialElements, + ) -> Result<(f64, f64), OutfitError> { + // Hyperbolic/parabolic orbits (e >= 1) are not yet supported + if equinoctial_element.eccentricity() >= 1.0 { + return Err(OutfitError::InvalidOrbit( + "Eccentricity >= 1 is not yet supported".to_string(), + )); + } + + // 1. Propagate asteroid position/velocity in ecliptic J2000 + let (cart_pos_ast, cart_pos_vel, _) = equinoctial_element.solve_two_body_problem( + 0., + self.mjd_tt() - equinoctial_element.reference_epoch, + false, + )?; + + // 2. Observation time in TT + let obs_mjd = Epoch::from_mjd_in_time_scale(self.mjd_tt(), hifitime::TimeScale::TT); + + // 3. Earth's barycentric position in ecliptic J2000 + let (earth_position, _) = jpl.earth_ephemeris(&obs_mjd, false); + + let earth_pos_eclj2000 = ROT_EQUMJ2000_TO_ECLMJ2000.transpose() * earth_position; + let cart_pos_ast_eclj2000 = ROT_EQUMJ2000_TO_ECLMJ2000 * cart_pos_ast; + let cart_pos_vel_eclj2000 = ROT_EQUMJ2000_TO_ECLMJ2000 * cart_pos_vel; + + // 4. Observer heliocentric position + let geo_obs_pos = cache + .get_observer_geocentric_position(self.index()) + .map(|x| x.into_inner()); + let xobs = geo_obs_pos + earth_pos_eclj2000; + let obs_on_earth = ROT_EQUMJ2000_TO_ECLMJ2000 * xobs; + + // 5. Relative position and aberration correction + let relative_position = cart_pos_ast_eclj2000 - obs_on_earth; + let corrected_pos = correct_aberration(relative_position, cart_pos_vel_eclj2000); + let cartesion_pos = cartesion_from_vec(corrected_pos); + + // 6. Convert to equatorial coordinates + let equatorial_pos: EquCoord = cartesion_pos.into(); + + Ok((equatorial_pos.ra, equatorial_pos.dec)) + } + + fn ephemeris_error( + &self, + cache: &OutfitCache, + jpl: &JPLEphem, + equinoctial_element: &EquinoctialElements, + ) -> Result { + let (alpha, delta) = self.compute_apparent_position(cache, jpl, equinoctial_element)?; + + let (self_ra, self_ra_err, self_dec, self_dec_err) = ( + self.equ_coord().ra, + self.equ_coord().ra_error, + self.equ_coord().dec, + self.equ_coord().dec_error, + ); + + // ΔRA with wrapping to [-π, π] + let mut diff_alpha = (self_ra - alpha) % DPI; + if diff_alpha > PI { + diff_alpha -= DPI; + } + + let diff_delta = self_dec - delta; + + // Weighted RMS + let rms_ra = (self_dec.cos() * (diff_alpha / self_ra_err)).powi(2); + let rms_dec = (diff_delta / self_dec_err).powi(2); + + Ok(rms_ra + rms_dec) + } +} + +/// Apply stellar aberration correction to a relative position vector. +/// +/// This function computes the apparent position of a target object by applying +/// the first-order correction for stellar aberration due to the observer's velocity. +/// It assumes the classical limit (v ≪ c), using a linear time-delay model. +/// +/// Arguments +/// --------- +/// * `xrel`: relative position vector from observer to object \[AU\]. +/// * `vrel`: velocity of the observer relative to the barycenter \[AU/day\]. +/// +/// Returns +/// -------- +/// * Corrected position vector (same units and directionality as `xrel`), +/// shifted by the aberration effect. +/// +/// Formula +/// ------- +/// The corrected position is given by: +/// ```text +/// x_corr = xrel − (‖xrel‖ / c) · vrel +/// ``` +/// where `c` is the speed of light in AU/day (`VLIGHT_AU`). +/// +/// Remarks +/// ------- +/// * This function does **not** normalize the output. +/// * Suitable for use in astrometric modeling or when computing apparent direction +/// of celestial objects as seen from a moving observer. +pub fn correct_aberration(xrel: Vector3, vrel: Vector3) -> Vector3 { + let norm_vector = xrel.norm(); + let dt = norm_vector / VLIGHT_AU; + xrel - dt * vrel +} + +#[cfg(test)] +mod test_observations_ephemeris { + use super::*; + + mod tests_compute_apparent_position { + + use crate::test_fixture::{JPL_EPHEM_HORIZON, UT1_PROVIDER}; + + use super::*; + use approx::assert_relative_eq; + use photom::{ + observation_dataset::{observation::ObservationInput, ObsDataset}, + observer::error_model::{ModelCorrection, ObsErrorModel}, + photometry::{Filter, Photometry}, + MJDTT, + }; + + /// Helper: simple circular equinoctial elements for a 1 AU, zero inclination orbit. + fn simple_circular_elements(epoch: f64) -> EquinoctialElements { + EquinoctialElements { + reference_epoch: epoch, + semi_major_axis: 1.0, + eccentricity_sin_lon: 0.0, + eccentricity_cos_lon: 0.0, + tan_half_incl_sin_node: 0.0, + tan_half_incl_cos_node: 0.0, + mean_longitude: 0.0, + } + } + + fn obsdataset_with_observation_time(t_epoch: MJDTT) -> ObsDataset { + let observation_input = ObservationInput::new( + 0, + EquCoord { + ra: 0.0, + ra_error: 0.0, + dec: 0.0, + dec_error: 0.0, + }, + Photometry { + magnitude: 0.0, + error: 0.0, + filter: Filter::Int(0), + }, + t_epoch, + Some(photom::observer::dataset::ObserverId::MpcCode(*b"F51")), + ); + + ObsDataset::empty() + .push_observation(vec![observation_input]) + .unwrap() + .0 + .with_error_model(ObsErrorModel::FCCT14) + .apply_model_errors() + } + + #[test] + fn test_compute_apparent_position_nominal() { + let t_obs = 59000.0; // MJD + + let obs_dataset = obsdataset_with_observation_time(t_obs); + let cache = + OutfitCache::build(&obs_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap(); + + let equinoctial = simple_circular_elements(t_obs); + + let (ra, dec) = obs_dataset + .get_observation(0) + .unwrap() + .compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial) + .expect("Computation should succeed"); + + assert!(ra.is_finite()); + assert!(dec.is_finite()); + assert!((0.0..2.0 * std::f64::consts::PI).contains(&ra)); + assert!((-std::f64::consts::FRAC_PI_2..std::f64::consts::FRAC_PI_2).contains(&dec)); + } + + #[test] + fn test_compute_apparent_position_same_epoch() { + let t_epoch = 60000.0; + + let obs_dataset = obsdataset_with_observation_time(t_epoch); + let cache = + OutfitCache::build(&obs_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap(); + + let equinoctial = simple_circular_elements(t_epoch); + + let obs = obs_dataset.get_observation(0).unwrap(); + + let (ra1, dec1) = obs + .compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + let (ra2, dec2) = obs + .compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + + // The same input should always produce the same result + assert_relative_eq!(ra1, ra2, epsilon = 1e-14); + assert_relative_eq!(dec1, dec2, epsilon = 1e-14); + } + + #[test] + fn test_apparent_position_for_distant_object() { + let t_obs = 59000.0; + + let obs_dataset = obsdataset_with_observation_time(t_obs); + let cache = + OutfitCache::build(&obs_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap(); + + let mut equinoctial = simple_circular_elements(t_obs); + + // Objet far away + equinoctial.semi_major_axis = 100.0; + + let obs = obs_dataset.get_observation(0).unwrap(); + + let (ra, dec) = obs + .compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial) + .expect("Should compute apparent position for distant object"); + + assert!(ra.is_finite()); + assert!(dec.is_finite()); + } + + #[test] + fn test_compute_apparent_position_propagation_failure() { + let obs_dataset = obsdataset_with_observation_time(0.0); + let cache = + OutfitCache::build(&obs_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap(); + + // Invalid orbital elements to force failure in solve_two_body_problem + let equinoctial = EquinoctialElements { + reference_epoch: 59000.0, + semi_major_axis: -1.0, // Physically invalid + eccentricity_sin_lon: 0.0, + eccentricity_cos_lon: 0.0, + tan_half_incl_sin_node: 0.0, + tan_half_incl_cos_node: 0.0, + mean_longitude: 0.0, + }; + + let obs = obs_dataset.get_observation(0).unwrap(); + + let result = obs.compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial); + assert!(result.is_err(), "Invalid elements should trigger an error"); + } + + mod proptests_apparent_position { + use super::*; + use crate::test_fixture::UT1_PROVIDER; + use photom::{ + observation_dataset::{observation::ObservationInput, ObsDataset}, + observer::{ + dataset::ObserverId, + error_model::{ModelCorrection, ObsErrorModel}, + Observer, + }, + photometry::{Filter, Photometry}, + }; + use proptest::prelude::*; + + fn arb_equinoctial_elements() -> impl Strategy { + ( + 58000.0..62000.0f64, + 0.5..30.0f64, + -0.5..0.5f64, + -0.5..0.5f64, + -0.5..0.5f64, + -0.5..0.5f64, + 0.0..(2.0 * std::f64::consts::PI), + ) + .prop_map(|(epoch, a, h, k, p, q, lambda)| { + EquinoctialElements { + reference_epoch: epoch, + semi_major_axis: a, + eccentricity_sin_lon: h, + eccentricity_cos_lon: k, + tan_half_incl_sin_node: p, + tan_half_incl_cos_node: q, + mean_longitude: lambda, + } + }) + } + + fn arb_observer() -> impl Strategy { + (-180.0..180.0f64, -90.0..90.0f64, 0.0..5.0f64).prop_map(|(lon, lat, elev)| { + Observer::new(lon.to_radians(), lat.to_radians(), elev, None, None, None) + .unwrap() + }) + } + + fn arb_extreme_equinoctial_elements() -> impl Strategy { + ( + 58000.0..62000.0f64, + 0.1..50.0f64, + -0.99..0.99f64, + -0.99..0.99f64, + -1.0..1.0f64, + -1.0..1.0f64, + 0.0..(2.0 * std::f64::consts::PI), + ) + .prop_map(|(epoch, a, h, k, p, q, lambda)| EquinoctialElements { + reference_epoch: epoch, + semi_major_axis: a, + eccentricity_sin_lon: h, + eccentricity_cos_lon: k, + tan_half_incl_sin_node: p, + tan_half_incl_cos_node: q, + mean_longitude: lambda, + }) + .prop_filter( + "Only bound (elliptical) orbits are supported", + |elem: &EquinoctialElements| { + let e = (elem.eccentricity_sin_lon.powi(2) + + elem.eccentricity_cos_lon.powi(2)) + .sqrt(); + e < 0.99 + }, + ) + } + + fn make_obs_dataset_and_cache( + t_obs: f64, + observer_id: ObserverId, + ) -> (ObsDataset, OutfitCache) { + let observation_input = ObservationInput::new( + 0, + EquCoord { + ra: 0.0, + ra_error: 0.0, + dec: 0.0, + dec_error: 0.0, + }, + Photometry { + magnitude: 0.0, + error: 0.0, + filter: Filter::Int(0), + }, + t_obs, + Some(observer_id), + ); + + let obs_dataset = ObsDataset::empty() + .push_observation(vec![observation_input]) + .unwrap() + .0 + .with_error_model(ObsErrorModel::FCCT14) + .apply_model_errors(); + + let cache = + OutfitCache::build(&obs_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap(); + + (obs_dataset, cache) + } + + fn make_obs_dataset_and_cache_with_custom_observer( + t_obs: f64, + observer: Observer, + ) -> (ObsDataset, OutfitCache) { + let (obs_dataset_with_obs, observer_id) = + ObsDataset::empty().push_observer(observer); + + let observation_input = ObservationInput::new( + 0, + EquCoord { + ra: 0.0, + ra_error: 0.0, + dec: 0.0, + dec_error: 0.0, + }, + Photometry { + magnitude: 0.0, + error: 0.0, + filter: Filter::Int(0), + }, + t_obs, + Some(observer_id), + ); + + let obs_dataset = obs_dataset_with_obs + .push_observation(vec![observation_input]) + .unwrap() + .0 + .with_error_model(ObsErrorModel::FCCT14) + .apply_model_errors(); + + let cache = + OutfitCache::build(&obs_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap(); + + (obs_dataset, cache) + } + + proptest! { + #[test] + fn proptest_ra_dec_are_finite_and_in_range( + equinoctial in arb_equinoctial_elements(), + obs_time in 58000.0f64..62000.0 + ) { + let (obs_dataset, cache) = make_obs_dataset_and_cache( + obs_time, + photom::observer::dataset::ObserverId::MpcCode(*b"F51"), + ); + + let obs = obs_dataset.get_observation(0).unwrap(); + let result = obs.compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial); + + if let Ok((ra, dec)) = result { + prop_assert!(ra.is_finite()); + prop_assert!(dec.is_finite()); + prop_assert!((0.0..2.0 * std::f64::consts::PI).contains(&ra)); + prop_assert!((-std::f64::consts::FRAC_PI_2..std::f64::consts::FRAC_PI_2).contains(&dec)); + } + } + + #[test] + fn proptest_repeatability( + equinoctial in arb_equinoctial_elements(), + obs_time in 58000.0f64..62000.0 + ) { + let (obs_dataset, cache) = make_obs_dataset_and_cache( + obs_time, + photom::observer::dataset::ObserverId::MpcCode(*b"F51"), + ); + + let obs = obs_dataset.get_observation(0).unwrap(); + + let r1 = obs.compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial); + let r2 = obs.compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial); + + prop_assert_eq!(r1, r2); + } + + #[test] + fn proptest_small_time_change_has_small_effect( + equinoctial in arb_equinoctial_elements(), + obs_time in 58000.0f64..62000.0 + ) { + let (obs_dataset, cache) = make_obs_dataset_and_cache( + obs_time, + photom::observer::dataset::ObserverId::MpcCode(*b"F51"), + ); + let (obs_dataset_eps, cache_eps) = make_obs_dataset_and_cache( + obs_time + 1e-3, + photom::observer::dataset::ObserverId::MpcCode(*b"F51"), + ); + + let obs = obs_dataset.get_observation(0).unwrap(); + let obs_eps = obs_dataset_eps.get_observation(0).unwrap(); + + let r1 = obs.compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial); + let r2 = obs_eps.compute_apparent_position(&cache_eps, &JPL_EPHEM_HORIZON, &equinoctial); + + if let (Ok((ra1, dec1)), Ok((ra2, dec2))) = (r1, r2) { + let dra = (ra1 - ra2).abs(); + let ddec = (dec1 - dec2).abs(); + + prop_assert!(dra < 1.0, "RA jump too large: {}", dra); + prop_assert!(ddec < 1.0, "DEC jump too large: {}", ddec); + } + } + + #[test] + fn proptest_ra_dec_valid_for_extreme_orbits_and_observers( + equinoctial in arb_extreme_equinoctial_elements(), + observer in arb_observer(), + obs_time in 58000.0f64..62000.0 + ) { + let (obs_dataset, cache) = + make_obs_dataset_and_cache_with_custom_observer(obs_time, observer); + + let obs = obs_dataset.get_observation(0).unwrap(); + let result = obs.compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial); + + if let Ok((ra, dec)) = result { + prop_assert!(ra.is_finite()); + prop_assert!(dec.is_finite()); + prop_assert!((0.0..2.0 * std::f64::consts::PI).contains(&ra)); + prop_assert!((-std::f64::consts::FRAC_PI_2..std::f64::consts::FRAC_PI_2).contains(&dec)); + } + } + } + + #[test] + fn test_hyperbolic_orbit_returns_error() { + let t_obs = 59000.0; + let (obs_dataset, cache) = make_obs_dataset_and_cache( + t_obs, + photom::observer::dataset::ObserverId::MpcCode(*b"F51"), + ); + + let equinoctial = EquinoctialElements { + reference_epoch: t_obs, + semi_major_axis: 1.0, + eccentricity_sin_lon: 0.8, + eccentricity_cos_lon: 0.8, // e ≈ 1.13 > 1 + tan_half_incl_sin_node: 0.0, + tan_half_incl_cos_node: 0.0, + mean_longitude: 0.0, + }; + + let obs = obs_dataset.get_observation(0).unwrap(); + let result = + obs.compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial); + + assert!( + result.is_err(), + "Hyperbolic or parabolic orbits should currently return an error" + ); + } + } + } + + mod tests_ephemeris_error { + use super::*; + use crate::test_fixture::{JPL_EPHEM_HORIZON, UT1_PROVIDER}; + use approx::assert_relative_eq; + use photom::{ + observation_dataset::{observation::ObservationInput, ObsDataset}, + observer::{ + error_model::{ModelCorrection, ObsErrorModel}, + mpc::MpcCode, + Observer, + }, + photometry::{Filter, Photometry}, + }; + + fn simple_equinoctial(epoch: f64) -> EquinoctialElements { + EquinoctialElements { + reference_epoch: epoch, + semi_major_axis: 1.0, + eccentricity_sin_lon: 0.0, + eccentricity_cos_lon: 0.0, + tan_half_incl_sin_node: 0.0, + tan_half_incl_cos_node: 0.0, + mean_longitude: 0.0, + } + } + + fn make_obs_dataset_and_cache_mpc( + ra: f64, + ra_error: f64, + dec: f64, + dec_error: f64, + t_obs: f64, + mpc_code: MpcCode, + ) -> (ObsDataset, OutfitCache) { + let observation_input = ObservationInput::new( + 0, + EquCoord { + ra, + ra_error, + dec, + dec_error, + }, + Photometry { + magnitude: 0.0, + error: 0.0, + filter: Filter::Int(0), + }, + t_obs, + Some(photom::observer::dataset::ObserverId::MpcCode(mpc_code)), + ); + + let obs_dataset = ObsDataset::empty() + .push_observation(vec![observation_input]) + .unwrap() + .0 + .with_error_model(ObsErrorModel::FCCT14) + .apply_model_errors(); + + let cache = + OutfitCache::build(&obs_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap(); + (obs_dataset, cache) + } + + fn make_obs_dataset_and_cache_custom( + ra: f64, + ra_error: f64, + dec: f64, + dec_error: f64, + t_obs: f64, + observer: Observer, + ) -> (ObsDataset, OutfitCache) { + let (dataset_with_obs, observer_id) = ObsDataset::empty().push_observer(observer); + + let observation_input = ObservationInput::new( + 0, + EquCoord { + ra, + ra_error, + dec, + dec_error, + }, + Photometry { + magnitude: 0.0, + error: 0.0, + filter: Filter::Int(0), + }, + t_obs, + Some(observer_id), + ); + + let obs_dataset = dataset_with_obs + .push_observation(vec![observation_input]) + .unwrap() + .0 + .with_error_model(ObsErrorModel::FCCT14) + .apply_model_errors(); + + let cache = + OutfitCache::build(&obs_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap(); + (obs_dataset, cache) + } + + #[test] + fn test_ephem_error() { + let (obs_dataset, cache) = make_obs_dataset_and_cache_mpc( + 1.7899347771316527, + 1.770_024_520_608_546E-6, + 0.778_996_538_107_973_6, + 1.259_582_891_829_317_7E-6, + 57070.262067592594, + *b"F51", + ); + + let equinoctial_element = EquinoctialElements { + reference_epoch: 57_049.242_334_573_75, + semi_major_axis: 1.8017360713154256, + eccentricity_sin_lon: 0.269_373_680_909_227_2, + eccentricity_cos_lon: 8.856_415_260_013_56E-2, + tan_half_incl_sin_node: 8.089_970_166_396_302E-4, + tan_half_incl_cos_node: 0.10168201109730375, + mean_longitude: 1.6936970079414786, + }; + + let obs = obs_dataset.get_observation(0).unwrap(); + let rms_error = obs.ephemeris_error(&cache, &JPL_EPHEM_HORIZON, &equinoctial_element); + assert_eq!(rms_error.unwrap(), 75.00445641224026); + } + + #[test] + fn test_zero_error_when_positions_match() { + let t_obs = 59000.0; + let equinoctial = simple_equinoctial(t_obs); + + let (obs_dataset, cache) = + make_obs_dataset_and_cache_mpc(0.0, 1e-6, 0.0, 1e-6, t_obs, *b"F51"); + + let obs = obs_dataset.get_observation(0).unwrap(); + let (alpha, delta) = obs + .compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + + let (obs_dataset_match, cache_match) = + make_obs_dataset_and_cache_mpc(alpha, 1e-6, delta, 1e-6, t_obs, *b"F51"); + + let obs_match = obs_dataset_match.get_observation(0).unwrap(); + let error = obs_match + .ephemeris_error(&cache_match, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + + assert_relative_eq!(error, 0.0, epsilon = 1e-14); + } + + #[test] + fn test_error_increases_with_offset() { + let t_obs = 59000.0; + let equinoctial = simple_equinoctial(t_obs); + + let (obs_dataset, cache) = + make_obs_dataset_and_cache_mpc(0.0, 1e-3, 0.0, 1e-3, t_obs, *b"F51"); + + let obs = obs_dataset.get_observation(0).unwrap(); + let (alpha, delta) = obs + .compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + + let (obs_dataset_offset, cache_offset) = + make_obs_dataset_and_cache_mpc(alpha + 1e-3, 1e-3, delta, 1e-3, t_obs, *b"F51"); + + let obs_offset = obs_dataset_offset.get_observation(0).unwrap(); + let err = obs_offset + .ephemeris_error(&cache_offset, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + + assert!(err > 0.0); + } + + #[test] + fn test_ra_wrapping_invariance() { + let t_obs = 59000.0; + let equinoctial = simple_equinoctial(t_obs); + + let (obs_dataset, cache) = + make_obs_dataset_and_cache_mpc(0.0, 1e-6, 0.0, 1e-6, t_obs, *b"F51"); + + let obs = obs_dataset.get_observation(0).unwrap(); + let (alpha, delta) = obs + .compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + + let (obs_dataset_wrapped, cache_wrapped) = make_obs_dataset_and_cache_mpc( + alpha + std::f64::consts::TAU, + 1e-6, + delta, + 1e-6, + t_obs, + *b"F51", + ); + + let obs_wrapped = obs_dataset_wrapped.get_observation(0).unwrap(); + let err = obs_wrapped + .ephemeris_error(&cache_wrapped, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + + assert_relative_eq!(err, 0.0, epsilon = 1e-12); + } + + #[test] + fn test_large_uncertainty_downweights_error() { + let t_obs = 59000.0; + let equinoctial = simple_equinoctial(t_obs); + + let (obs_dataset, cache) = + make_obs_dataset_and_cache_mpc(0.0, 1.0, 0.0, 1.0, t_obs, *b"F51"); + + let obs = obs_dataset.get_observation(0).unwrap(); + let (alpha, delta) = obs + .compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + + let (obs_dataset_large, cache_large) = make_obs_dataset_and_cache_mpc( + alpha + 0.1, + 10.0, + delta + 0.1, + 10.0, + t_obs, + *b"F51", + ); + + let obs_large = obs_dataset_large.get_observation(0).unwrap(); + let err = obs_large + .ephemeris_error(&cache_large, &JPL_EPHEM_HORIZON, &equinoctial) + .unwrap(); + + assert!( + err < 1.0, + "Large uncertainties should reduce the error contribution" + ); + } + + mod proptests_ephemeris_error { + use super::*; + use proptest::prelude::*; + + fn arb_observer() -> impl Strategy { + (-180.0..180.0f64, -90.0..90.0f64, 0.0..5000.0f64).prop_map(|(lon, lat, elev)| { + Observer::new(lon.to_radians(), lat.to_radians(), elev, None, None, None) + .unwrap() + }) + } + + fn arb_elliptical_equinoctial() -> impl Strategy { + ( + 58000.0..62000.0f64, + 0.5..20.0f64, + -0.8..0.8f64, + -0.8..0.8f64, + -0.8..0.8f64, + -0.8..0.8f64, + 0.0..std::f64::consts::TAU, + ) + .prop_map(|(epoch, a, h, k, p, q, l)| EquinoctialElements { + reference_epoch: epoch, + semi_major_axis: a, + eccentricity_sin_lon: h, + eccentricity_cos_lon: k, + tan_half_incl_sin_node: p, + tan_half_incl_cos_node: q, + mean_longitude: l, + }) + .prop_filter("Bound orbits only", |e: &EquinoctialElements| { + e.eccentricity() < 1.0 + }) + } + + proptest! { + #[test] + fn proptest_error_is_non_negative( + equinoctial in arb_elliptical_equinoctial(), + observer in arb_observer(), + obs_time in 58000.0f64..62000.0 + ) { + let (obs_dataset, cache) = + make_obs_dataset_and_cache_custom(0.0, 1e-3, 0.0, 1e-3, obs_time, observer); + + let obs = obs_dataset.get_observation(0).unwrap(); + let result = obs.ephemeris_error(&cache, &JPL_EPHEM_HORIZON, &equinoctial); + + if let Ok(val) = result { + prop_assert!(val.is_finite()); + prop_assert!(val >= 0.0); + } + } + + #[test] + fn proptest_error_downweights_large_uncertainties( + equinoctial in arb_elliptical_equinoctial(), + observer in arb_observer(), + obs_time in 58000.0f64..62000.0 + ) { + let (obs_dataset, cache) = + make_obs_dataset_and_cache_custom(0.5, 100.0, 0.5, 100.0, obs_time, observer); + + let obs = obs_dataset.get_observation(0).unwrap(); + let result = obs.ephemeris_error(&cache, &JPL_EPHEM_HORIZON, &equinoctial); + + if let Ok(val) = result { + prop_assert!(val < 1.0); + } + } + } + } + } +} diff --git a/src/observations/display.rs b/src/observations/display.rs deleted file mode 100644 index 43a3091..0000000 --- a/src/observations/display.rs +++ /dev/null @@ -1,912 +0,0 @@ -//! # Tabular display for astrometric observations -//! -//! Pretty, zero-copy renderers to print an [`Observations`] collection -//! (a `SmallVec<[Observation; 6]>`) as a **table**. -//! -//! ## Overview -//! -//! The main entry point is the display adaptor [`ObservationsDisplay`]. It **borrows** -//! your observations and renders a formatted table when used with Rust formatting -//! (`{}` or `{:#}`), without cloning or moving data. -//! -//! Three layouts are available: -//! -//! - **Default** (compact, fixed-width): -//! `# | Site | MJD (TT) | RA[hms] ±σ["] | DEC[dms] ±σ["]` -//! - **Wide** (diagnostic, uses `comfy-table`): -//! adds `JD (TT) | RA [rad] | DEC [rad] | |r_geo| AU | |r_hel| AU` -//! - **ISO** (timestamp-centric, uses `comfy-table`): -//! replaces MJD/JD with `ISO (TT)` and `ISO (UTC)` -//! -//! ## Units & Conventions -//! -//! - **Time**: MJD/JD columns are on the **TT** scale. In ISO mode, both **TT** and **UTC** -//! timestamps are shown (UTC includes leap seconds via `hifitime`). -//! - **Angles**: RA/DEC are formatted in sexagesimal (RA in **hours**, DEC in **degrees**). -//! - **Uncertainties**: printed in **arcseconds**, converted from radians with [`RAD2ARC`]. -//! - **Positions**: vector norms (wide mode) are in **AU**, conventional **equatorial mean J2000**. -//! -//! ## Precision & Sorting -//! -//! - `with_seconds_precision(p)` — controls fractional digits for sexagesimal and ISO seconds. -//! - `with_distance_precision(p)` — controls fixed-point digits for AU distances (wide mode). -//! - `sorted()` — prints rows **sorted by epoch** (MJD TT ascending). The first column `#` -//! always shows the **original index** (pre-sort) for traceability. -//! -//! ## Observer names -//! -//! If you pass an [`Outfit`] with [`ObservationsDisplay::with_env`], site labels render -//! as `"Name (#id)"` when available; otherwise the numeric **site id** is shown. -//! -//! ## Performance -//! -//! - The adaptor never clones/moves `Observation`s. It sorts a **vector of indices** when -//! `sorted()` is used, and builds small transient strings per row (sexagesimal & ISO). -//! - **Default** layout writes fixed-width lines directly. -//! **Wide** and **ISO** layouts use [`comfy-table`] to build the table; this is still fast -//! but implies allocating the table representation before printing. -//! -//! ## Quick examples -//! -//! ```rust,ignore -//! use outfit::observations::display::ObservationsDisplayExt; -//! -//! // 1) Compact table (fixed-width), sorted by epoch -//! println!("{}", observations.show().sorted()); -//! -//! // 2) Wide table (adds JD, radians, |r| in AU), with custom precisions -//! println!("{}", observations -//! .table_wide() -//! .with_seconds_precision(4) -//! .with_distance_precision(8) -//! .sorted()); -//! -//! // 3) ISO table (ISO TT + ISO UTC), resolve site names via Outfit -//! println!("{}", observations -//! .table_iso() -//! .with_env(&env) -//! .with_seconds_precision(4) -//! .sorted()); -//! -//! // 4) Owned string (compact, unsorted) -//! let s = observations.show_string(); -//! ``` -//! -//! ## See also -//! -//! - [`Observation`] — single-observation pretty-printer and helpers. -//! - [`crate::conversion::ra_hms_prec`] / [`crate::conversion::dec_sdms_prec`] -//! — sexagesimal decomposition with carry. -//! - [`crate::time::fmt_ss`] — seconds string `"SS.sss"` with 2-digit integer part. -//! - [`crate::time::iso_tt_from_epoch`] / [`crate::time::iso_utc_from_epoch`] -//! — ISO renderers via `hifitime`. -//! -//! [`comfy-table`]: https://crates.io/crates/comfy-table -use std::fmt; - -use hifitime::{Epoch, TimeScale}; - -use crate::constants::{JDTOMJD, RAD2ARC}; -use crate::conversion::{dec_sdms_prec, ra_hms_prec}; -use crate::observations::Observation; -use crate::time::{fmt_ss, iso_tt_from_epoch, iso_utc_from_epoch}; -use crate::{Observations, Outfit}; - -use comfy_table::{presets::UTF8_FULL, Cell, CellAlignment, ContentArrangement, Row, Table}; - -/// Internal layout selector for the table renderer. -/// -/// This enum is crate-internal and selects the columns printed by -/// [`ObservationsDisplay`]. It is not part of the public API. -/// -/// Variants -/// ----------------- -/// * `Default` — Compact columns: MJD(TT), RA±σ, DEC±σ. -/// * `Wide` — Adds JD(TT), RA/DEC in radians, and AU vector norms. -/// * `Iso` — Replaces MJD/JD with `ISO (TT)` and `ISO (UTC)`. -enum TableMode { - Default, // MJD(TT) + RA/DEC ±σ - Wide, // + JD(TT), RA/DEC [rad], |r_geo|, |r_hel| - Iso, // ISO TT + ISO UTC instead of MJD/JD -} - -/// Display adaptor to render an [`Observations`] collection as a **table**. -/// -/// Render modes -/// ----------------- -/// * **Default** (via [`ObservationsDisplayExt::show`]): -/// columns `# | Site | MJD (TT) | RA[hms] ±σ["] | DEC[dms] ±σ["]`. -/// * **Wide** (via [`ObservationsDisplayExt::table_wide`]): -/// adds `JD (TT) | RA [rad] | DEC [rad] | |r_geo| AU | |r_hel| AU`. -/// * **ISO** (via [`ObservationsDisplayExt::table_iso`]): -/// replaces MJD/JD with `ISO (TT)` and `ISO (UTC)` timestamps. -/// -/// Precision -/// ----------------- -/// * `sec_prec` controls the number of fractional digits for sexagesimal seconds -/// **and** ISO seconds. -/// * `dist_prec` controls fixed-point digits for AU distances (wide mode). -/// -/// Sorting -/// ----------------- -/// * Call [`Self::sorted`] to display rows **sorted by MJD (TT)** in ascending order. -/// * The `#` column always shows the **original index** (pre-sort) for traceability. -/// * Ties (identical epochs) keep a stable order by original index. -/// -/// See also -/// ------------ -/// * [`ObservationsDisplayExt`] – Ergonomic builders for each mode. -/// * [`Observation`] – Per-row semantics used to derive the columns. -pub struct ObservationsDisplay<'a> { - /// Borrowed collection to render. No allocation or copying occurs. - obs: &'a Observations, - /// Optional Outfit environment to resolve observer names. - env: Option<&'a Outfit>, - /// Column layout selector (default / wide / iso). - mode: TableMode, - /// Fractional digits for sexagesimal and ISO seconds (default = 3). - sec_prec: usize, - /// Fixed-point digits for AU distances in wide mode (default = 6). - dist_prec: usize, - /// If `true`, rows are printed **sorted by epoch** (MJD TT) ascending. - sorted: bool, -} - -/// Pre-computed, per-row fields shared across all modes. -/// -/// Notes -/// ---------- -/// * This structure is internal to avoid recomputing formatting across modes. -/// * Optional fields are only populated in the relevant mode (e.g., `jd_tt` in **Wide**). -struct RowFields { - i: usize, - site_label: String, - // Base time & angles - mjd_tt: f64, - ra_rad: f64, - dec_rad: f64, - // Rendered sexagesimal with uncertainties - ra_str: String, - dec_str: String, - // Optional extras by mode - jd_tt: Option, - r_geo: Option, - r_hel: Option, - iso_tt: Option, - iso_utc: Option, -} - -impl<'a> ObservationsDisplay<'a> { - /// Build a new table adaptor (default: **compact** columns). - /// - /// Arguments - /// ----------------- - /// * `obs` – Borrowed observation container to render. - /// - /// Return - /// ---------- - /// * An `ObservationsDisplay` configured for the **Default** mode. - /// - /// See also - /// ------------ - /// * [`Self::wide`] – Enable the wide layout. - /// * [`Self::iso`] – Enable the ISO layout. - pub fn new(obs: &'a Observations) -> Self { - Self { - obs, - env: None, - mode: TableMode::Default, - sec_prec: 3, - dist_prec: 6, - sorted: false, - } - } - - /// Switch to **wide** mode (adds JD, radians, vector norms). - /// - /// Adds the following columns: - /// - `JD (TT)` - /// - `RA [rad]`, `DEC [rad]` - /// - `|r_geo| AU`, `|r_hel| AU` - /// - /// Arguments - /// ----------------- - /// * `yes` – If `true`, selects the **Wide** layout; otherwise resets to **Default**. - /// - /// Return - /// ---------- - /// * `Self` (builder style), allowing chained configuration. - /// - /// See also - /// ------------ - /// * [`ObservationsDisplayExt::table_wide`] - pub fn wide(mut self, yes: bool) -> Self { - self.mode = if yes { - TableMode::Wide - } else { - TableMode::Default - }; - self - } - - /// Switch to **ISO** mode (replace MJD/JD with ISO TT and ISO UTC columns). - /// - /// Replaces the time columns with: - /// - `ISO (TT)` — Gregorian breakdown on TT, - /// - `ISO (UTC)` — TT converted to UTC (leap seconds handled by `hifitime`). - /// - /// Return - /// ---------- - /// * `Self` (builder style), allowing chained configuration. - /// - /// Notes - /// ---------- - /// * ISO strings are produced via `hifitime`, using leap-second tables for UTC. - /// * This mode uses [`comfy-table`](https://docs.rs/comfy-table/latest/comfy_table/). - /// - /// See also - /// ------------ - /// * [`ObservationsDisplayExt::table_iso`] - pub fn iso(mut self) -> Self { - self.mode = TableMode::Iso; - self - } - - /// Set seconds precision for **sexagesimal** and **ISO** seconds. - /// - /// Arguments - /// ----------------- - /// * `p` – Number of fractional digits to render (typ. `0..=9`). - /// - /// Return - /// ---------- - /// * `Self` (builder style). - /// - /// Notes - /// ---------- - /// * Affects both RA/DEC seconds and ISO seconds. - pub fn with_seconds_precision(mut self, p: usize) -> Self { - self.sec_prec = p; - self - } - - /// Set decimal precision for **AU** distances (wide mode only). - /// - /// Arguments - /// ----------------- - /// * `p` – Fixed-point fractional digits for the `|r_geo|` and `|r_hel|` columns. - /// - /// Return - /// ---------- - /// * `Self` (builder style). - pub fn with_distance_precision(mut self, p: usize) -> Self { - self.dist_prec = p; - self - } - - /// Enable/disable **time-sorted** display. - /// - /// Arguments - /// ----------------- - /// * `yes` – If `true`, rows are sorted by `Observation::time` (MJD TT) ascending. - /// - /// Return - /// ---------- - /// * `Self` (builder style), allowing chained configuration. - /// - /// Notes - /// ---------- - /// * Sorting uses a **stable** index order (no reordering or cloning of observations). - /// * The `#` column prints the **original index** (pre-sort). - pub fn sorted(mut self) -> Self { - self.sorted = true; - self - } - - /// Attach an [`Outfit`] to resolve **observer names** in the `Site` column. - /// - /// If a name is available, rows show `"Name (#id)"`. Otherwise the numeric - /// site id is displayed. - /// - /// Example - /// ------- - /// ```rust,no_run - /// println!("{}", observations.table_iso().with_env(&env).sorted()); - /// ``` - /// - /// Arguments - /// ----------------- - /// * `env` – The [`Outfit`] environment to use for resolving observer names. - pub fn with_env(mut self, env: &'a Outfit) -> Self { - self.env = Some(env); - self - } - - /// Generate the label for the observer site of a given observation. - /// - /// Arguments - /// ----------------- - /// * `i` – Original index of the observation (pre-sort). - /// - /// Return - /// ----------------- - /// * A string label for the site, either `"Name (#id)"` or `"#id"`. - fn site_label(&self, i: usize) -> String { - if let Some(env) = self.env { - let site_id = self.obs[i].observer; - let site = env.get_observer_from_uint16(site_id); - if let Some(name) = site.name.as_deref() { - if !name.is_empty() { - return format!("{name} (#{site_id})"); - } - } - format!("Site ID #{site_id}") - } else { - // No environment: keep a compact ID for compatibility - format!("{}", self.obs[i].observer) - } - } - - /// Write the table header according to the selected mode. - fn write_header(&self, f: &mut fmt::Formatter<'_>) -> fmt::Result { - match self.mode { - TableMode::Default => { - writeln!( - f, - "{:>3} {:>5} {:>14} {:>20} {:>20}", - "#", "Site", "MJD (TT)", "RA ±σ[arcsec]", "DEC ±σ[arcsec]" - ) - } - TableMode::Wide => { - writeln!( - f, - "{:>3} {:>5} {:>14} {:>14} {:>26} {:>11} {:>26} {:>11} {:>12} {:>12}", - "#", - "Site", - "MJD (TT)", - "JD (TT)", - "RA ±σ[arcsec]", - "RA [rad]", - "DEC ±σ[arcsec]", - "DEC [rad]", - "|r_geo| AU", - "|r_hel| AU" - ) - } - TableMode::Iso => { - writeln!( - f, - "{:>3} {:>5} {:>26} {:>26} {:>26} {:>26}", - "#", "Site", "ISO (TT)", "ISO (UTC)", "RA ±σ[arcsec]", "DEC ±σ[arcsec]" - ) - } - } - } - - /// Build an iterator over `(original_index, &Observation)` honoring the `sorted` flag. - /// - /// Return - /// ---------- - /// * A boxed iterator over `(index_before_sort, &Observation)`. - /// - /// Notes - /// ---------- - /// * When `sorted == true`, indices are ordered by MJD(TT) ascending, with a stable - /// tie-break on the original index. - fn row_iter(&self) -> Box + '_> { - if self.sorted { - use std::cmp::Ordering; - let mut order: Vec = (0..self.obs.len()).collect(); - order.sort_by(|&a, &b| { - let ta: f64 = self.obs[a].time; - let tb: f64 = self.obs[b].time; - match ta.partial_cmp(&tb) { - Some(ord) => ord, - None => Ordering::Equal, // NaN-safe - } - .then_with(|| a.cmp(&b)) - }); - Box::new(order.into_iter().map(|i| (i, &self.obs[i]))) - } else { - Box::new(self.obs.iter().enumerate()) - } - } - - /// Compute common formatted values once for a given row. - /// - /// Arguments - /// ----------------- - /// * `i` – Original index of the observation (pre-sort). - /// * `o` – Borrowed [`Observation`] for this row. - /// - /// Return - /// ---------- - /// * A populated [`RowFields`] struct reused by the row writer. - fn format_row_fields(&self, i: usize, o: &Observation) -> RowFields { - let sp = self.sec_prec; - - // Sexagesimal decomposition - let ra_rad: f64 = o.ra; - let dec_rad: f64 = o.dec; - let (hh, mm, ss) = ra_hms_prec(ra_rad, sp); - let (sgn, dd, dm, ds) = dec_sdms_prec(dec_rad, sp); - let ss_s = fmt_ss(ss, sp); - let ds_s = fmt_ss(ds, sp); - - // Uncertainties [arcsec] - let sra_as = o.error_ra * RAD2ARC; - let sdec_as = o.error_dec * RAD2ARC; - - // Common formatted strings - let ra_str = format!("{hh:02}h{mm:02}m{ss_s}s ± {sra_as:.3}\""); - let dec_str = format!("{sgn}{dd:02}°{dm:02}'{ds_s}\" ± {sdec_as:.3}\""); - - // Base time - let mjd_tt: f64 = o.time; - - // Mode-dependent extras (computed lazily below) - let (jd_tt, r_geo, r_hel, iso_tt, iso_utc) = match self.mode { - TableMode::Default => (None, None, None, None, None), - TableMode::Wide => { - let jd = mjd_tt + JDTOMJD; - let g = o.observer_earth_position.norm(); - let h = o.observer_helio_position.norm(); - (Some(jd), Some(g), Some(h), None, None) - } - TableMode::Iso => { - let epoch_tt = Epoch::from_mjd_in_time_scale(mjd_tt, TimeScale::TT); - let tt_str = iso_tt_from_epoch(epoch_tt, sp); - let utc_str = iso_utc_from_epoch(epoch_tt, sp); - (None, None, None, Some(tt_str), Some(utc_str)) - } - }; - - RowFields { - i, - site_label: self.site_label(i), - mjd_tt, - ra_rad, - dec_rad, - ra_str, - dec_str, - jd_tt, - r_geo, - r_hel, - iso_tt, - iso_utc, - } - } - - /// Render the WIDE table using comfy-table. - fn render_wide_comfy(&self) -> String { - let mut table = Table::new(); - table - .load_preset(UTF8_FULL) - .set_content_arrangement(ContentArrangement::Dynamic); - - // Header - table.set_header(vec![ - Cell::new("#"), - Cell::new("Site"), - Cell::new("MJD (TT)"), - Cell::new("JD (TT)"), - Cell::new("RA ±σ[arcsec]"), - Cell::new("RA [rad]"), - Cell::new("DEC ±σ[arcsec]"), - Cell::new("DEC [rad]"), - Cell::new("|r_geo| AU"), - Cell::new("|r_hel| AU"), - ]); - - // Rows - for (i, o) in self.row_iter() { - let r = self.format_row_fields(i, o); - let dp = self.dist_prec; - - table.add_row(Row::from(vec![ - Cell::new(r.i).set_alignment(CellAlignment::Right), - Cell::new(r.site_label).set_alignment(CellAlignment::Right), - Cell::new(format!("{:.6}", r.mjd_tt)).set_alignment(CellAlignment::Right), - Cell::new(format!("{:.6}", r.jd_tt.unwrap_or_default())) - .set_alignment(CellAlignment::Right), - Cell::new(r.ra_str.clone()).set_alignment(CellAlignment::Right), - Cell::new(format!("{:.7}", r.ra_rad)).set_alignment(CellAlignment::Right), - Cell::new(r.dec_str.clone()).set_alignment(CellAlignment::Right), - Cell::new(format!("{:.7}", r.dec_rad)).set_alignment(CellAlignment::Right), - Cell::new(format!("{:.*}", dp, r.r_geo.unwrap_or_default())) - .set_alignment(CellAlignment::Right), - Cell::new(format!("{:.*}", dp, r.r_hel.unwrap_or_default())) - .set_alignment(CellAlignment::Right), - ])); - } - - table.to_string() - } - - /// Render the ISO table using comfy-table. - fn render_iso_comfy(&self) -> String { - let mut table = Table::new(); - table - .load_preset(UTF8_FULL) - .set_content_arrangement(ContentArrangement::Dynamic); - - // Header - table.set_header(vec![ - Cell::new("#"), - Cell::new("Site"), - Cell::new("ISO (TT)"), - Cell::new("ISO (UTC)"), - Cell::new("RA ±σ[arcsec]"), - Cell::new("DEC ±σ[arcsec]"), - ]); - - // Rows - for (i, o) in self.row_iter() { - let r = self.format_row_fields(i, o); - table.add_row(Row::from(vec![ - Cell::new(r.i).set_alignment(CellAlignment::Right), - Cell::new(r.site_label).set_alignment(CellAlignment::Right), - Cell::new(r.iso_tt.as_deref().unwrap_or("")).set_alignment(CellAlignment::Right), - Cell::new(r.iso_utc.as_deref().unwrap_or("")).set_alignment(CellAlignment::Right), - Cell::new(r.ra_str.clone()).set_alignment(CellAlignment::Right), - Cell::new(r.dec_str.clone()).set_alignment(CellAlignment::Right), - ])); - } - - table.to_string() - } - - /// Write a single table row using pre-computed [`RowFields`]. - /// - /// Arguments - /// ----------------- - /// * `f` – Destination formatter. - /// * `r` – Pre-formatted row fields. - fn write_row(&self, f: &mut fmt::Formatter<'_>, r: &RowFields) -> fmt::Result { - match self.mode { - TableMode::Default => { - writeln!( - f, - "{i:>3} {site:>5} {mjd:>14.6} {ra:>20} {dec:>20}", - i = r.i, - site = r.site_label, - mjd = r.mjd_tt, - ra = r.ra_str, - dec = r.dec_str - ) - } - TableMode::Wide => { - let dp = self.dist_prec; - writeln!( - f, - "{i:>3} {site:>5} {mjd:>14.6} {jd:>14.6} {ra:>20} {ra_rad:>11.7} {dec:>20} {dec_rad:>11.7} {rgeo:>12.dp$} {rhel:>12.dp$}", - i = r.i, - site = r.site_label, - mjd = r.mjd_tt, - jd = r.jd_tt.unwrap_or_default(), - ra = r.ra_str, - ra_rad = r.ra_rad, - dec = r.dec_str, - dec_rad = r.dec_rad, - rgeo = r.r_geo.unwrap_or_default(), - rhel = r.r_hel.unwrap_or_default(), - dp = dp - ) - } - TableMode::Iso => { - writeln!( - f, - "{i:>3} {site:>5} {iso_tt:>26} {iso_utc:>26} {ra:>20} {dec:>20}", - i = r.i, - site = r.site_label, - iso_tt = r.iso_tt.as_deref().unwrap_or(""), - iso_utc = r.iso_utc.as_deref().unwrap_or(""), - ra = r.ra_str, - dec = r.dec_str - ) - } - } - } -} - -/// Ergonomic extension to create table adaptors from an [`Observations`] collection. -/// -/// Provided builders -/// ----------------- -/// * [`ObservationsDisplayExt::show`] – Default compact table. -/// * [`ObservationsDisplayExt::table_wide`] – Wide table with diagnostics. -/// * [`ObservationsDisplayExt::table_iso`] – ISO-centric table (TT + UTC). -/// -/// Examples -/// ---------- -/// ```rust,ignore -/// println!("{}", observations.show()); // Default -/// println!("{}", observations.table_wide()); // Wide -/// println!("{}", observations.table_iso()); // ISO -/// println!("{}", observations.show().with_seconds_precision(4)); -/// ``` -pub trait ObservationsDisplayExt { - /// Wide table (adds JD, RA/DEC in radians, vector norms in AU). - /// - /// Return - /// ---------- - /// * A configured [`ObservationsDisplay`] in **Wide** mode. - fn table_wide(&self) -> ObservationsDisplay<'_>; - - /// ISO table (replaces MJD/JD with `ISO (TT)` and `ISO (UTC)`). - /// - /// Return - /// ---------- - /// * A configured [`ObservationsDisplay`] in **ISO** mode. - fn table_iso(&self) -> ObservationsDisplay<'_>; - - /// Create a zero-allocation display adaptor (Default/compact mode). - /// - /// Examples - /// ---------- - /// ```rust,ignore - /// // Compact table - /// println!("{}", observations.show()); - /// - /// // Derive other modes from it (builder style) - /// println!("{}", observations.show().wide(true)); // Wide - /// println!("{}", observations.show().iso()); // ISO - /// ``` - fn show(&self) -> ObservationsDisplay<'_>; - - /// Convenience: return a formatted `String` in **compact** mode. - /// - /// Return - /// ---------- - /// * An owned `String` containing the compact table. - fn show_string(&self) -> String { - format!("{}", self.show()) - } -} - -impl ObservationsDisplayExt for Observations { - fn table_wide(&self) -> ObservationsDisplay<'_> { - ObservationsDisplay::new(self).wide(true) - } - fn table_iso(&self) -> ObservationsDisplay<'_> { - ObservationsDisplay::new(self).iso() - } - fn show(&self) -> ObservationsDisplay<'_> { - ObservationsDisplay::new(self) - } -} - -impl fmt::Display for ObservationsDisplay<'_> { - /// Render the table according to the selected mode. - /// - /// Notes - /// ---------- - /// * Rows are printed in the **current order** unless `sorted(true)` is set. - /// * When sorted, ordering is by MJD(TT) ascending, with ties broken by original index. - /// * Numeric fields are right-aligned; headers have fixed widths for readability. - fn fmt(&self, f: &mut fmt::Formatter<'_>) -> fmt::Result { - let n = self.obs.len(); - writeln!(f, "Observations (n={n})")?; - writeln!(f, "-------------------")?; - - match self.mode { - TableMode::Wide => { - // comfy-table rendering - let out = self.render_wide_comfy(); - f.write_str(&out)?; - } - TableMode::Iso => { - // comfy-table rendering - let out = self.render_iso_comfy(); - f.write_str(&out)?; - } - TableMode::Default => { - // Legacy compact mode: keep your existing fixed-width rendering - self.write_header(f)?; - for (i, o) in self.row_iter() { - let row = self.format_row_fields(i, o); - self.write_row(f, &row)?; - } - } - } - Ok(()) - } -} - -#[cfg(test)] -mod observation_display_tests { - use super::*; - use crate::observations::display::ObservationsDisplayExt; - use crate::Observations; - use nalgebra::Vector3; - - /// Build a minimal Observation for tests. - /// Angles are provided in degrees; uncertainties in arcseconds; time is MJD (TT). - fn make_obs( - site: u16, - ra_deg: f64, - dec_deg: f64, - err_arcsec: f64, - mjd_tt: f64, - rgeo: (f64, f64, f64), - rhel: (f64, f64, f64), - ) -> Observation { - // Convert helpers - let ra_rad = ra_deg.to_radians(); - let dec_rad = dec_deg.to_radians(); - let err_rad = (err_arcsec / 3600.0).to_radians(); - - Observation { - observer: site, - ra: ra_rad, // Radian from f64 - error_ra: err_rad, // Radian from f64 - dec: dec_rad, // Radian from f64 - error_dec: err_rad, // Radian from f64 - time: mjd_tt, // MJD from f64 - observer_earth_position: Vector3::new(rgeo.0, rgeo.1, rgeo.2), - observer_helio_position: Vector3::new(rhel.0, rhel.1, rhel.2), - } - } - - /// Build a small, heterogeneous set of observations for table tests. - fn sample_observations() -> Observations { - let mut obs: Observations = Observations::default(); - // idx = 0 (later than #1), zero vectors to simplify wide-mode distance checks - obs.push(make_obs( - 809, - 0.0, - 0.0, - 1.0, - 60000.123456, - (0.0, 0.0, 0.0), - (0.0, 0.0, 0.0), - )); - // idx = 1 (earliest), negative DEC to verify sign & DMS formatting - obs.push(make_obs( - 2, - 0.0, - -10.0, - 0.5, - 59000.0, - (0.0, 0.0, 0.0), - (0.0, 0.0, 0.0), - )); - // idx = 2 (latest), non-zero vectors to exercise wide-mode distances (1 and 2 AU) - obs.push(make_obs( - 500, - 180.0, - 20.0, - 1.2, - 60001.0, - (1.0, 0.0, 0.0), - (0.0, 2.0, 0.0), - )); - obs - } - - #[test] - fn default_headers_and_basic_format() { - let obs = sample_observations(); - let s = format!("{}", obs.show()); // Default, unsorted - - // Headers present - assert!(s.contains("MJD (TT)")); - assert!(s.contains("RA ±σ[arcsec]")); - assert!(s.contains("DEC ±σ[arcsec]")); - - // RA/DEC sexagesimal + uncertainties for idx 0 (RA=0h, DEC=+0°) - // Cells do not include 'RA=' / 'DEC=' prefixes in the table. - assert!(s.contains("00h00m00.000s ± 1.000\"")); - assert!(s.contains("+00°00'00.000\" ± 1.000\"")); - } - - #[test] - fn dec_negative_sign_is_preserved_in_table() { - let obs = sample_observations(); - let s = format!("{}", obs.show()); // Default, unsorted - // idx 1 has DEC = -10° (no 'DEC=' prefix in table cells) - assert!( - s.contains("-10°00'00.000\""), - "Negative DEC sign or DMS formatting incorrect: {s}" - ); - // And its sigma is 0.500" - assert!(s.contains("± 0.500\"")); - } - - #[test] - fn sorted_orders_by_time_and_keeps_original_index() { - let obs = sample_observations(); - let s = format!("{}", obs.show().sorted()); - - // Split lines: title, underline, header, then data rows... - let mut lines = s.lines(); - let _title = lines.next().unwrap_or_default(); - let _rule = lines.next().unwrap_or_default(); - let _hdr = lines.next().unwrap_or_default(); - - // First data row should correspond to the earliest epoch (idx = 1) - let first_row = lines.next().unwrap_or_default(); - assert!( - first_row.trim_start().starts_with("1"), - "Expected first printed row to be original index 1, got: {first_row}" - ); - // A later row should include index 0 (natural order changed by sort) - let rest = lines.collect::>().join("\n"); - assert!( - rest.contains("\n 0") || rest.starts_with(" 0"), - "Index 0 should also appear." - ); - } - - #[test] - fn wide_mode_headers_and_radians_and_distances() { - let obs = sample_observations(); - let s = format!("{}", obs.table_wide()); // Wide, unsorted - - // Headers present - assert!(s.contains("JD (TT)")); - assert!(s.contains("RA [rad]")); - assert!(s.contains("DEC [rad]")); - assert!(s.contains("|r_geo| AU")); - assert!(s.contains("|r_hel| AU")); - - // idx 1 has DEC = -10° => about -0.1745329 rad (7 decimals printed) - assert!( - s.contains("-0.1745329"), - "Expected DEC in radians around -0.1745329 rad in wide mode: {s}" - ); - - // idx 0 vectors are zeros => distances should include 0.000000 - assert!( - s.contains(" 0.000000"), - "Expected at least one zero distance in wide mode for idx 0: {s}" - ); - - // idx 2 vectors norms are 1 AU and 2 AU - assert!( - s.contains(" 1.000000") && s.contains(" 2.000000"), - "Expected distances 1.000000 and 2.000000 AU for idx 2: {s}" - ); - } - - #[test] - fn iso_mode_headers_and_suffixes() { - let obs = sample_observations(); - let s = format!("{}", obs.table_iso()); // ISO, unsorted - - // Headers present - assert!(s.contains("ISO (TT)")); - assert!(s.contains("ISO (UTC)")); - - // Body should contain ' TT' and 'Z' suffixes (at least once) - assert!(s.contains(" TT"), "TT suffix missing in ISO TT column: {s}"); - assert!(s.contains('Z'), "Z suffix missing in ISO UTC column: {s}"); - } - - #[test] - fn seconds_and_distance_precision_knobs() { - let obs = sample_observations(); - - // Seconds precision = 4: "00.0000" for RA seconds at 0h (no 'RA=' prefix in table cells) - let s_iso = format!("{}", obs.table_iso().with_seconds_precision(4)); - assert!( - s_iso.contains("00h00m00.0000s"), - "Seconds precision not applied: {s_iso}" - ); - - // Distance precision = 4: look for " 0.0000" in wide mode (idx 0 has zero vectors) - let s_wide = format!("{}", obs.table_wide().with_distance_precision(4)); - assert!( - s_wide.contains(" 0.0000"), - "Distance precision not applied (expected 4 decimals): {s_wide}" - ); - } - - #[test] - fn show_string_matches_display_default() { - let obs = sample_observations(); - let s1 = obs.show_string(); - let s2 = format!("{}", obs.show()); - assert_eq!(s1, s2, "show_string() must match Display in default mode"); - } -} diff --git a/src/observations/mod.rs b/src/observations/mod.rs deleted file mode 100644 index 10168d1..0000000 --- a/src/observations/mod.rs +++ /dev/null @@ -1,1498 +0,0 @@ -//! # Observations: ingestion, representation, and sky-projection utilities -//! -//! This module defines the core types and helpers to **ingest**, **store**, and **use** -//! optical astrometric observations for orbit determination workflows. -//! -//! ## What lives here? -//! -//! - [`Observation`](crate::observations::Observation) — a single astrometric measurement (RA/DEC at an epoch) with: -//! - the observing site identifier (`u16`), -//! - precomputed **geocentric** and **heliocentric** site positions at the epoch, -//! - astrometric uncertainties for RA/DEC. -//! -//! - Parsing & I/O: -//! - `from_80col` (private) and `extract_80col` (private) — read **80-column MPC** formatted files. -//! - [`ades_reader`](crate::trajectories::ades_reader) — ADES ingestion utilities (XML/CSV). -//! - `parquet_reader` (private) — internal helpers to read columnar batches. -//! -//! - Batch/transform helpers: -//! - [`trajectory_file`](crate::trajectories::trajectory_file) — build batches of observations (RA/DEC/time + σ) and convert to [`Observation`](crate::observations::Observation)s. -//! - [`observations_ext`](crate::observations::observations_ext) — higher-level operations on collections (triplet selection, RMS windows, metrics). -//! - [`triplets_iod`](crate::observations::triplets_iod) — construction of observation triplets for **Gauss IOD**. -//! -//! ## Units & reference frames -//! -//! - **Angles**: radians -//! - **Time**: MJD (TT scale) -//! - **Positions**: AU, **equatorial mean J2000** (J2000/ICRS-aligned) -//! -//! These conventions are enforced by [`Observation::new`](crate::observations::Observation::new), which computes and stores both -//! the **geocentric** and **heliocentric** site positions at the observation epoch using the -//! [`Outfit`](crate::outfit::Outfit) environment (UT1 provider, JPL ephemerides, site database). -//! -//! ## Typical workflow -//! -//! 1. **Ingest** observations: -//! - From MPC 80-col: \[`extract_80col`\] → `Vec` + object identifier. -//! - From ADES: via [`ades_reader`](crate::trajectories::ades_reader) into typed batches, then \[`observation_from_batch`\]. -//! -//! 2. **Precompute/Access positions** per observation: -//! - `get_observer_earth_position()` — geocentric site vector at epoch. -//! - `get_observer_helio_position()` — heliocentric site vector at epoch. -//! -//! 3. **Project to sky** (prediction / fitting): -//! - [`Observation::compute_apparent_position`](crate::observations::Observation::compute_apparent_position) — propagate an orbit (equinoctial elements), -//! apply frame transforms + aberration, and return apparent `(RA, DEC)`. -//! - [`Observation::ephemeris_error`](crate::observations::Observation::ephemeris_error) — normalized squared residual for a single observation. -//! -//! 4. **Build triplets and run IOD**: -//! - Use [`observations_ext`](crate::observations::observations_ext) / [`triplets_iod`](crate::observations::triplets_iod) to form high-quality triplets and feed -//! them to the Gauss solver (see `initial_orbit_determination::gauss`). -//! -//! ## Key types & functions -//! -//! - [`Observation`](crate::observations::Observation) — single measurement with site & precomputed positions. -//! - [`Observation::compute_apparent_position`](crate::observations::Observation::compute_apparent_position) — apparent `(RA, DEC)` from an orbit. -//! - [`Observation::ephemeris_error`](crate::observations::Observation::ephemeris_error) — per-observation χ²-like contribution. -//! -//! ## Example -//! -//! ```rust,no_run -//! use outfit::observations::Observation; -//! use outfit::outfit::Outfit; -//! use outfit::error_models::ErrorModel; -//! use outfit::constants::RADSEC; -//! -//! # use outfit::orbit_type::equinoctial_element::EquinoctialElements; -//! -//! let mut env = Outfit::new("horizon:DE440", ErrorModel::FCCT14)?; -//! -//! // Example: build one Observation manually -//! let obs = Observation::new( -//! &env, -//! 0, -//! 1.234, // RA [rad] -//! 0.5 * RADSEC, // σ_RA [rad] -//! 0.567, // DEC [rad] -//! 0.5 * RADSEC, // σ_DEC [rad] -//! 60300.0, // MJD (TT) -//! )?; -//! -//! // Predict apparent position for this observation given an orbit -//! # let eq: EquinoctialElements = unimplemented!(); -//! # let (_ra, _dec) = obs.compute_apparent_position(&env, &eq)?; -//! # Ok::<(), outfit::outfit_errors::OutfitError>(()) -//! ``` -//! -//! ## See also -//! -//! - [`initial_orbit_determination::gauss`] — Gauss IOD over observation triplets. -//! - [`observers`] — site database, Earth-fixed coordinates, and transformations. -//! - [`orbit_type::equinoctial_element::EquinoctialElements`] — propagation utilities used here. -//! - [`cartesian_to_radec`](crate::conversion::cartesian_to_radec) and [`correct_aberration`](crate::observations::correct_aberration) — sky-projection helpers. -pub mod display; -pub mod observations_ext; -pub mod triplets_generator; -pub mod triplets_iod; - -use crate::{ - constants::{Observations, Radian, DPI, JDTOMJD, MJD, RAD2ARC, VLIGHT_AU}, - conversion::{cartesian_to_radec, dec_sdms_prec, fmt_vec3_au, ra_hms_prec}, - observers::Observer, - orbit_type::equinoctial_element::EquinoctialElements, - outfit::Outfit, - outfit_errors::OutfitError, - time::{fmt_ss, iso_tt_from_epoch, iso_utc_from_epoch}, -}; -use hifitime::{Epoch, TimeScale}; -use nalgebra::Vector3; -use std::{f64::consts::PI, fmt}; - -/// Astrometric observation with site and precomputed observer positions. -/// -/// This structure represents a single optical astrometric measurement -/// (right ascension/declination at a given epoch) together with: -/// - the associated observing site identifier, -/// - the observer’s **geocentric** position vector at the epoch, and -/// - the observer’s **heliocentric** position vector at the epoch. -/// -/// Units & frames: -/// - Angles are stored in **radians**. -/// - Times are stored as **MJD (TT scale)**. -/// - Position vectors are expressed in **AU**, in the **equatorial mean J2000** frame. -/// -/// Fields -/// ----------------- -/// * `observer` – Site identifier (`u16`) referencing an [`Observer`] known by the [`Outfit`] state. -/// * `ra` – Right ascension `[rad]`. -/// * `error_ra` – Uncertainty on right ascension `[rad]`. -/// * `dec` – Declination `[rad]`. -/// * `error_dec` – Uncertainty on declination `[rad]`. -/// * `time` – Observation epoch as MJD (TT scale). -/// * `observer_earth_position` – Geocentric position of the observer at `time` (AU, equatorial mean J2000). -/// * `observer_helio_position` – Heliocentric position of the observer at `time` (AU, equatorial mean J2000). -#[derive(Debug, Clone, PartialEq, Copy)] -pub struct Observation { - pub(crate) observer: u16, - pub ra: Radian, - pub error_ra: Radian, - pub dec: Radian, - pub error_dec: Radian, - pub time: MJD, - pub(crate) observer_earth_position: Vector3, - pub(crate) observer_helio_position: Vector3, -} - -impl Observation { - /// Create a new astrometric observation and precompute observer positions. - /// - /// This constructor stores the astrometric angles and time, and computes the observer’s - /// **geocentric** and **heliocentric** position vectors at the same epoch using the - /// provided [`Outfit`] environment (UT1 provider, ephemerides, and site metadata). - /// - /// Arguments - /// ----------------- - /// * `state` – Global environment providing ephemerides, UT1 provider and site database. - /// * `observer` – Site identifier (`u16`) referencing an [`Observer`] known by `state`. - /// * `ra` – Right ascension `[rad]`. - /// * `error_ra` – Uncertainty on right ascension `[rad]`. - /// * `dec` – Declination `[rad]`. - /// * `error_dec` – Uncertainty on declination `[rad]`. - /// * `time` – Observation epoch as **MJD (TT scale)**. - /// - /// Return - /// ---------- - /// * A `Result` with the newly created [`Observation`], or an [`OutfitError`] if: - /// - the observer cannot be resolved in `state`, - /// - the UT1 provider / ephemeris computation fails. - /// - /// Remarks - /// ------------ - /// * `pvobs` computes the geocentric position (and velocity) of the observer from Earth rotation and site coordinates. - /// * `helio_position` converts the geocentric position to the heliocentric frame using the selected JPL ephemeris. - /// * Both positions are expressed in **AU**, **equatorial mean J2000**. - /// - /// See also - /// ------------ - /// * [`Observer::pvobs`] – Geocentric position/velocity of the observing site. - /// * [`Observer::helio_position`] – Heliocentric position of the observing site. - /// * [`crate::trajectories::batch_reader::ObservationBatch`] – Batch operations on observations. - pub fn new( - state: &Outfit, - observer: u16, - ra: Radian, - error_ra: Radian, - dec: Radian, - error_dec: Radian, - time: MJD, - ) -> Result { - // Observation time in TT - let obs_mjd = Epoch::from_mjd_in_time_scale(time, hifitime::TimeScale::TT); - let obs = state.get_observer_from_uint16(observer); - let (geo_obs_pos, _) = obs.pvobs(&obs_mjd, state.get_ut1_provider())?; - let helio_obs_pos = obs.helio_position(state, &obs_mjd, &geo_obs_pos)?; - - Ok(Observation { - observer, - ra, - error_ra, - dec, - error_dec, - time, - observer_earth_position: geo_obs_pos, - observer_helio_position: helio_obs_pos, - }) - } - - /// Construct an [`Observation`] from precomputed observer positions. - /// - /// This constructor is a **fast-path alternative** to [`Observation::new`]: - /// it skips all ephemeris calls by directly injecting the observer’s - /// geocentric and heliocentric positions. This is useful in ingestion - /// pipelines (e.g. Parquet readers) where positions can be cached and - /// reused for multiple observations sharing the same `(observer, time)`. - /// - /// Arguments - /// ----------------- - /// * `observer` – Packed observer identifier (`u16`). - /// * `ra`, `error_ra` – Right ascension in radians and its 1-σ uncertainty (radians). - /// * `dec`, `error_dec` – Declination in radians and its 1-σ uncertainty (radians). - /// * `time` – Observation epoch in Modified Julian Date (TT scale). - /// * `observer_earth_position` – Geocentric observer position vector (AU, equatorial mean J2000). - /// * `observer_helio_position` – Heliocentric observer position vector (AU, equatorial mean J2000). - /// - /// Return - /// ---------- - /// * A fully initialized [`Observation`] where astrometric quantities are set - /// and observer positions are trusted to be externally consistent. - /// - /// Remarks - /// ------------ - /// * Use this constructor only when you can guarantee that positions were - /// computed consistently with the same environment (`Outfit`, UT1, ephemerides). - /// * All getter methods behave identically to those of [`Observation::new`]. - /// - /// See also - /// ------------ - /// * [`Observation::new`] – Computes positions internally (slower, but self-contained). - /// * [`Observer::pvobs`] – Routine for geocentric position/velocity. - /// * [`Observer::helio_position`] – Routine for heliocentric position. - #[allow(clippy::too_many_arguments)] - pub fn with_positions( - observer: u16, - ra: Radian, - error_ra: Radian, - dec: Radian, - error_dec: Radian, - time: MJD, - observer_earth_position: Vector3, - observer_helio_position: Vector3, - ) -> Self { - Self { - observer, - ra, - error_ra, - dec, - error_dec, - time, - observer_earth_position, - observer_helio_position, - } - } - - /// Get the observer heliocentric position at the observation epoch. - /// - /// Arguments - /// ----------------- - /// * *(none)* – Accessor method. - /// - /// Return - /// ---------- - /// * A copy of the `3D` position vector (AU, equatorial mean J2000) of the observer - /// at `self.time` (MJD TT). - /// - /// See also - /// ------------ - /// * [`Observation::new`] – Computes and stores this vector at construction. - /// * [`Observer::helio_position`] – Underlying routine used to compute the value. - pub fn get_observer_helio_position(&self) -> Vector3 { - self.observer_helio_position - } - - /// Get the observer geocentric position at the observation epoch. - /// - /// Arguments - /// ----------------- - /// * *(none)* – Accessor method. - /// - /// Return - /// ---------- - /// * A copy of the `3D` position vector (AU, equatorial mean J2000) of the observer - /// relative to the Earth’s center at `self.time` (MJD TT). - /// - /// Remarks - /// ------------ - /// * This vector is computed at construction via [`Observer::pvobs`]. - /// * Units are astronomical units (AU), in the equatorial mean J2000 frame. - /// - /// See also - /// ------------ - /// * [`Observation::new`] – Computes and stores this vector at construction. - /// * [`Observer::pvobs`] – Underlying routine used to compute the value. - pub fn get_observer_earth_position(&self) -> Vector3 { - self.observer_earth_position - } - - /// Get the observer from the observation - /// - /// Arguments - /// --------- - /// * `env_state`: a mutable reference to the Outfit instance - /// - /// Return - /// ------ - /// * The observer - pub fn get_observer<'a>(&self, env_state: &'a Outfit) -> &'a Observer { - env_state.get_observer_from_uint16(self.observer) - } - - /// Compute the apparent equatorial coordinates (RA, DEC) of a solar system body - /// as seen by this observation’s site at its epoch. - /// - /// Overview - /// ----------------- - /// This method determines the apparent sky position of a target body, - /// described by equinoctial orbital elements, as seen from the observing site - /// corresponding to this [`Observation`]. - /// - /// The computation steps are: - /// 1. **Orbit propagation** – Propagate the body’s state from its reference epoch to the observation epoch using a two-body model. - /// 2. **Reference frame handling** – Retrieve Earth’s barycentric position from the JPL ephemeris and transform to *ecliptic mean J2000*. - /// 3. **Observer position** – Compute the observer’s heliocentric position (Earth + site geocentric offset). - /// 4. **Light-time and aberration correction** – Form the observer–object vector and correct for aberration. - /// 5. **Conversion to equatorial coordinates** – Convert the corrected line-of-sight vector to (RA, DEC). - /// - /// Arguments - /// ----------------- - /// * `state` – Global environment providing ephemerides, UT1 provider, and frame utilities. - /// * `equinoctial_element` – Orbital elements of the target body. - /// - /// Return - /// ---------- - /// * `Result<(f64, f64), OutfitError>` – The apparent right ascension and declination `[rad]`. - /// - /// Units - /// ---------- - /// * Positions: AU - /// * Velocities: AU/day - /// * Angles: radians - /// * Time: MJD TT - /// - /// Errors - /// ---------- - /// Returns [`OutfitError`] if: - /// - Orbit propagation fails, - /// - Ephemeris data is unavailable, - /// - Reference-frame transformation fails. - /// - /// See also - /// ------------ - /// * [`EquinoctialElements::solve_two_body_problem`] – Orbit propagation. - /// * [`Observer::pvobs`] – Computes observer’s geocentric position. - /// * [`correct_aberration`] – Aberration correction. - /// * [`cartesian_to_radec`] – Convert Cartesian vectors to (RA, DEC). - pub fn compute_apparent_position( - &self, - state: &Outfit, - equinoctial_element: &EquinoctialElements, - ) -> Result<(f64, f64), OutfitError> { - // Hyperbolic/parabolic orbits (e >= 1) are not yet supported - if equinoctial_element.eccentricity() >= 1.0 { - return Err(OutfitError::InvalidOrbit( - "Eccentricity >= 1 is not yet supported".to_string(), - )); - } - - // 1. Propagate asteroid position/velocity in ecliptic J2000 - let (cart_pos_ast, cart_pos_vel, _) = equinoctial_element.solve_two_body_problem( - 0., - self.time - equinoctial_element.reference_epoch, - false, - )?; - - // 2. Observation time in TT - let obs_mjd = Epoch::from_mjd_in_time_scale(self.time, hifitime::TimeScale::TT); - - // 3. Earth's barycentric position in ecliptic J2000 - let (earth_position, _) = state.get_jpl_ephem()?.earth_ephemeris(&obs_mjd, false); - - // 4. get rotation from equatorial mean J2000 to ecliptic mean J2000 - let matrix_elc_transform = state.get_rot_equmj2000_to_eclmj2000(); - - let earth_pos_eclj2000 = matrix_elc_transform.transpose() * earth_position; - let cart_pos_ast_eclj2000 = matrix_elc_transform * cart_pos_ast; - let cart_pos_vel_eclj2000 = matrix_elc_transform * cart_pos_vel; - - // 5. Observer heliocentric position - let geo_obs_pos = self.observer_earth_position; - let xobs = geo_obs_pos + earth_pos_eclj2000; - let obs_on_earth = matrix_elc_transform * xobs; - - // 6. Relative position and aberration correction - let relative_position = cart_pos_ast_eclj2000 - obs_on_earth; - let corrected_pos = correct_aberration(relative_position, cart_pos_vel_eclj2000); - - // 7. Convert to RA/DEC - let (alpha, delta, _) = cartesian_to_radec(corrected_pos); - Ok((alpha, delta)) - } - - /// Compute the normalized squared astrometric residuals (RA, DEC) - /// between an observed position and a propagated ephemeris. - /// - /// Overview - /// ----------------- - /// This method compares the actual astrometric measurement stored in `self` - /// against the expected position of the target body propagated from - /// equinoctial elements. - /// It returns a scalar representing the sum of squared, normalized residuals - /// in RA and DEC. - /// - /// Arguments - /// ----------------- - /// * `state` – Global environment providing ephemerides and time conversions. - /// * `equinoctial_element` – Orbital elements of the target body. - /// - /// Return - /// ---------- - /// * `Result` – Dimensionless scalar value representing the weighted sum - /// of squared residuals. Equivalent to a chi² contribution for a single observation (without division by 2). - /// - /// Remarks - /// ---------- - /// * Residuals are normalized by the astrometric uncertainties `error_ra` and `error_dec`. - /// * RA residuals are multiplied by `cos(dec)` to account for projection effects. - /// * All angles are in radians. - /// - /// Errors - /// ---------- - /// Returns [`OutfitError`] if propagation or ephemeris lookup fails. - /// - /// See also - /// ------------ - /// * [`compute_apparent_position`](crate::observations::Observation::compute_apparent_position) – Used internally to obtain predicted RA/DEC. - /// * [`Observer::pvobs`] – Computes observer’s geocentric position. - /// * [`correct_aberration`] – Applies aberration correction. - /// * [`cartesian_to_radec`] – Converts 3D vectors to (RA, DEC). - /// * [`EquinoctialElements::solve_two_body_problem`] – Two-body propagation. - pub fn ephemeris_error( - &self, - state: &Outfit, - equinoctial_element: &EquinoctialElements, - ) -> Result { - let (alpha, delta) = self.compute_apparent_position(state, equinoctial_element)?; - - // ΔRA with wrapping to [-π, π] - let mut diff_alpha = (self.ra - alpha) % DPI; - if diff_alpha > PI { - diff_alpha -= DPI; - } - - let diff_delta = self.dec - delta; - - // Weighted RMS - let rms_ra = (self.dec.cos() * (diff_alpha / self.error_ra)).powi(2); - let rms_dec = (diff_delta / self.error_dec).powi(2); - - Ok(rms_ra + rms_dec) - } -} - -/// Apply stellar aberration correction to a relative position vector. -/// -/// This function computes the apparent position of a target object by applying -/// the first-order correction for stellar aberration due to the observer's velocity. -/// It assumes the classical limit (v ≪ c), using a linear time-delay model. -/// -/// Arguments -/// --------- -/// * `xrel`: relative position vector from observer to object \[AU\]. -/// * `vrel`: velocity of the observer relative to the barycenter \[AU/day\]. -/// -/// Returns -/// -------- -/// * Corrected position vector (same units and directionality as `xrel`), -/// shifted by the aberration effect. -/// -/// Formula -/// ------- -/// The corrected position is given by: -/// ```text -/// x_corr = xrel − (‖xrel‖ / c) · vrel -/// ``` -/// where `c` is the speed of light in AU/day (`VLIGHT_AU`). -/// -/// Remarks -/// ------- -/// * This function does **not** normalize the output. -/// * Suitable for use in astrometric modeling or when computing apparent direction -/// of celestial objects as seen from a moving observer. -pub fn correct_aberration(xrel: Vector3, vrel: Vector3) -> Vector3 { - let norm_vector = xrel.norm(); - let dt = norm_vector / VLIGHT_AU; - xrel - dt * vrel -} - -impl fmt::Display for Observation { - fn fmt(&self, f: &mut fmt::Formatter<'_>) -> fmt::Result { - // Extract numeric values (adapt if Radian/MJD are newtypes). - let ra_rad: f64 = self.ra; - let dec_rad: f64 = self.dec; - let sra_as: f64 = self.error_ra * RAD2ARC; - let sdec_as: f64 = self.error_dec * RAD2ARC; - let mjd_tt: f64 = self.time; - let jd_tt = mjd_tt + JDTOMJD; - - // Formatting precisions - let sec_prec = 3; - let pos_prec = 6; - - // Sexagesimal angles with carry-safe rounding - let (rh, rm, rs) = ra_hms_prec(ra_rad, sec_prec); - let (sgn, dd, dm, ds) = dec_sdms_prec(dec_rad, sec_prec); - let rs_s = fmt_ss(rs, sec_prec); - let ds_s = fmt_ss(ds, sec_prec); - - if f.alternate() { - // Pretty multi-line variant with {:#} - let site = self.observer; - let r_geo = fmt_vec3_au(&self.observer_earth_position, pos_prec); - let r_hel = fmt_vec3_au(&self.observer_helio_position, pos_prec); - - // Build TT epoch and derive both TT ISO & UTC ISO via hifitime. - let epoch_tt = Epoch::from_mjd_in_time_scale(mjd_tt, TimeScale::TT); - let iso_tt = iso_tt_from_epoch(epoch_tt, sec_prec); - let iso_utc = iso_utc_from_epoch(epoch_tt, sec_prec); - - writeln!(f, "Astrometric observation")?; - writeln!(f, "----------------------")?; - writeln!(f, "Site ID : {site}")?; - writeln!(f, "Epoch (TT) : MJD {mjd_tt:.6}, JD {jd_tt:.6}")?; - writeln!(f, "Epoch (ISO TT) : {iso_tt}")?; - writeln!(f, "Epoch (ISO UTC): {iso_utc}")?; - writeln!( - f, - "RA / σ : {rh:02}h {rm:02}m {rs_s}s (σ = {sra_as:.3}\" )" - )?; - writeln!( - f, - "DEC / σ : {sgn}{dd:02}° {dm:02}' {ds_s}\" (σ = {sdec_as:.3}\" )" - )?; - writeln!(f, "Observer (geo) : {r_geo}")?; - writeln!(f, "Observer (hel) : {r_hel}") - } else { - // Compact single line — keep the original contract so existing tests still pass. - let site = self.observer; - let r_geo = fmt_vec3_au(&self.observer_earth_position, pos_prec); - let r_hel = fmt_vec3_au(&self.observer_helio_position, pos_prec); - - write!( - f, - "Obs(site={site}, MJD={mjd_tt:.6} TT, RA={rh:02}h{rm:02}m{rs_s}s ± {sra_as:.3}\", \ -DEC={sgn}{dd:02}°{dm:02}'{ds_s}\" ± {sdec_as:.3}\", r_geo={r_geo}, r_hel={r_hel})" - ) - } - } -} - -#[cfg(test)] -#[cfg(feature = "jpl-download")] -mod test_observations { - - use crate::unit_test_global::OUTFIT_HORIZON_TEST; - - use super::*; - - mod tests_compute_apparent_position { - - use super::*; - use crate::unit_test_global::OUTFIT_HORIZON_TEST; - use approx::assert_relative_eq; - - /// Helper: simple circular equinoctial elements for a 1 AU, zero inclination orbit. - fn simple_circular_elements(epoch: f64) -> EquinoctialElements { - EquinoctialElements { - reference_epoch: epoch, - semi_major_axis: 1.0, - eccentricity_sin_lon: 0.0, - eccentricity_cos_lon: 0.0, - tan_half_incl_sin_node: 0.0, - tan_half_incl_cos_node: 0.0, - mean_longitude: 0.0, - } - } - - #[test] - fn test_compute_apparent_position_nominal() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let t_obs = 59000.0; // MJD - let equinoctial = simple_circular_elements(t_obs); - - let obs = Observation::new(state, observer_code, 0.0, 0.0, 0.0, 0.0, t_obs).unwrap(); - - let (ra, dec) = obs - .compute_apparent_position(state, &equinoctial) - .expect("Computation should succeed"); - - assert!(ra.is_finite()); - assert!(dec.is_finite()); - assert!((0.0..2.0 * std::f64::consts::PI).contains(&ra)); - assert!((-std::f64::consts::FRAC_PI_2..std::f64::consts::FRAC_PI_2).contains(&dec)); - } - - #[test] - fn test_compute_apparent_position_same_epoch() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let t_epoch = 60000.0; - let equinoctial = simple_circular_elements(t_epoch); - - let obs = Observation::new(state, observer_code, 0.0, 0.0, 0.0, 0.0, t_epoch).unwrap(); - - let (ra1, dec1) = obs.compute_apparent_position(state, &equinoctial).unwrap(); - let (ra2, dec2) = obs.compute_apparent_position(state, &equinoctial).unwrap(); - - // The same input should always produce the same result - assert_relative_eq!(ra1, ra2, epsilon = 1e-14); - assert_relative_eq!(dec1, dec2, epsilon = 1e-14); - } - - #[test] - fn test_apparent_position_for_distant_object() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - let t_obs = 59000.0; - let mut equinoctial = simple_circular_elements(t_obs); - - // Objet far away - equinoctial.semi_major_axis = 100.0; - - let obs = Observation::new(state, observer_code, 0.0, 0.0, 0.0, 0.0, t_obs).unwrap(); - - let (ra, dec) = obs - .compute_apparent_position(state, &equinoctial) - .expect("Should compute apparent position for distant object"); - - assert!(ra.is_finite()); - assert!(dec.is_finite()); - } - - #[test] - fn test_compute_apparent_position_propagation_failure() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - // Invalid orbital elements to force failure in solve_two_body_problem - let equinoctial = EquinoctialElements { - reference_epoch: 59000.0, - semi_major_axis: -1.0, // Physically invalid - eccentricity_sin_lon: 0.0, - eccentricity_cos_lon: 0.0, - tan_half_incl_sin_node: 0.0, - tan_half_incl_cos_node: 0.0, - mean_longitude: 0.0, - }; - - let obs = Observation::new(state, observer_code, 0.0, 0.0, 0.0, 0.0, 59000.0).unwrap(); - - let result = obs.compute_apparent_position(state, &equinoctial); - assert!(result.is_err(), "Invalid elements should trigger an error"); - } - - mod proptests_apparent_position { - use std::sync::Arc; - - use super::*; - use proptest::prelude::*; - - /// Strategy: generates random but reasonable equinoctial elements - /// for property-based tests. - fn arb_equinoctial_elements() -> impl Strategy { - ( - 58000.0..62000.0, // reference_epoch (MJD) - 0.5..30.0, // semi-major axis (AU) - -0.5..0.5, // h = e * sin(Ω+ω) - -0.5..0.5, // k = e * cos(Ω+ω) - -0.5..0.5, // p = tan(i/2)*sin Ω - -0.5..0.5, // q = tan(i/2)*cos Ω - 0.0..(2.0 * std::f64::consts::PI), // mean longitude (rad) - ) - .prop_map(|(epoch, a, h, k, p, q, lambda)| { - EquinoctialElements { - reference_epoch: epoch, - semi_major_axis: a, - eccentricity_sin_lon: h, - eccentricity_cos_lon: k, - tan_half_incl_sin_node: p, - tan_half_incl_cos_node: q, - mean_longitude: lambda, - } - }) - } - - /// Strategy: generates random observer locations on Earth. - /// - longitude in [-180, 180] degrees - /// - latitude in [-90, 90] degrees - /// - elevation from 0 to 5 km - fn arb_observer() -> impl Strategy { - (-180.0..180.0, -90.0..90.0, 0.0..5.0).prop_map(|(lon, lat, elev)| { - Observer::new(lon, lat, elev, None, None, None).unwrap() - }) - } - - /// Strategy: generates equinoctial elements with a wide range, - /// including extreme eccentricities and inclinations. - fn arb_extreme_equinoctial_elements() -> impl Strategy { - ( - 58000.0..62000.0, - 0.1..50.0, - -0.99..0.99, - -0.99..0.99, - -1.0..1.0, - -1.0..1.0, - 0.0..(2.0 * std::f64::consts::PI), - ) - .prop_map(|(epoch, a, h, k, p, q, lambda)| EquinoctialElements { - reference_epoch: epoch, - semi_major_axis: a, - eccentricity_sin_lon: h, - eccentricity_cos_lon: k, - tan_half_incl_sin_node: p, - tan_half_incl_cos_node: q, - mean_longitude: lambda, - }) - // Filter out cases where eccentricity >= 1 - .prop_filter( - "Only bound (elliptical) orbits are supported", - |elem: &EquinoctialElements| { - let e = (elem.eccentricity_sin_lon.powi(2) - + elem.eccentricity_cos_lon.powi(2)) - .sqrt(); - e < 0.99 - }, - ) - } - - proptest! { - /// Property test: RA and DEC are always finite and in the expected ranges. - #[test] - fn proptest_ra_dec_are_finite_and_in_range( - equinoctial in arb_equinoctial_elements(), - obs_time in 58000.0f64..62000.0 - ) { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let obs = Observation::new( - state, - observer_code, - 0.0, - 0.0, - 0.0, - 0.0, - obs_time, - ).unwrap(); - - let result = obs.compute_apparent_position(state, &equinoctial); - - if let Ok((ra, dec)) = result { - // Invariant: returned values must be finite - prop_assert!(ra.is_finite()); - prop_assert!(dec.is_finite()); - - // RA must be in [0, 2π), DEC must be in [-π/2, π/2] - prop_assert!((0.0..2.0 * std::f64::consts::PI).contains(&ra)); - prop_assert!((-std::f64::consts::FRAC_PI_2..std::f64::consts::FRAC_PI_2).contains(&dec)); - } - } - - /// Property test: Calling the function twice with the same inputs must produce exactly - /// the same output (determinism). - #[test] - fn proptest_repeatability( - equinoctial in arb_equinoctial_elements(), - obs_time in 58000.0f64..62000.0 - ) { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let obs = Observation::new( - state, - observer_code, - 0.0, - 0.0, - 0.0, - 0.0, - obs_time, - ).unwrap(); - - let r1 = obs.compute_apparent_position(state, &equinoctial); - let r2 = obs.compute_apparent_position(state, &equinoctial); - - // Invariant: repeated computation with the same input should be identical - prop_assert_eq!(r1, r2); - } - - /// Property test: A very small change in observation time (1e-3 days ≈ 1.4 min) - /// should not cause huge jumps in the resulting RA/DEC. - #[test] - fn proptest_small_time_change_has_small_effect( - equinoctial in arb_equinoctial_elements(), - obs_time in 58000.0f64..62000.0 - ) { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let obs = Observation::new( - state, - observer_code, - 0.0, - 0.0, - 0.0, - 0.0, - obs_time, - ).unwrap(); - - let obs_eps = Observation { - time: obs_time + 1e-3, // shift by 1.4 minutes - ..obs - }; - - let r1 = obs.compute_apparent_position(state, &equinoctial); - let r2 = obs_eps.compute_apparent_position(state, &equinoctial); - - if let (Ok((ra1, dec1)), Ok((ra2, dec2))) = (r1, r2) { - let dra = (ra1 - ra2).abs(); - let ddec = (dec1 - dec2).abs(); - - // Invariant: no catastrophic jumps (> 1 radian) for a small time shift - prop_assert!(dra < 1.0); - prop_assert!(ddec < 1.0); - } - } - } - - proptest! { - /// Property: RA/DEC remain finite and in valid ranges for extreme orbits and random observers. - #[test] - fn proptest_ra_dec_valid_for_extreme_orbits_and_observers( - equinoctial in arb_extreme_equinoctial_elements(), - observer in arb_observer(), - obs_time in 58000.0f64..62000.0 - ) { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.add_observer_internal(Arc::new(observer)); - - let obs = Observation::new( - state, - observer_code, - 0.0, - 0.0, - 0.0, - 0.0, - obs_time, - ).unwrap(); - - let result = obs.compute_apparent_position(state, &equinoctial); - - if let Ok((ra, dec)) = result { - // Values must be finite - prop_assert!(ra.is_finite()); - prop_assert!(dec.is_finite()); - // Angles must be within their valid intervals - prop_assert!((0.0..2.0 * std::f64::consts::PI).contains(&ra)); - prop_assert!((-std::f64::consts::FRAC_PI_2..std::f64::consts::FRAC_PI_2).contains(&dec)); - } - } - } - - #[test] - fn test_hyperbolic_orbit_returns_error() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let obs = - Observation::new(state, observer_code, 0.0, 0.0, 0.0, 0.0, 59000.0).unwrap(); - - let equinoctial = EquinoctialElements { - reference_epoch: 59000.0, - semi_major_axis: 1.0, - eccentricity_sin_lon: 0.8, - eccentricity_cos_lon: 0.8, // e ≈ 1.13 > 1 - tan_half_incl_sin_node: 0.0, - tan_half_incl_cos_node: 0.0, - mean_longitude: 0.0, - }; - - let result = obs.compute_apparent_position(state, &equinoctial); - assert!( - result.is_err(), - "Hyperbolic or parabolic orbits should currently return an error" - ); - } - } - } - - #[test] - fn test_new_observation() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let observation = - Observation::new(state, observer_code, 1.0, 0.1, 2.0, 0.2, 59000.0).unwrap(); - assert_eq!( - observation, - Observation { - observer: 2, - ra: 1.0, - error_ra: 0.1, - dec: 2.0, - error_dec: 0.2, - time: 59000.0, - observer_earth_position: [ - -1.4662164592060655e-6, - 4.2560356749756634e-5, - -2.1126391698196086e-6 - ] - .into(), - observer_helio_position: [ - -0.35113019606349866, - -0.8726512942340473, - -0.37829699890414364 - ] - .into(), - } - ); - - let observation_2 = Observation::new( - state, - 2, - 343.097_375, - 2.777_777_777_777_778E-6, - -14.784833333333333, - 2.777_777_777_777_778E-5, - 59001.0, - ) - .unwrap(); - - assert_eq!( - observation_2, - Observation { - observer: 2, - ra: 343.097375, - error_ra: 2.777777777777778e-6, - dec: -14.784833333333333, - error_dec: 2.777777777777778e-5, - time: 59001.0, - observer_earth_position: [ - -2.1521316017998277e-6, - 4.2531873012231404e-5, - -2.0988352183088593e-6 - ] - .into(), - observer_helio_position: [ - -0.33522248840408125, - -0.8780465618894304, - -0.380635845615707 - ] - .into(), - } - ); - } - - mod tests_ephemeris_error { - use super::*; - use crate::unit_test_global::OUTFIT_HORIZON_TEST; - use approx::assert_relative_eq; - - fn simple_equinoctial(epoch: f64) -> EquinoctialElements { - EquinoctialElements { - reference_epoch: epoch, - semi_major_axis: 1.0, - eccentricity_sin_lon: 0.0, - eccentricity_cos_lon: 0.0, - tan_half_incl_sin_node: 0.0, - tan_half_incl_cos_node: 0.0, - mean_longitude: 0.0, - } - } - - #[test] - fn test_ephem_error() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let obs = Observation::new( - state, - observer_code, - 1.7899347771316527, - 1.770_024_520_608_546E-6, - 0.778_996_538_107_973_6, - 1.259_582_891_829_317_7E-6, - 57070.262067592594, - ) - .unwrap(); - - let equinoctial_element = EquinoctialElements { - reference_epoch: 57_049.242_334_573_75, - semi_major_axis: 1.8017360713154256, - eccentricity_sin_lon: 0.269_373_680_909_227_2, - eccentricity_cos_lon: 8.856_415_260_013_56E-2, - tan_half_incl_sin_node: 8.089_970_166_396_302E-4, - tan_half_incl_cos_node: 0.10168201109730375, - mean_longitude: 1.6936970079414786, - }; - - let rms_error = obs.ephemeris_error(&OUTFIT_HORIZON_TEST.0, &equinoctial_element); - assert_eq!(rms_error.unwrap(), 75.00445641224026); - } - - /// When the observed RA/DEC exactly match the propagated RA/DEC, - /// the ephemeris_error must be zero. - #[test] - fn test_zero_error_when_positions_match() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let t_obs = 59000.0; - let equinoctial = simple_equinoctial(t_obs); - - // Compute the propagated position - let obs = Observation::new(state, observer_code, 0.0, 1e-6, 0.0, 1e-6, t_obs).unwrap(); - let (alpha, delta) = obs.compute_apparent_position(state, &equinoctial).unwrap(); - - // New observation with exact same RA/DEC - let obs_match = - Observation::new(state, observer_code, alpha, 1e-6, delta, 1e-6, t_obs).unwrap(); - - let error = obs_match.ephemeris_error(state, &equinoctial).unwrap(); - assert_relative_eq!(error, 0.0, epsilon = 1e-14); - } - - /// Error grows if RA is off by a known amount - #[test] - fn test_error_increases_with_offset() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let t_obs = 59000.0; - let equinoctial = simple_equinoctial(t_obs); - - let base_obs = Observation { - observer: observer_code, - ra: 0.0, - error_ra: 1e-3, - dec: 0.0, - error_dec: 1e-3, - time: t_obs, - observer_earth_position: Vector3::zeros(), - observer_helio_position: Vector3::zeros(), - }; - let (alpha, delta) = base_obs - .compute_apparent_position(state, &equinoctial) - .unwrap(); - - // Same dec, but RA offset by 1 milliradian - let obs_offset = Observation { - observer: 0, - ra: alpha + 1e-3, - error_ra: 1e-3, - dec: delta, - error_dec: 1e-3, - time: t_obs, - observer_earth_position: Vector3::zeros(), - observer_helio_position: Vector3::zeros(), - }; - - let err = obs_offset.ephemeris_error(state, &equinoctial).unwrap(); - assert!(err > 0.0); - } - - /// Check that wrapping of RA (close to 2π) does not affect the error - #[test] - fn test_ra_wrapping_invariance() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let t_obs = 59000.0; - let equinoctial = simple_equinoctial(t_obs); - - let base_obs = - Observation::new(state, observer_code, 0.0, 1e-6, 0.0, 1e-6, t_obs).unwrap(); - let (alpha, delta) = base_obs - .compute_apparent_position(state, &equinoctial) - .unwrap(); - - // Same position but RA shifted by ±2π - let obs_wrapped = Observation::new( - state, - observer_code, - alpha + std::f64::consts::TAU, - 1e-6, - delta, - 1e-6, - t_obs, - ) - .unwrap(); - - let err1 = obs_wrapped.ephemeris_error(state, &equinoctial).unwrap(); - assert_relative_eq!(err1, 0.0, epsilon = 1e-12); - } - - /// When RA/DEC uncertainties are very large, error is small even with a mismatch. - #[test] - fn test_large_uncertainty_downweights_error() { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.uint16_from_mpc_code(&"F51".to_string()); - - let t_obs = 59000.0; - let equinoctial = simple_equinoctial(t_obs); - - let base_obs = - Observation::new(state, observer_code, 0.0, 1.0, 0.0, 1.0, t_obs).unwrap(); - let (alpha, delta) = base_obs - .compute_apparent_position(state, &equinoctial) - .unwrap(); - - let obs_large_uncertainty = Observation::new( - state, - observer_code, - alpha + 0.1, - 10.0, - delta + 0.1, - 10.0, - t_obs, - ) - .unwrap(); - - let err = obs_large_uncertainty - .ephemeris_error(state, &equinoctial) - .unwrap(); - assert!( - err < 1.0, - "Large uncertainties should reduce the error contribution" - ); - } - - mod proptests_ephemeris_error { - use std::sync::Arc; - - use super::*; - use proptest::prelude::*; - - fn arb_observer() -> impl Strategy { - (-180.0..180.0, -90.0..90.0, 0.0..5.0).prop_map(|(lon, lat, elev)| { - Observer::new(lon, lat, elev, None, None, None).unwrap() - }) - } - - fn arb_elliptical_equinoctial() -> impl Strategy { - ( - 58000.0..62000.0, - 0.5..20.0, - -0.8..0.8, - -0.8..0.8, - -0.8..0.8, - -0.8..0.8, - 0.0..std::f64::consts::TAU, - ) - .prop_map(|(epoch, a, h, k, p, q, l)| EquinoctialElements { - reference_epoch: epoch, - semi_major_axis: a, - eccentricity_sin_lon: h, - eccentricity_cos_lon: k, - tan_half_incl_sin_node: p, - tan_half_incl_cos_node: q, - mean_longitude: l, - }) - .prop_filter("Bound orbits only", |e: &EquinoctialElements| { - e.eccentricity() < 1.0 - }) - } - - proptest! { - /// Property: error is always non-negative and finite for valid inputs - #[test] - fn proptest_error_is_non_negative( - equinoctial in arb_elliptical_equinoctial(), - observer in arb_observer(), - obs_time in 58000.0f64..62000.0 - ) { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.add_observer_internal(Arc::new(observer)); - let obs = Observation::new(state, observer_code, - 0.0, - 1e-3, - 0.0, - 1e-3, - obs_time,).unwrap(); - - let result = obs.ephemeris_error(state, &equinoctial); - if let Ok(val) = result { - prop_assert!(val.is_finite()); - prop_assert!(val >= 0.0); - } - } - - /// Property: If uncertainties are huge, the error must be small - #[test] - fn proptest_error_downweights_large_uncertainties( - equinoctial in arb_elliptical_equinoctial(), - observer in arb_observer(), - obs_time in 58000.0f64..62000.0 - ) { - let state = &mut OUTFIT_HORIZON_TEST.0.clone(); - let observer_code = state.add_observer_internal(Arc::new(observer)); - let obs = Observation::new(state, observer_code, - 0.5, - 100.0, - 0.5, - 100.0, - obs_time,).unwrap(); - - let result = obs.ephemeris_error(state, &equinoctial); - if let Ok(val) = result { - prop_assert!(val < 1.0); - } - } - } - } - } - - #[cfg(test)] - mod display_obs_tests { - use super::*; - use nalgebra::Vector3; - - // --- Helpers ------------------------------------------------------------- - - /// Convert arcseconds to radians. - fn arcsec_to_rad(asx: f64) -> f64 { - asx / 206_264.806_247_096_37 - } - - /// Build an Observation with full control on fields. - /// This stays in the same module (pub(crate) fields are accessible here). - #[allow(clippy::too_many_arguments)] - fn make_obs( - site: u16, - ra_rad: f64, - dec_rad: f64, - sra_arcsec: f64, - sdec_arcsec: f64, - mjd_tt: f64, - geo: (f64, f64, f64), - hel: (f64, f64, f64), - ) -> Observation { - Observation { - observer: site, - ra: Radian::from(ra_rad), - error_ra: Radian::from(arcsec_to_rad(sra_arcsec)), - dec: Radian::from(dec_rad), - error_dec: Radian::from(arcsec_to_rad(sdec_arcsec)), - time: MJD::from(mjd_tt), - observer_earth_position: Vector3::new(geo.0, geo.1, geo.2), - observer_helio_position: Vector3::new(hel.0, hel.1, hel.2), - } - } - - // --- Tests --------------------------------------------------------------- - - #[test] - fn display_compact_basic() { - // Case: RA=0, DEC=0, uncertainties = 1.0 arcsec, simple positions. - let obs = make_obs( - 809, - 0.0, - 0.0, - 1.0, - 1.0, - 60000.123456, // MJD (TT) - (0.123456789, -1.0, 0.000042), - (0.0, 1.234567, -0.5), - ); - - let s = format!("{obs}"); - - // Site and MJD - assert!( - s.contains("site=809"), - "site field not present/incorrect: {s}" - ); - assert!( - s.contains("MJD=60000.123456"), - "MJD formatting to 6 decimals expected: {s}" - ); - - // RA/DEC with uncertainties in arcsec; 3 decimals on seconds and uncertainties. - // RA=0 -> 00h00m00.000s; DEC=+00°00'00.000" - assert!( - s.contains("RA=00h00m00.000s ± 1.000\""), - "RA sexagesimal or sigma not formatted as expected: {s}" - ); - assert!( - s.contains("DEC=+00°00'00.000\" ± 1.000\""), - "DEC sexagesimal or sigma not formatted as expected: {s}" - ); - - // JD = MJD + 2400000.5 is only printed in pretty mode, so not checked here. - - // Vectors formatted with 6 decimals and 'AU' tag - assert!( - s.contains("r_geo=[ 0.123457, -1.000000, 0.000042 ] AU"), - "Geocentric vector formatting/precision mismatch: {s}" - ); - assert!( - s.contains("r_hel=[ 0.000000, 1.234567, -0.500000 ] AU"), - "Heliocentric vector formatting/precision mismatch: {s}" - ); - } - - #[test] - fn display_pretty_multiline() { - // Non-zero RA/DEC to exercise general formatting. - // RA = 2h 30m 15s -> in radians; DEC = +12° 34' 56" - let ra_hours = 2.0 + 30.0 / 60.0 + 15.0 / 3600.0; - let ra_rad = ra_hours * std::f64::consts::PI / 12.0; - let dec_deg: f64 = 12.0 + 34.0 / 60.0 + 56.0 / 3600.0; - let dec_rad = dec_deg.to_radians(); - - let obs = make_obs( - 500, - ra_rad, - dec_rad, - 0.321, // arcsec - 0.789, // arcsec - 60200.5, - (1.0, 2.0, 3.0), - (-0.1, 0.2, -0.3), - ); - - let s = format!("{obs:#}"); - - // Header and labels should be present (human-readable multi-line) - assert!( - s.starts_with("Astrometric observation"), - "Pretty header missing: {s}" - ); - assert!( - s.contains("Site ID : 500"), - "Pretty site line missing: {s}" - ); - - // Epoch line with MJD and JD - assert!( - s.contains("Epoch (TT) : MJD 60200.500000, JD 2460201.000000"), - "Epoch line with JD=MJD+2400000.5 expected: {s}" - ); - - // RA/σ line (check fragments to avoid locale/spacing issues) - assert!(s.contains("RA / σ : "), "RA line missing: {s}"); - assert!( - s.contains("h") && s.contains("m") && s.contains("s"), - "RA HMS units missing: {s}" - ); - assert!( - s.contains("(σ = 0.321"), - "RA sigma arcsec missing/incorrect: {s}" - ); - - // DEC/σ line with sign and DMS glyphs - assert!(s.contains("DEC / σ : +"), "DEC sign missing: {s}"); - assert!( - s.contains("°") && s.contains("'") && s.contains("\""), - "DEC units missing: {s}" - ); - assert!( - s.contains("(σ = 0.789"), - "DEC sigma arcsec missing/incorrect: {s}" - ); - - // Vectors lines - assert!( - s.contains("Observer (geo) : [ 1.000000, 2.000000, 3.000000 ] AU"), - "Geo vector line mismatch: {s}" - ); - assert!( - s.contains("Observer (hel) : [ -0.100000, 0.200000, -0.300000 ] AU"), - "Hel vector line mismatch: {s}" - ); - } - - #[test] - fn ra_wraps_into_24h() { - // RA slightly negative should wrap to near 24h in display. - let tiny = 1e-6; - let obs = make_obs( - 1, - -tiny, // slightly negative angle - 0.0, - 0.1, - 0.1, - 59000.0, - (0.0, 0.0, 0.0), - (0.0, 0.0, 0.0), - ); - - let s = format!("{obs}"); - - // Expect "23h59m..." rather than negative hours - assert!( - s.contains("RA=23h59m") || s.contains("RA=24h00m"), - "RA should wrap to [0, 24h): {s}" - ); - assert!( - !s.contains("-"), - "RA string must not contain a negative sign after wrapping: {s}" - ); - } - - #[test] - fn dec_negative_sign_is_preserved() { - // DEC = -10° 00' 00" - let dec_rad = (-10.0f64).to_radians(); - let obs = make_obs( - 2, - 0.0, - dec_rad, - 0.5, - 0.5, - 59000.0, - (0.0, 0.0, 0.0), - (0.0, 0.0, 0.0), - ); - - let s = format!("{obs}"); - - assert!( - s.contains("DEC=-10°00'00.000\""), - "Negative DEC sign or DMS formatting incorrect: {s}" - ); - } - - #[test] - fn uncertainties_are_in_arcseconds() { - // Store uncertainties in radians corresponding to 2.345 arcsec. - let asx = 2.345; - let obs = make_obs( - 3, - 0.0, - 0.0, - asx, // provided in arcsec, helper converts to rad - asx, - 60001.0, - (0.0, 0.0, 0.0), - (0.0, 0.0, 0.0), - ); - - let s1 = format!("{obs}"); - let s2 = format!("{obs:#}"); - - // Both compact and pretty should surface the same arcsec value to 3 decimals. - assert!( - s1.contains("± 2.345\"") && s2.contains("(σ = 2.345"), - "Arcsecond uncertainties not printed as expected.\nCompact: {s1}\nPretty:\n{s2}" - ); - } - - #[test] - fn vector_precision_and_units() { - // Ensure 6-decimal rounding and AU suffix are stable. - let obs = make_obs( - 4, - 0.0, - 0.0, - 1.0, - 1.0, - 60010.0, - (0.9999996, -0.9999996, 0.12345649), - (1.23456749, -1.23456751, 2.00000049), - ); - - let s = format!("{obs}"); - - // Rounded at 6 decimals, with AU suffix. - assert!( - s.contains("r_geo=[ 1.000000, -1.000000, 0.123456 ] AU"), - "Geo rounding/units mismatch: {s}" - ); - assert!( - s.contains("r_hel=[ 1.234567, -1.234568, 2.000000 ] AU"), - "Hel rounding/units mismatch: {s}" - ); - } - } -} diff --git a/src/observations/observations_ext.rs b/src/observations/observations_ext.rs deleted file mode 100644 index b94f22e..0000000 --- a/src/observations/observations_ext.rs +++ /dev/null @@ -1,1245 +0,0 @@ -//! # Observation extensions for orbit determination -//! -//! This module extends the base [`Observations`] collection with methods -//! essential for **initial orbit determination (IOD)** and orbit quality -//! assessment. -//! It provides two core traits: -//! -//! ## [`ObservationsExt`] -//! -//! High-level utilities for processing and analyzing sets of [`Observation`]s: -//! -//! - **Triplet generation**: [`compute_triplets`](ObservationsExt::compute_triplets) -//! Build optimized triplets of three observations for Gauss IOD. -//! -//! - **RMS evaluation**: [`select_rms_interval`](ObservationsExt::select_rms_interval), -//! [`rms_orbit_error`](ObservationsExt::rms_orbit_error) -//! Select subsets of observations around a triplet and compute RMS residuals -//! for candidate orbits. -//! -//! - **Error handling**: [`apply_batch_rms_correction`](ObservationsExt::apply_batch_rms_correction) -//! Apply statistical corrections to observational errors based on temporal clustering. -//! -//! - **Uncertainty extraction**: [`extract_errors`](ObservationsExt::extract_errors) -//! Retrieve RA/DEC uncertainties for a given triplet. -//! -//! ## [`ObservationIOD`] -//! -//! A high-level trait encapsulating the full **initial orbit determination workflow**: -//! -//! 1. Apply uncertainty calibration with [`ObservationsExt::apply_batch_rms_correction`], -//! 2. Generate candidate triplets with [`ObservationsExt::compute_triplets`], -//! 3. Perform Monte Carlo perturbations to simulate astrometric noise, -//! 4. Run the Gauss method on each triplet, -//! 5. Select the orbit with the lowest RMS over the full arc using [`ObservationsExt::rms_orbit_error`]. -//! -//! This workflow is designed for **short arcs** (newly discovered asteroids, comets, NEOs), -//! where only a handful of observations are available. -//! -//! ## Typical usage -//! -//! ```rust, no_run -//! use rand::{rngs::StdRng, SeedableRng}; -//! use outfit::initial_orbit_determination::IODParams; -//! use outfit::constants::Observations; -//! use outfit::observations::observations_ext::ObservationIOD; -//! -//! let params = IODParams::builder() -//! .n_noise_realizations(50) -//! .noise_scale(1.0) -//! .dtmax(30.0) -//! .max_triplets(20) -//! .build().unwrap(); -//! -//! let observations: Observations = unimplemented!(); // Load observations here -//! let state = unimplemented!(); // Outfit environment -//! let error_model = unimplemented!(); // Astrometric error model -//! let mut rng = StdRng::seed_from_u64(123); -//! -//! let (best_orbit, rms) = observations.estimate_best_orbit( -//! &state, &error_model, &mut rng, ¶ms -//! ).unwrap(); -//! println!("Best preliminary orbit RMS = {rms}"); -//! ``` -//! -//! ## References -//! -//! * Danby, J.M.A. (1992). *Fundamentals of Celestial Mechanics* (2nd ed.). -//! Willmann-Bell. Classic reference for Gauss, Laplace, and related IOD methods. -//! -//! * Milani, A., & Gronchi, G. F. (2009). *Theory of Orbit Determination*. -//! Cambridge University Press. [doi:10.1017/CBO9781139175371](https://doi.org/10.1017/CBO9781139175371) -//! -//! * Carpino, M., Milani, A., & Chesley, S. R. (2003). *OrbFit: Software for Preliminary Orbit Determination*. -//! [https://adams.dm.unipi.it/orbfit/](https://adams.dm.unipi.it/orbfit/) -//! -//! ## See also -//! -//! - [`Observation`] – Representation of a single astrometric measurement. -//! - [`GaussObs`] – Structure encoding a triplet of observations for Gauss IOD. -//! - [`GaussResult`] – Output of the Gauss preliminary orbit solver. -//! - [`IODParams`] – Parameters controlling IOD (triplet constraints, noise realizations). -use itertools::Itertools; -use nalgebra::Vector3; -use std::{collections::VecDeque, ops::ControlFlow}; - -use crate::{ - constants::{Observations, Radian}, - error_models::ErrorModel, - initial_orbit_determination::{gauss::GaussObs, gauss_result::GaussResult, IODParams}, - observations::{triplets_iod::generate_triplets, Observation}, - orbit_type::equinoctial_element::EquinoctialElements, - outfit::Outfit, - outfit_errors::OutfitError, -}; - -/// Extension trait for [`Observations`] providing high-level operations -/// commonly used in orbit determination workflows. -/// -/// This trait adds methods to process and analyze a collection of -/// astrometric [`Observation`] objects, including: -/// -/// * Selection of observation triplets optimized for initial orbit determination (IOD). -/// * Selection of subsets of observations for root-mean-square (RMS) error calculation. -/// * Computation of orbit quality metrics (RMS of astrometric residuals). -/// * Statistical corrections of observational errors based on temporal clustering. -/// * Extraction of astrometric uncertainties for given observation indices. -/// -/// # Typical usage -/// -/// This trait is intended to be implemented on: -/// -/// ```rust, ignore -/// pub type Observations = SmallVec<[Observation; 6]>; -/// ``` -/// -/// It provides functionality essential for the Gauss method and related -/// algorithms used in preliminary orbit determination. -/// -/// # Provided methods -/// - [`compute_triplets`](ObservationsExt::compute_triplets): -/// Build time-filtered triplets of observations, sorted by weight. -/// - [`select_rms_interval`](ObservationsExt::select_rms_interval): -/// Given a triplet, determine which observations lie in an expanded time window. -/// - [`rms_orbit_error`](ObservationsExt::rms_orbit_error): -/// Evaluate the fit of an orbit by computing RMS residuals. -/// - [`apply_batch_rms_correction`](ObservationsExt::apply_batch_rms_correction): -/// Apply correlation-based scaling factors to astrometric errors based on temporal clustering. -/// - [`extract_errors`](ObservationsExt::extract_errors): -/// Retrieve the RA/DEC uncertainties for a given triplet of observations. -/// -/// # See also -/// * [`GaussObs`] – Data structure used to represent a triplet of observations. -/// * [`Outfit`] – Global state providing ephemerides and reference frames. -/// * [`KeplerianElements`](crate::orbit_type::keplerian_element::KeplerianElements) – Orbital elements used to propagate orbits. -/// * [`Observation`] – Individual observation data structure. -/// -/// # References -/// -/// * Danby, J.M.A. (1992). *Fundamentals of Celestial Mechanics* (2nd ed.). -/// Willmann-Bell. -/// Classic reference for preliminary orbit determination methods -/// (Gauss, Laplace, Vaisala) and iterative improvement techniques. -/// -/// * Milani, A., & Gronchi, G. F. (2009). *Theory of Orbit Determination*. -/// Cambridge University Press. -/// Comprehensive modern treatment of statistical orbit determination, -/// including least-squares methods, weighting, and correlation handling. -/// [https://doi.org/10.1017/CBO9781139175371](https://doi.org/10.1017/CBO9781139175371) -/// -/// * Carpino, M., Milani, A., & Chesley, S. R. (2003). *OrbFit: Software for Preliminary Orbit Determination*. -/// Technical documentation distributed with the OrbFit package: -/// [https://adams.dm.unipi.it/orbfit/](https://adams.dm.unipi.it/orbfit/) -/// -/// These references describe the algorithms used for: -/// - Building and filtering observation triplets (Gauss method) -/// - Propagating trial orbits and refining them via differential corrections -/// - Handling of astrometric uncertainties and RMS weighting. -/// -/// This trait is central to orbit determination pipelines and is designed -/// to work with small batches of observations (often < 100 per object). -pub trait ObservationsExt { - /// Compute **time-feasible, best-K** triplets of observations for Gauss IOD, - /// leveraging a lazy **index stream** and a bounded **max-heap** on spacing weight. - /// - /// Overview - /// ----------------- - /// This method is a convenience wrapper around [`generate_triplets`]. It operates - /// directly on `self` (the current observation set) and returns up to `max_triplet` - /// **best-scored** candidates for the Gauss preliminary solution. Internally it: - /// - /// 1) Uses a `TripletIndexGenerator` that: - /// - sorts epochs in place, - /// - downsamples to at most `max_obs_for_triplets` (uniform with edges), - /// - lazily **streams reduced indices** `(first, middle, last)` constrained by: - /// `dt_min ≤ t[last] − t[first] ≤ dt_max`. - /// 2) Scores each feasible triplet with [`triplet_weight`](crate::observations::triplets_iod::triplet_weight) against `optimal_interval_time`. - /// 3) Keeps only the **K** smallest weights in a bounded **max-heap** (best-K selection). - /// 4) Materializes the survivors as [`GaussObs`] by (re)borrowing `self` immutably. - /// - /// Compared to brute-force `O(n³)`, the time-windowed enumeration drives the effective - /// cost toward ~`O(n²)` in typical time distributions, plus `O(n log K)` for heap updates. - /// - /// Arguments - /// ----------------- - /// * `dt_min` – Minimum allowed timespan `[same units as Observation::time]` between the first and last epoch of a triplet. - /// * `dt_max` – Maximum allowed timespan between the first and last epoch of a triplet. - /// * `optimal_interval_time` – Target per-gap spacing (e.g., days) used by [`triplet_weight`](crate::observations::triplets_iod::triplet_weight). - /// * `max_obs_for_triplets` – Upper bound on observations kept after downsampling (uniform with endpoints). - /// * `max_triplet` – Number `K` of best-scoring triplets to return. - /// - /// Return - /// ---------- - /// * A `Vec` of length `≤ max_triplet`, **sorted by increasing weight** - /// (best geometric spacing first), ready to be passed to `GaussObs::prelim_orbit`. - /// - /// Remarks - /// ------------- - /// * Sorting is **in-place**; call sites should not rely on original ordering afterward. - /// * The generator avoids overlapping borrows of `self`; only the final K triplets are materialized. - /// * For robustness studies, each returned triplet can be expanded with - /// `GaussObs::realizations_iter` (lazy Monte-Carlo noise). - /// - /// Complexity - /// ----------------- - /// * Enumeration: ~`O(n²)` (per-anchor time window). - /// * Selection: `O(n log K)` (bounded max-heap). - /// * Space: `O(1)` per yielded candidate; only K triplets are allocated at the end. - /// - /// See also - /// ------------ - /// * [`generate_triplets`] – Low-level function performing the selection (index stream + heap + materialization). - /// * [`TripletIndexGenerator`](crate::observations::triplets_generator::TripletIndexGenerator) – Lazy stream of reduced indices constrained by `(dt_min, dt_max)`. - /// * [`triplet_weight`](crate::observations::triplets_iod::triplet_weight) – Spacing heuristic around `optimal_interval_time`. - /// * [`GaussObs::realizations_iter`] – On-the-fly noisy realizations for a given triplet. - fn compute_triplets( - &mut self, - dt_min: f64, - dt_max: f64, - optimal_interval_time: f64, - max_obs_for_triplets: usize, - max_triplet: u32, - ) -> Vec; - - /// Select the interval of observations for RMS calculation. - /// - /// This function selects the interval of observations for RMS calculation based on the provided triplet. - /// It computes the maximum allowed interval and finds the start and end indices of the observations - /// within that interval. - /// - /// Arguments - /// --------- - /// * `triplets`: A reference to a `GaussObs` representing the triplet of observations. - /// * `extf`: A `f64` representing the external factor for the interval calculation. - /// * `dtmax`: A `f64` representing the maximum allowed interval. - /// - /// Return - /// ------ - /// * A `Result` containing a tuple of start and end indices of the observations within the interval, - /// or an `OutfitError` if an error occurs. - fn select_rms_interval( - &self, - triplets: &GaussObs, - extf: f64, - dtmax: f64, - ) -> Result<(usize, usize), OutfitError>; - - /// Evaluate the orbit quality by computing the RMS of normalized astrometric residuals - /// over a time window centered on a Gauss triplet. - /// - /// Scientific context - /// ------------------- - /// This function measures how well a preliminary orbit reproduces the observed - /// astrometry (RA, DEC). It computes the **root-mean-square (RMS)** of the - /// normalized residuals between predicted and observed positions, aggregated over - /// a set of observations surrounding a Gauss triplet. - /// - /// Interval selection - /// ------------------- - /// The observation arc is defined by: - /// * `extf` – fractional extension factor applied around the triplet center, - /// * `dtmax` – absolute maximum time span (days) allowed for the arc. - /// - /// The effective interval is determined by - /// [`select_rms_interval`](Self::select_rms_interval), which returns the first - /// and last indices of the observations to include. - /// - /// Computation - /// ------------ - /// * Each observation contributes a squared normalized residual - /// from [`Observation::ephemeris_error`](crate::observations::Observation::ephemeris_error). - /// * The final RMS is - /// - /// ```text - /// RMS = √[ (1 / (2N)) · Σᵢ (ΔRAᵢ² + ΔDECᵢ²) ] - /// ``` - /// - /// where `N` is the number of observations in the selected interval. - /// - /// Pruning mode - /// ------------ - /// If `prune_if_rms_ge` is set: - /// * The summation stops early once the partial RMS reaches the threshold, - /// returning the pruning value directly. - /// * If `prune_if_rms_ge = ∞`, no early exit occurs (equivalent to no pruning). - /// - /// Arguments - /// ---------- - /// * `state` – Global context providing ephemerides, Earth orientation, and time conversion. - /// * `triplets` – The Gauss triplet that defined the preliminary orbit. - /// * `orbit_element` – The orbit (in equinoctial elements) to be tested against the arc. - /// * `extf` – Fractional time extension of the interval around the triplet. - /// * `dtmax` – Maximum arc duration (days). - /// * `prune_if_rms_ge` – Optional RMS cutoff for early termination (see *Pruning mode*). - /// - /// Return - /// ------- - /// * `Ok(rms)` – RMS of the normalized astrometric residuals (radians). - /// * `Err(OutfitError)` – If interval selection fails or propagation/ephemeris lookup fails. - /// - /// Units - /// ------- - /// * The returned RMS is dimensionless but expressed in **radians**. - fn rms_orbit_error( - &self, - state: &Outfit, - triplets: &GaussObs, - orbit_element: &EquinoctialElements, - extf: f64, - dtmax: f64, - prune_if_rms_ge: Option, - ) -> Result; - - /// Apply RMS correction based on temporally clustered batches of observations. - /// - /// This method adjusts the astrometric uncertainties (`error_ra`, `error_dec`) of each observation - /// based on the local density of observations in time and observer identity. Observations that are - /// close in time (within 8 hours) and come from the same observer are grouped into batches, and a - /// correction factor is applied to reflect statistical correlation or improvement due to redundancy. - /// - /// # Arguments - /// --------------- - /// * `error_model` - The error model to use when applying the batch correction. Supported values include: - /// - `"vfcc17"`: uses a reduced factor `√(n × 0.25)` if the batch has at least 5 observations, - /// - any other string: uses the standard `√n` factor. - /// * `gap_max` - The maximum time gap (in days) to consider observations as part of the same batch. - /// - /// # Behavior - /// ---------- - /// - Observations are grouped by `observer` and sorted in time. - /// - A batch is formed when consecutive observations from the same observer are spaced by less than 8 hours. - /// - Each observation in a batch of size `n` receives a correction: - /// - `√n` for standard models, - /// - `√(n × 0.25)` for `vfcc17` when `n ≥ 5`. - /// - If `n < 5` with `vfcc17`, it falls back to `√n`. - /// - Observations with fixed weights (`force_w`) are not affected (not yet implemented in this version). - /// - /// # Returns - /// ---------- - /// * `()` - This function modifies the observations in-place; it does not return a value. - /// - /// # Computation Details - /// ---------- - /// - The time comparison is based on Modified Julian Date (`MJD`), and the batch window is fixed at 8 hours (i.e., `8.0 / 24.0` days). - /// - The error fields `error_ra` and `error_dec` are both scaled by the same batch correction factor. - /// - /// # Units - /// ---------- - /// - Input and output uncertainties (`error_ra`, `error_dec`) are expressed in **radians**. - fn apply_batch_rms_correction(&mut self, error_model: &ErrorModel, gap_max: f64); - - /// Extract astrometric uncertainties (RA and DEC) for a set of three observations. - /// - /// Given a triplet of observation indices, this function retrieves the corresponding - /// astrometric errors in right ascension and declination from the observation set. - /// - /// # Arguments - /// --------------- - /// * `idx_obs` - A vector of three indices referring to the observations used in the triplet. - /// - /// # Returns - /// --------------- - /// * A tuple of two `Vector3`: - /// - The first vector contains the RA uncertainties in radians. - /// - The second vector contains the DEC uncertainties in radians. - /// - /// # Panics - /// --------------- - /// This function will panic if any index in `idx_obs` is out of bounds of the observation set. - fn extract_errors(&self, idx_obs: Vector3) -> (Vector3, Vector3); -} - -/// Trait for performing Initial Orbit Determination (IOD) on a set of astrometric observations. -/// -/// This trait encapsulates high-level algorithms to derive a **preliminary orbit** -/// from a time series of astrometric observations, using the **Gauss method**. -/// It focuses on searching for the best-fitting orbit over all valid triplets of observations. -/// -/// ## Purpose -/// -/// The main goal of this trait is to automate the process of: -/// 1. Building candidate triplets of observations (see [`compute_triplets`](ObservationsExt::compute_triplets)), -/// 2. Estimating a preliminary orbit for each triplet using the Gauss method, -/// 3. Perturbing triplets with Gaussian noise to simulate observational uncertainties, -/// 4. Selecting the orbit that minimizes the root-mean-square (RMS) of astrometric residuals -/// when compared to the entire set of observations. -/// -/// This process is the standard entry point for orbit determination workflows. -/// It is designed for **short observational arcs**, such as those of newly discovered asteroids. -/// -/// ## Typical usage -/// -/// ```rust, no_run -/// use rand::{rngs::StdRng, SeedableRng}; -/// use outfit::initial_orbit_determination::IODParams; -/// use outfit::constants::Observations; -/// use outfit::observations::observations_ext::ObservationIOD; -/// -/// let params = IODParams::builder() -/// .n_noise_realizations(100) -/// .noise_scale(1.0) -/// .dtmax(30.0) -/// .max_triplets(50) -/// .build().unwrap(); -/// -/// let observations: Observations = unimplemented!(); // Your observations here -/// let state = unimplemented!(); // Your state here -/// let error_model = unimplemented!(); // Your error model here -/// let mut rng = StdRng::seed_from_u64(42); -/// -/// let (best_orbit, rms) = observations.estimate_best_orbit( -/// &state, &error_model, &mut rng, ¶ms).unwrap(); -/// println!("Best preliminary orbit RMS = {rms}"); -/// ``` -/// -/// ## Algorithmic steps -/// -/// 1. **Batch uncertainty correction:** -/// Observations are first passed through [`ObservationsExt::apply_batch_rms_correction`]. -/// -/// 2. **Triplet generation:** -/// Valid combinations of three observations are extracted with [`ObservationsExt::compute_triplets`], -/// using the configuration parameters from [`IODParams`] (e.g., `dt_min`, `dt_max_triplet`, -/// `optimal_interval_time`, `max_obs_for_triplets`, `max_triplets`). -/// -/// 3. **Orbit estimation:** -/// For each triplet, `n_noise_realizations` noisy variants are generated (Monte Carlo) -/// and processed by the Gauss method to obtain preliminary orbital elements. -/// -/// 4. **Orbit evaluation:** -/// Each preliminary orbit is propagated and compared to the full observation arc using -/// [`ObservationsExt::rms_orbit_error`]. The orbit with the smallest RMS is returned. -/// -/// ## Performance considerations -/// -/// * Typically applied to **short arcs with tens of observations**. -/// * The number of triplets can be limited via `params.max_triplets`. -/// * The Monte Carlo loop (`params.n_noise_realizations`) dominates runtime. -/// -/// ## Returns -/// -/// * `Ok((Some(best_orbit), best_rms))` – if a valid orbit was found, -/// * `Ok((None, f64::MAX))` – if no valid orbit could be estimated, -/// * `Err(OutfitError)` – if an error occurs during propagation or fitting. -/// -/// ## Parameters -/// -/// * [`IODParams`] – Controls the noise sampling, temporal constraints on triplets, -/// and the maximum number of triplets to evaluate. -/// -/// ## See also -/// -/// * [`ObservationsExt::compute_triplets`] – Generates candidate triplets from the observation set. -/// * [`ObservationsExt::rms_orbit_error`] – Evaluates the quality of an orbit over the full arc. -/// * [`GaussResult`] – Data structure holding the result of a single Gauss method run. -/// * [`KeplerianElements`](crate::orbit_type::keplerian_element::KeplerianElements) – Orbital elements returned by successful preliminary orbit estimation. -/// * [`IODParams`] – Groups all configuration options for IOD. -pub trait ObservationIOD { - /// Estimate the best-fitting preliminary orbit from a full set of astrometric observations. - /// - /// This method searches for the best preliminary orbit by evaluating a limited number of - /// observation triplets generated from the dataset. The process includes: - /// - /// 1. **Error calibration**: - /// Observations are first preprocessed with [`ObservationsExt::apply_batch_rms_correction`] to account for - /// temporal clustering and observer-specific error models. - /// - /// 2. **Triplet generation**: - /// Candidate triplets are generated using [`ObservationsExt::compute_triplets`], which: - /// * Sorts observations by time, - /// * Optionally downsamples the dataset to at most `params.max_obs_for_triplets` points - /// (uniform in time, always keeping the first and last), - /// * Filters valid triplets according to `params.dt_min`, `params.dt_max_triplet`, - /// and `params.optimal_interval_time`. - /// - /// 3. **Monte Carlo noise sampling**: - /// For each triplet, `params.n_noise_realizations` perturbed versions are created using - /// Gaussian noise scaled by `params.noise_scale` times the nominal astrometric uncertainties. - /// - /// 4. **Orbit estimation and selection**: - /// For each (possibly perturbed) triplet, a preliminary orbit is computed with the Gauss method. - /// The resulting orbit is evaluated over the full set of observations using [`ObservationsExt::rms_orbit_error`]. - /// The orbit with the smallest RMS is returned. - /// - /// # Arguments - /// - /// * `state` – - /// Global [`Outfit`] state, providing ephemerides and time conversions. - /// * `error_model` – - /// The astrometric error model (typically per-band or per-observatory). - /// * `rng` – - /// A random number generator used to draw Gaussian perturbations. - /// * `params` – - /// Parameters controlling the initial orbit determination, including: - /// * `n_noise_realizations`: number of noisy triplet variants generated per original triplet, - /// * `noise_scale`: scaling factor for the noise, - /// * `extf`: extrapolation factor for RMS evaluation, - /// * `dtmax`: maximum time interval for RMS evaluation, - /// * `dt_min`, `dt_max_triplet`, `optimal_interval_time`: constraints on triplet spans, - /// * `max_obs_for_triplets`: maximum number of observations to keep when building triplets, - /// * `max_triplets`: maximum number of triplets to process, - /// * `gap_max`: maximum allowed time gap within a batch for RMS corrections. - /// - /// # Returns - /// - /// * `Ok((Some(best_orbit), best_rms))` – The best preliminary orbit found and its RMS. - /// * `Ok((None, f64::MAX))` – No valid orbit could be estimated. - /// * `Err(e)` – An error occurred during orbit estimation or RMS evaluation. - /// - /// # Notes - /// - /// - RMS values are computed with [`ObservationsExt::rms_orbit_error`], which accounts for - /// light-time correction and ephemeris propagation. - /// - Each triplet can produce several preliminary orbit candidates due to - /// noise realizations. - /// - The `max_obs_for_triplets` parameter is crucial for large datasets, - /// as it avoids the combinatorial explosion of triplets. - /// - /// # See also - /// - /// * [`ObservationsExt::compute_triplets`] – Selects triplets from the observation set. - /// * [`GaussObs::generate_noisy_realizations`] – Creates perturbed triplets with Gaussian noise. - /// * [`GaussObs::prelim_orbit`] – Computes a preliminary orbit from a single triplet. - /// * [`ObservationsExt::rms_orbit_error`] – Measures the goodness-of-fit of an orbit against observations. - /// * [`IODParams`] – Configuration options for the IOD process. - fn estimate_best_orbit( - &mut self, - state: &Outfit, - error_model: &ErrorModel, - rng: &mut impl rand::Rng, - params: &IODParams, - ) -> Result<(GaussResult, f64), OutfitError>; -} - -impl ObservationsExt for Observations { - fn compute_triplets( - &mut self, - dt_min: f64, - dt_max: f64, - optimal_interval_time: f64, - max_obs_for_triplets: usize, - max_triplet: u32, - ) -> Vec { - generate_triplets( - self, - dt_min, - dt_max, - optimal_interval_time, - max_obs_for_triplets, - max_triplet, - ) - } - - fn select_rms_interval( - &self, - triplets: &GaussObs, - extf: f64, - dtmax: f64, - ) -> Result<(usize, usize), OutfitError> { - let nobs = self.len(); - - let idx_obs1 = triplets.idx_obs[0]; - let obs1 = self - .get(idx_obs1) - .ok_or(OutfitError::ObservationNotFound(idx_obs1))?; - - let idx_obs3 = triplets.idx_obs[2]; - let obs3 = self - .get(idx_obs3) - .ok_or(OutfitError::ObservationNotFound(idx_obs3))?; - - let first_obs = self.first().ok_or(OutfitError::ObservationNotFound(0))?; - let last_obs = self - .last() - .ok_or(OutfitError::ObservationNotFound(nobs - 1))?; - // Step 1: Compute the maximum allowed interval - let mut dt = if extf >= 0.0 { - (obs3.time - obs1.time) * extf - } else { - 10.0 * (last_obs.time - first_obs.time) - }; - - if dtmax >= 0.0 { - dt = dt.max(dtmax); - } - - let mut i_start = 0; - - for i in (0..=idx_obs1).rev() { - if let Some(obs_i) = self.get(i) { - if obs1.time - obs_i.time > dt { - break; - } - i_start = i; - } - } - - let mut i_end = nobs - 1; - - for i in idx_obs3..nobs { - if let Some(obs_i) = self.get(i) { - if obs_i.time - obs3.time > dt { - break; - } - i_end = i; - } - } - - Ok((i_start, i_end)) - } - - fn rms_orbit_error( - &self, - state: &Outfit, - triplets: &GaussObs, - orbit_element: &EquinoctialElements, - extf: f64, - dtmax: f64, - prune_if_rms_ge: Option, - ) -> Result { - // Select the time interval [start_obs_rms, end_obs_rms] over which the RMS - // error is evaluated. The interval depends on the triplet and on external - // filtering parameters (extf, dtmax). - let (start_obs_rms, end_obs_rms) = self.select_rms_interval(triplets, extf, dtmax)?; - - // Number of observations contributing to the RMS - let n_obs = (end_obs_rms - start_obs_rms + 1) as f64; - - // Denominator of the RMS formula: here weighted by 2.0 for consistency - // with the convention used elsewhere in the code. - let denom = 2.0 * n_obs; - - // ========================================================================= - // Case 1: No pruning → behave like the "classical" RMS definition - // ========================================================================= - if prune_if_rms_ge.is_none() { - // Accumulate the squared ephemeris errors for each observation - let sum = self[start_obs_rms..=end_obs_rms] - .iter() - .map(|obs| obs.ephemeris_error(state, orbit_element)) - // try_fold propagates errors from ephemeris_error while summing - .try_fold(0.0, |acc, term| term.map(|v| acc + v))?; - - // Final RMS = sqrt( sum / denom ) - return Ok((sum / denom).sqrt()); - } - - // ========================================================================= - // Case 2: Pruning enabled → early stop if RMS exceeds a threshold - // ========================================================================= - let prune = prune_if_rms_ge.unwrap(); - - // Convert the RMS cutoff into a sum cutoff: - // RMS² = sum / denom → stop if sum ≥ (prune² * denom). - let sum_cutoff = if prune.is_finite() { - prune * prune * denom - } else { - f64::INFINITY // "no real cutoff" if prune = ∞ - }; - - // Iterate over observations and accumulate squared errors. - // We use ControlFlow to allow early exit: - // - Continue(sum): keep summing, - // - Break(value): stop early and return the pruning threshold. - let folded: ControlFlow = self[start_obs_rms..=end_obs_rms] - .iter() - .map(|obs| obs.ephemeris_error(state, orbit_element)) - .try_fold(0.0, |acc, term| match term { - Ok(v) => { - let new_sum = acc + v; - if new_sum >= sum_cutoff { - // Early exit: threshold reached, return directly - ControlFlow::Break(prune) - } else { - ControlFlow::Continue(new_sum) - } - } - // In case of error in ephemeris_error, also exit with pruning value. - Err(_) => ControlFlow::Break(prune), - }); - - // Final RMS depending on whether we exited early or not - match folded { - ControlFlow::Continue(sum) => Ok((sum / denom).sqrt()), - ControlFlow::Break(rms) => Ok(rms), - } - } - - fn apply_batch_rms_correction(&mut self, error_model: &ErrorModel, gap_max: f64) { - // Step 1: Sort in time - self.sort_by(|a, b| a.time.partial_cmp(&b.time).unwrap()); - - // Step 2: Group by observer - for (_observer_id, group) in &self.into_iter().chunk_by(|obs| obs.observer) { - // Step 3: Batch grouping using sliding window - let mut batch: VecDeque<&mut Observation> = VecDeque::new(); - let mut iter = group.peekable(); - - while let Some(obs) = iter.next() { - batch.push_back(obs); - - // Extend batch while within gap_max - while let Some(next) = iter.peek() { - let dt = next.time - - batch - .back() - .expect("in apply_batch_rms_correction: batch should not be empty") - .time; - if dt <= gap_max { - batch.push_back(iter.next().expect( - "in apply_batch_rms_correction: next in batch should not be None", - )); - } else { - break; - } - } - - // Apply correction to current batch - let n = batch.len(); - if n > 0 { - let factor = match error_model { - ErrorModel::VFCC17 if n >= 5 => (n as f64 * 0.25).sqrt(), - _ => (n as f64).sqrt(), - }; - - for obs in batch.drain(..) { - obs.error_ra *= factor; - obs.error_dec *= factor; - } - } - } - } - } - - fn extract_errors(&self, idx_obs: Vector3) -> (Vector3, Vector3) { - let (errors_ra, errors_dec): (Vec<_>, Vec<_>) = idx_obs - .into_iter() - .map(|i| { - let obs = &self[*i]; - (obs.error_ra, obs.error_dec) - }) - .unzip(); - - ( - Vector3::from_column_slice(&errors_ra), - Vector3::from_column_slice(&errors_dec), - ) - } -} - -impl ObservationIOD for Observations { - fn estimate_best_orbit( - &mut self, - state: &Outfit, - error_model: &ErrorModel, - rng: &mut impl rand::Rng, - params: &IODParams, - ) -> Result<(GaussResult, f64), OutfitError> { - // --- Stage 1: Calibrate uncertainties once for the whole batch. - // This aligns quoted per-obs errors with empirical RMS statistics. - self.apply_batch_rms_correction(error_model, params.gap_max); - - // --- Stage 2: Enumerate candidate triplets under temporal constraints. - let triplets = self.compute_triplets( - params.dt_min, - params.dt_max_triplet, - params.optimal_interval_time, - params.max_obs_for_triplets, - params.max_triplets, - ); - - if triplets.is_empty() { - let span = if self.is_empty() { - 0.0 - } else { - self.last().unwrap().time - self.first().unwrap().time - }; - return Err(OutfitError::NoFeasibleTriplets { - span, - n_obs: self.len(), - dt_min: params.dt_min, - dt_max: params.dt_max_triplet, - }); - } - - // Current best (lowest) RMS and its orbit. - // Using +∞ avoids Option branching in the hot path. - let mut best_rms = f64::INFINITY; - let mut best_orbit: Option = None; - - // Keep the last encountered error so that we can report something meaningful if *all* fail. - // We don't clone: we keep only the most recent error by moving it in. - let mut last_error: Option = None; - - // For diagnostics, count how many realizations we actually attempted. - let mut n_attempts: usize = 0; - - // --- Stage 3: Explore each triplet. - for triplet in triplets { - // Extract 1-σ astrometric uncertainties for the three obs of this triplet. - let (error_ra, error_dec) = self.extract_errors(triplet.idx_obs); - - // --- Stage 4: For each (lazy) noisy realization of this triplet... - // The iterator yields the original triplet first, then noisy copies. - for realization in triplet.realizations_iter( - &error_ra, - &error_dec, - params.n_noise_realizations, - params.noise_scale, - rng, - ) { - n_attempts += 1; - - // 4.a) Preliminary Gauss solution on the current realization. - let gauss_res = match realization.prelim_orbit(state, params) { - Ok(res) => res, - Err(e) => { - // Record the failure and continue exploring. - last_error = Some(e); - continue; - } - }; - - // 4.b) Convert to the element set required by the scorer. - let equinoctial_elements = gauss_res.get_orbit().to_equinoctial()?; - - // 4.c) Score orbit vs. full observation set (RMS residual). - let rms = match self.rms_orbit_error( - state, - &realization, - &equinoctial_elements, - params.extf, - params.dtmax, - Some(best_rms), - ) { - Ok(v) => { - if !v.is_finite() { - last_error = Some(OutfitError::NonFiniteScore(v)); - continue; - } else { - v - } - } - Err(e) => { - last_error = Some(e); - continue; - } - }; - - // 4.d) Keep the best candidate so far. - if rms < best_rms { - best_rms = rms; - best_orbit = Some(gauss_res); - } - } - } - - // --- Stage 5: If at least one candidate succeeded, return the best; otherwise, propagate an error. - if let Some(orbit) = best_orbit { - Ok((orbit, best_rms)) - } else { - // If nothing succeeded, propagate a structured error with the last underlying cause. - // Fallback to a domain-specific unit error if we never captured any (e.g., no attempts). - let root_cause = match last_error { - Some(e) => e, - None => panic!("In estimate_best_orbit: no error captured but best_orbit is None, this should not happen"), - }; - Err(OutfitError::NoViableOrbit { - cause: Box::new(root_cause), - attempts: n_attempts, - }) - } - } -} - -#[cfg(test)] -mod test_obs_ext { - - use crate::error_models::ErrorModel; - - use super::*; - - #[test] - #[cfg(feature = "jpl-download")] - fn test_select_rms_interval() { - use crate::unit_test_global::OUTFIT_HORIZON_TEST; - - let mut traj_set = OUTFIT_HORIZON_TEST.1.clone(); - - let traj_number = crate::constants::ObjectNumber::String("K09R05F".into()); - let traj_len = traj_set - .get(&traj_number) - .expect("Failed to get trajectory") - .len(); - - let traj = traj_set - .get_mut(&traj_number) - .expect("Failed to get trajectory"); - - let triplets = traj.compute_triplets(0.03, 150.0, 20.0, traj_len, 10); - let (u1, u2) = traj - .select_rms_interval(triplets.first().unwrap(), -1., 30.) - .unwrap(); - - assert_eq!(u1, 0); - assert_eq!(u2, 36); - - let (u1, u2) = traj - .select_rms_interval(triplets.first().unwrap(), 10., 30.) - .unwrap(); - - assert_eq!(u1, 14); - assert_eq!(u2, 36); - - let (u1, u2) = traj - .select_rms_interval(triplets.first().unwrap(), 0.001, 3.) - .unwrap(); - - assert_eq!(u1, 17); - assert_eq!(u2, 33); - } - - #[test] - #[cfg(feature = "jpl-download")] - fn test_rms_trajectory() { - use nalgebra::Matrix3; - - use crate::{ - orbit_type::keplerian_element::KeplerianElements, unit_test_global::OUTFIT_HORIZON_TEST, - }; - - let mut traj_set = OUTFIT_HORIZON_TEST.1.clone(); - - let traj = traj_set - .get_mut(&crate::constants::ObjectNumber::String("K09R05F".into())) - .expect("Failed to get trajectory"); - - traj.apply_batch_rms_correction(&ErrorModel::FCCT14, 8.0 / 24.0); - - let triplets = GaussObs { - idx_obs: Vector3::new(34, 35, 36), - ra: [[ - 1.789_797_623_341_267, - 1.789_865_909_348_251, - 1.7899347771316527, - ]] - .into(), - dec: [[ - 0.779_178_052_350_181, - 0.779_086_664_971_291_9, - 0.778_996_538_107_973_6, - ]] - .into(), - time: [[ - 57070.238017592594, - 57_070.250_007_592_59, - 57070.262067592594, - ]] - .into(), - observer_helio_position: Matrix3::zeros(), - }; - - let kepler = KeplerianElements { - reference_epoch: 57_049.242_334_573_75, - semi_major_axis: 1.8017360713154256, - eccentricity: 0.283_559_145_668_705_7, - inclination: 0.20267383288689386, - ascending_node_longitude: 7.955_979_023_693_781E-3, - periapsis_argument: 1.2451951387589135, - mean_anomaly: 0.44054589015887125, - }; - - let rms = traj - .rms_orbit_error( - &OUTFIT_HORIZON_TEST.0, - &triplets, - &kepler.into(), - -1.0, - 30., - None, - ) - .unwrap(); - - assert_eq!(rms, 68.88650730830162); - } - - mod test_batch_rms_correction { - use crate::constants::MJD; - use approx::assert_ulps_eq; - use smallvec::smallvec; - - use super::*; - - fn obs(observer: u16, time: MJD) -> Observation { - Observation { - observer, - ra: 1.0, - error_ra: 1e-6, - dec: 0.5, - error_dec: 2e-6, - time, - observer_earth_position: Vector3::zeros(), - observer_helio_position: Vector3::zeros(), - } - } - - #[test] - fn test_single_batch_vfcc17_large() { - let base_time = 59000.0; - let mut obs: Observations = smallvec![ - obs(1, base_time), - obs(1, base_time + 0.01), - obs(1, base_time + 0.02), - obs(1, base_time + 0.03), - obs(1, base_time + 0.04), // n = 5 - ]; - - obs.apply_batch_rms_correction(&ErrorModel::VFCC17, 8.0 / 24.0); - - let factor = (5.0_f64 * 0.25_f64).sqrt(); - for ob in &obs { - assert_ulps_eq!(ob.error_ra, 1e-6 * factor, max_ulps = 2); - assert_ulps_eq!(ob.error_dec, 2e-6 * factor, max_ulps = 2); - } - } - - #[test] - fn test_single_batch_small_n() { - let base_time = 59000.0; - let mut obs: Observations = smallvec![ - obs(2, base_time), - obs(2, base_time + 0.01), // n = 2 - ]; - - obs.apply_batch_rms_correction(&ErrorModel::FCCT14, 8.0 / 24.0); - - let factor = (2.0f64).sqrt(); - for ob in &obs { - assert_ulps_eq!(ob.error_ra, 1e-6 * factor, max_ulps = 2); - assert_ulps_eq!(ob.error_dec, 2e-6 * factor, max_ulps = 2); - } - } - - #[test] - fn test_multiple_batches_same_observer() { - let base_time = 59000.0; - let mut obs: Observations = smallvec![ - obs(3, base_time), - obs(3, base_time + 0.01), // batch 1 (n = 2) - obs(3, base_time + 1.0), // isolated, batch 2 (n = 1) - ]; - - obs.apply_batch_rms_correction(&ErrorModel::FCCT14, 8.0 / 24.0); - - let factor1 = (2.0f64).sqrt(); - let factor2 = 1.0; - - assert_ulps_eq!(obs[0].error_ra, 1e-6 * factor1, max_ulps = 2); - assert_ulps_eq!(obs[1].error_ra, 1e-6 * factor1, max_ulps = 2); - assert_ulps_eq!(obs[2].error_ra, 1e-6 * factor2, max_ulps = 2); - } - - #[test] - fn test_different_observers_are_not_grouped() { - let base_time = 59000.0; - let mut obs: Observations = smallvec![ - obs(10, base_time), - obs(11, base_time + 0.01), - obs(12, base_time + 0.02), - ]; - - obs.apply_batch_rms_correction(&ErrorModel::FCCT14, 8.0 / 24.0); - - for ob in &obs { - assert_ulps_eq!(ob.error_ra, 1e-6, max_ulps = 2); - assert_ulps_eq!(ob.error_dec, 2e-6, max_ulps = 2); - } - } - - #[test] - fn test_batch_gaps_exceed_gapmax() { - let mut obs: Observations = smallvec![ - obs(5, 59000.0), - obs(5, 59001.0), // > 8h => separate - ]; - - obs.apply_batch_rms_correction(&ErrorModel::FCCT14, 8.0 / 24.0); - - for ob in &obs { - assert_ulps_eq!(ob.error_ra, 1e-6, max_ulps = 2); - assert_ulps_eq!(ob.error_dec, 2e-6, max_ulps = 2); - } - } - - #[test] - #[cfg(feature = "jpl-download")] - fn test_batch_real_data() { - use crate::unit_test_global::OUTFIT_HORIZON_TEST; - - let mut traj_set = OUTFIT_HORIZON_TEST.1.clone(); - - let traj = traj_set - .get_mut(&crate::constants::ObjectNumber::String("K09R05F".into())) - .expect("Failed to get trajectory"); - - traj.apply_batch_rms_correction(&ErrorModel::FCCT14, 8.0 / 24.0); - - assert_ulps_eq!(traj[0].error_ra, 2.507075226057322e-6, max_ulps = 2); - assert_ulps_eq!(traj[0].error_dec, 2.036217397086327e-6, max_ulps = 2); - - assert_ulps_eq!(traj[1].error_ra, 2.5070681687218917e-6, max_ulps = 2); - assert_ulps_eq!(traj[1].error_dec, 2.036217397086327e-6, max_ulps = 2); - - assert_ulps_eq!(traj[2].error_ra, 2.507_059_507_890_695_2E-6, max_ulps = 2); - assert_ulps_eq!(traj[2].error_dec, 2.036217397086327e-6, max_ulps = 2); - } - } - - mod test_extract_errors { - use super::*; - use approx::assert_ulps_eq; - use smallvec::smallvec; - - fn make_observations() -> Observations { - smallvec![ - Observation { - observer: 0, - ra: 1.0, - dec: 0.5, - error_ra: 1e-6, - error_dec: 2e-6, - time: 59000.0, - observer_earth_position: Vector3::zeros(), - observer_helio_position: Vector3::zeros(), - }, - Observation { - observer: 0, - ra: 1.1, - dec: 0.6, - error_ra: 3e-6, - error_dec: 4e-6, - time: 59000.1, - observer_earth_position: Vector3::zeros(), - observer_helio_position: Vector3::zeros(), - }, - Observation { - observer: 0, - ra: 1.2, - dec: 0.7, - error_ra: 5e-6, - error_dec: 6e-6, - time: 59000.2, - observer_earth_position: Vector3::zeros(), - observer_helio_position: Vector3::zeros(), - }, - ] - } - - #[test] - fn test_extract_errors_basic() { - let obs = make_observations(); - let idx_obs = Vector3::new(0, 1, 2); - - let (ra_errors, dec_errors) = obs.extract_errors(idx_obs); - - assert_ulps_eq!(ra_errors[0], 1e-6, max_ulps = 2); - assert_ulps_eq!(ra_errors[1], 3e-6, max_ulps = 2); - assert_ulps_eq!(ra_errors[2], 5e-6, max_ulps = 2); - - assert_ulps_eq!(dec_errors[0], 2e-6, max_ulps = 2); - assert_ulps_eq!(dec_errors[1], 4e-6, max_ulps = 2); - assert_ulps_eq!(dec_errors[2], 6e-6, max_ulps = 2); - } - - #[test] - #[should_panic(expected = "index out of bounds")] - fn test_extract_errors_out_of_bounds() { - let obs = make_observations(); - let idx_obs = Vector3::new(0, 1, 10); // 10 is out of bounds - let _ = obs.extract_errors(idx_obs); - } - } - - #[test] - #[cfg(feature = "jpl-download")] - fn test_estimate_best_orbit() { - use approx::assert_relative_eq; - use rand::{rngs::StdRng, SeedableRng}; - - use crate::{ - orbit_type::{ - keplerian_element::KeplerianElements, orbit_type_test::approx_equal, - OrbitalElements, - }, - unit_test_global::OUTFIT_HORIZON_TEST, - }; - - let mut traj_set = OUTFIT_HORIZON_TEST.1.clone(); - - let traj_number = crate::constants::ObjectNumber::String("K09R05F".into()); - let traj_len = traj_set - .get(&traj_number) - .expect("Failed to get trajectory") - .len(); - - let traj = traj_set - .get_mut(&traj_number) - .expect("Failed to get trajectory"); - - let mut rng = StdRng::seed_from_u64(42_u64); // seed for reproducibility - - let gap_max = 8.0 / 24.0; // 8 hours in days - - let params = IODParams { - n_noise_realizations: 5, - max_obs_for_triplets: traj_len, - gap_max, - ..Default::default() - }; - - let (best_orbit, best_rms) = traj - .estimate_best_orbit( - &OUTFIT_HORIZON_TEST.0, - &ErrorModel::FCCT14, - &mut rng, - ¶ms, - ) - .unwrap(); - - let binding = best_orbit; - let orbit = binding.get_orbit(); - - let expected_orbit = OrbitalElements::Keplerian(KeplerianElements { - reference_epoch: 57049.22904488294, - semi_major_axis: 1.801748431600605, - eccentricity: 0.283572284127787, - inclination: 0.20266779609836036, - ascending_node_longitude: 0.008022659889281067, - periapsis_argument: 1.245060173584828, - mean_anomaly: 0.44047943792316746, - }); - - assert!(approx_equal(orbit, &expected_orbit, 1e-14)); - assert_relative_eq!(best_rms, 55.14810894219461, epsilon = 1e-14); - } -} diff --git a/src/observations/triplets_generator.rs b/src/observations/triplets_generator.rs deleted file mode 100644 index 3ff4cb9..0000000 --- a/src/observations/triplets_generator.rs +++ /dev/null @@ -1,323 +0,0 @@ -//! # IOD Triplet Index Generator (lazy, windowed by time span) -//! -//! Streams **reduced indices** `(first, middle, last)` of time-feasible IOD triplets, -//! after sorting and downsampling the input observations. This is intended to be the -//! *index-level* counterpart of a Gauss triplet generator, allowing clients to compute -//! their own heuristics (e.g., a spacing weight) before materializing actual `GaussObs`. -//! -//! ## What “reduced indices” means -//! The generator first downsamples the full observation set to a smaller, **time-sorted** -//! subset (the “reduced” view). Indices yielded by the iterator refer to this reduced -//! view; use `selected_original_indices()` to map **reduced → original** indices. -//! -//! ## Feasibility constraints -//! For each yielded triplet `(first, middle, last)` with `first < middle < last`, the -//! following time-span constraint holds: -//! -//! ```text -//! dt_min ≤ t[last] - t[first] ≤ dt_max -//! ``` -//! -//! where `t[*]` are the **reduced** epochs (same units as your observation times, e.g. TT/MJD). -//! -//! ## Why this generator? -//! - **Lazy**: no intermediate `Vec` of triplets; you can start consuming immediately. -//! - **Better complexity**: a per-anchor two-pointer window on `last` reduces the -//! effective cost towards ~`O(n²)` in typical time distributions (vs. `O(n³)` brute force). -//! - **No overlapping borrows**: the generator **owns** its internal buffers (times, -//! mapping), so you can iterate without holding long-lived borrows of the input. -//! -//! ## Typical flow -//! 1. Build with `TripletIndexGenerator::from_observations(...)` (sorts + downsamples). -//! 2. Iterate lazily over `(i, j, k)` **reduced** indices. -//! 3. If needed, map to originals via `gen.selected_original_indices()[i]`. -//! 4. (Optional) Compute a heuristic (e.g., spacing weight) and keep the best-K with a heap. -//! 5. Only then materialize full `GaussObs` from the original observations. -//! -//! ## Invariants per anchor -//! - `first < middle < last` always holds. -//! - For the current `first`, the **feasible window** for `last` is -//! `[last_lower_bound_reduced_idx, last_upper_bound_reduced_idx]` such that -//! `dt_min ≤ t[last] - t[first] ≤ dt_max`. -//! - The initial `middle` is `first + 1` and the initial `last` is -//! `max(last_lower_bound_reduced_idx, middle + 1)`. -//! -//! ## Complexity -//! - Time: typically ~`O(n²)` (one window sweep per anchor). -//! - Space: `O(1)` per yielded triplet (the generator holds only the reduced times and mapping). -//! -//! ## Notes & pitfalls -//! - `dt_min`/`dt_max` must be in the **same time units** as your observation epochs. -//! - If `dt_min > dt_max` or there are fewer than 3 reduced observations, the iterator is empty. -//! - The generator **does not** impose any ordering by a heuristic (e.g., “optimal interval”); -//! it only ensures time-feasibility. Best-first strategies should be layered on top. -//! -//! ## See also -//! - A Gauss triplet generator that yields `GaussObs` and can be combined with Monte-Carlo -//! perturbations (`realizations_iter`). -//! - An IOD search routine (e.g., `estimate_best_orbit`) that consumes indices for early-stop. - -use crate::observations::{triplets_iod::downsample_uniform_with_edges_indices, Observations}; - -/// Stream-only generator of **reduced indices** `(first, middle, last)` -/// for time-feasible IOD triplets. -/// -/// Arguments -/// ----------------- -/// * `dt_min` – Minimum allowed time span between **first** and **last**. -/// * `dt_max` – Maximum allowed time span between **first** and **last**. -/// * `max_triplets_to_yield` – Optional cap on the number of yielded triplets (use `usize::MAX` for no cap). -/// -/// Return -/// ---------- -/// * Implements `Iterator` where the tuple contains -/// **reduced** indices `(first, middle, last)`. -/// -/// See also -/// ------------ -/// * [`selected_original_indices`](TripletIndexGenerator::selected_original_indices) – Map reduced indices back to original ones. -/// * A `GaussObs`-level generator if you need full triplets instead of indices. -pub struct TripletIndexGenerator { - /// Map reduced index → original index (owned). - reduced_to_original_index: Vec, - /// Epochs of the reduced observations (same units as input times; owned). - reduced_epochs_tt_mjd: Vec, - - /// Current **first** (anchor) index in reduced space. - first_reduced_idx: usize, - /// Current **middle** index in reduced space. - middle_reduced_idx: usize, - /// Current **last** index in reduced space. - last_reduced_idx: usize, - - /// Lower bound (inclusive) for `last` given the current `first`. - last_lower_bound_reduced_idx: usize, - /// Upper bound (inclusive) for `last` given the current `first`. - last_upper_bound_reduced_idx: usize, - - /// Number of reduced observations. - reduced_len: usize, - - /// Time-window constraints on `(first, last)`. - dt_min: f64, - dt_max: f64, - - /// Count of triplets yielded so far (monotonic). - yielded_triplets_count: usize, - /// Hard cap on the number of triplets to yield. - max_triplets_to_yield: usize, -} - -impl TripletIndexGenerator { - /// Build a generator from a full observation set: - /// - Sorts by time (in-place), - /// - Downsamples to at most `max_obs_for_triplets`, - /// - Caches reduced epochs and the reduced→original mapping (both **owned**), - /// - Positions on the first feasible window if any. - /// - /// Arguments - /// ----------------- - /// * `observations` – The full set; will be **sorted by time in place**. - /// * `dt_min`, `dt_max` – Time-span constraints on `(first, last)`. - /// * `max_obs_for_triplets` – Downsampling cap (uniform with edges). - /// * `max_triplets_to_yield` – Upper bound on yielded triplets (`usize::MAX` for no cap). - /// - /// Return - /// ---------- - /// * A `TripletIndexGenerator` positioned at the first feasible window, - /// or “empty” if fewer than 3 reduced observations remain. - /// - /// See also - /// ------------ - /// * [`TripletIndexGenerator::selected_original_indices`] - /// * [`TripletIndexGenerator::reduced_times`] - pub fn from_observations( - observations: &mut Observations, - dt_min: f64, - dt_max: f64, - max_obs_for_triplets: usize, - max_triplets_to_yield: usize, - ) -> Self { - // 1) Sort by epoch (ascending) - observations.sort_by(|a, b| a.time.partial_cmp(&b.time).unwrap()); - - // 2) Downsample → keep indices only (no long borrows) - let reduced_to_original_index = - downsample_uniform_with_edges_indices(observations.len(), max_obs_for_triplets); - - // 3) Cache reduced epochs (owned) aligned with reduced indices - let reduced_epochs_tt_mjd: Vec = reduced_to_original_index - .iter() - .map(|&orig| observations[orig].time) - .collect(); - - let reduced_len = reduced_epochs_tt_mjd.len(); - - // Initialize; the precise window is set by `init_last_window_for_first` - let mut gen = Self { - reduced_to_original_index, - reduced_epochs_tt_mjd, - first_reduced_idx: 0, - middle_reduced_idx: 1, - last_reduced_idx: 2, - last_lower_bound_reduced_idx: 2, - last_upper_bound_reduced_idx: 1, // sentinel; will be recomputed - reduced_len, - dt_min, - dt_max, - yielded_triplets_count: 0, - max_triplets_to_yield, - }; - - if gen.reduced_len >= 3 { - gen.init_last_window_for_first(); - } - gen - } - - /// Access the reduced→original index mapping. - /// - /// Return - /// ---------- - /// * A slice of original indices; `selected_original_indices()[r]` maps reduced `r` → original. - /// - /// See also - /// ------------ - /// * [`TripletIndexGenerator::reduced_times`] - pub fn selected_original_indices(&self) -> &[usize] { - &self.reduced_to_original_index - } - - /// Access the reduced epochs (TT/MJD). - /// - /// Return - /// ---------- - /// * A slice of epochs aligned with reduced indices. - pub fn reduced_times(&self) -> &[f64] { - &self.reduced_epochs_tt_mjd - } - - /// Recompute the feasible `last` window `[lower, upper]` for the current `first`. - /// - /// Invariants - /// ----------------- - /// * `lower` is the earliest `last` with `t[last] - t[first] ≥ dt_min`. - /// * `upper` is the latest `last` with `t[last] - t[first] ≤ dt_max`. - /// * `middle = first + 1`. - /// * `last = max(lower, middle + 1)`. - fn init_last_window_for_first(&mut self) { - let first = self.first_reduced_idx; - - // Lower bound (earliest last satisfying the min span; need one middle in (first, last)) - let mut lower = first + 2; - while lower < self.reduced_len - && (self.reduced_epochs_tt_mjd[lower] - self.reduced_epochs_tt_mjd[first]) < self.dt_min - { - lower += 1; - } - - // Upper bound (latest last satisfying the max span) - let mut upper = lower.saturating_sub(1).max(first + 1); - while (upper + 1) < self.reduced_len - && (self.reduced_epochs_tt_mjd[upper + 1] - self.reduced_epochs_tt_mjd[first]) - <= self.dt_max - { - upper += 1; - } - - self.last_lower_bound_reduced_idx = lower; - self.last_upper_bound_reduced_idx = upper; - - self.middle_reduced_idx = first + 1; - self.last_reduced_idx = self - .last_lower_bound_reduced_idx - .max(self.middle_reduced_idx + 1); - } - - /// Move to the next `first` anchor and refresh its feasible `last` window. - /// - /// Return - /// ---------- - /// * `true` if there are still enough reduced observations to form a triplet; `false` otherwise. - fn advance_first_anchor(&mut self) -> bool { - self.first_reduced_idx += 1; - if self.first_reduced_idx + 2 >= self.reduced_len { - return false; - } - self.init_last_window_for_first(); - true - } - - /// Whether the current `(first, middle, last)` window is empty. - /// - /// Return - /// ---------- - /// * `true` if the time-feasible window is empty or invalid; `false` otherwise. - fn last_window_is_empty(&self) -> bool { - self.last_lower_bound_reduced_idx >= self.reduced_len - || self.last_lower_bound_reduced_idx <= self.first_reduced_idx + 1 - || self.last_upper_bound_reduced_idx <= self.first_reduced_idx + 1 - || self.last_lower_bound_reduced_idx > self.last_upper_bound_reduced_idx - } -} - -impl Iterator for TripletIndexGenerator { - type Item = (usize, usize, usize); // reduced indices (first, middle, last) - - fn next(&mut self) -> Option { - // Respect the optional global cap. - if self.yielded_triplets_count >= self.max_triplets_to_yield { - return None; - } - - while self.first_reduced_idx + 2 < self.reduced_len { - // If the current last-window is empty, move to the next anchor. - if self.last_window_is_empty() { - if !self.advance_first_anchor() { - return None; - } - continue; - } - - // If `middle` reached the upper bound, switch to the next `first`. - if self.middle_reduced_idx >= self.last_upper_bound_reduced_idx { - if !self.advance_first_anchor() { - return None; - } - continue; - } - - // Ensure `last` is within the feasible window and respects `middle < last`. - if self.last_reduced_idx < self.last_lower_bound_reduced_idx - || self.last_reduced_idx <= self.middle_reduced_idx - { - self.last_reduced_idx = self - .last_lower_bound_reduced_idx - .max(self.middle_reduced_idx + 1); - } - - // If `last` exceeded the window, advance `middle` and reset `last`. - if self.last_reduced_idx > self.last_upper_bound_reduced_idx { - self.middle_reduced_idx += 1; - self.last_reduced_idx = self - .last_lower_bound_reduced_idx - .max(self.middle_reduced_idx + 1); - continue; - } - - // We have a feasible triplet (first, middle, last). - let i = self.first_reduced_idx; - let j = self.middle_reduced_idx; - let k = self.last_reduced_idx; - - // Prepare the next candidate by advancing `last`. - self.last_reduced_idx += 1; - - self.yielded_triplets_count += 1; - return Some((i, j, k)); - } - - // No more anchors → enumeration complete. - None - } -} diff --git a/src/observer_extension.rs b/src/observer_extension.rs new file mode 100644 index 0000000..ad6329b --- /dev/null +++ b/src/observer_extension.rs @@ -0,0 +1,191 @@ +use hifitime::{ut1::Ut1Provider, Epoch}; +use nalgebra::Vector3; +use ordered_float::NotNan; +use photom::{constants::ERAU, observer::Observer}; + +use crate::{ + cache::{ + observer_centric_cache::{ + ObserverGeocentricPosition, ObserverGeocentricVelocity, ObserverHeliocentricPosition, + }, + observer_fixed_cache::{ObserverFixedCache, ObserverFixedPosition, ObserverFixedVelocity}, + }, + constants::{EARTH_ROTATION, ROT_ECLMJ2000_TO_EQUMJ2000}, + conversion::ToNotNan, + earth_orientation::equequ, + ref_system::{rotmt, rotpn, RefEpoch, RefSystem}, + time::gmst, + JPLEphem, OutfitError, +}; + +pub(crate) trait ResolvedObserver { + /// Get the fixed position of an observatory using its geographic coordinates + /// + /// Return + /// ------ + /// * observer fixed coordinates vector on the Earth (not corrected from Earth motion) + /// * units is AU + fn earth_fixed_position(&self) -> Result; + + /// Get the fixed velocity of an observatory due to Earth rotation, using its geographic coordinates + /// + /// Return + /// ------ + /// * observer fixed velocity vector due to Earth rotation, in the Earth-fixed frame (not corrected from Earth motion) + /// * units is AU/day + fn earth_fixed_velocity(&self) -> Result; + + /// Compute the observer’s geocentric position and velocity in the ecliptic J2000 frame. + /// + /// This function calculates the position and velocity of a ground-based observer relative to the Earth's + /// center of mass, accounting for Earth rotation (via GMST), nutation, and the observer’s geographic location. + /// The result is expressed in the ecliptic mean J2000 frame, suitable for use in orbital initial determination. + /// + /// Arguments + /// --------- + /// * `observer`: a reference to an [`Observer`] containing the site longitude and parallax parameters. + /// * `tmjd`: observation epoch as a [`hifitime::Epoch`] in TT. + /// * `ut1_provider`: a reference to a [`hifitime::ut1::Ut1Provider`] for accurate UT1 conversion. + /// + /// Returns + /// -------- + /// * `(dx, dv)` – Tuple of: + /// - `dx`: observer geocentric position vector in ecliptic mean J2000 frame \[AU\]. + /// - `dv`: observer velocity vector due to Earth's rotation, in the same frame \[AU/day\]. + /// + /// Remarks + /// ------- + /// * Internally, this function: + /// 1. get the body-fixed coordinates of the observer. + /// 2. get its rotational velocity: `v = ω × r`. + /// 3. Applies Earth orientation corrections using: + /// - Greenwich Mean Sidereal Time (GMST), + /// - Equation of the equinoxes, + /// - Precession and nutation transformation (`rotpn`). + /// 4. Returns position and velocity in the J2000 ecliptic frame (used in classical orbital mechanics). + /// + /// # See also + /// * [`Observer::body_fixed_coord`] – observer's base vector in Earth-fixed frame + /// * [`rotpn`] – rotation between reference frames + /// * [`gmst`], [`equequ`] – time-dependent Earth orientation + fn pvobs( + tmjd: &Epoch, + ut1_provider: &Ut1Provider, + observer_fixed_vectors: &ObserverFixedCache, + ) -> Result<(ObserverGeocentricPosition, ObserverGeocentricVelocity), OutfitError>; + + /// Compute the observer’s heliocentric position in the **equatorial mean J2000** frame. + /// + /// This method forms the full heliocentric position of the observing site by combining: + /// - the site **geocentric** position vector at `epoch`, and + /// - the Earth’s **heliocentric** position from the JPL ephemerides. + /// + /// The input geocentric vector is assumed to be expressed in the **ecliptic mean J2000** frame + /// (AU). It is rotated to **equatorial mean J2000**, then added to Earth’s heliocentric + /// position (also in equatorial mean J2000). + /// + /// Arguments + /// ----------------- + /// * `jpl` – [`JPLEphem`] providing Earth's heliocentric state. + /// * `epoch` – Observation epoch in the **TT** time scale. + /// * `observer_geocentric_position` – Geocentric site position **in ecliptic mean J2000** (AU). + /// + /// Return + /// ---------- + /// * `Result` – Observer’s **heliocentric** position at `epoch`, + /// in **AU**, expressed in **equatorial mean J2000**. + /// + /// Remarks + /// ------------- + /// * If your geocentric site vector is already in **equatorial** J2000, rotate it to + /// **ecliptic** before calling this method, or adapt the rotation accordingly. + /// * This routine is typically used internally when constructing per-observation geometry + /// (e.g., within `Observation::new`), ensuring consistent frames for Gauss IOD. + /// + /// See also + /// ------------ + /// * [`Observer::pvobs`] – Geocentric position (and velocity) of the site at `epoch`. + /// * [`Outfit::get_jpl_ephem`] – Access Earth’s heliocentric state from JPL ephemerides. + /// * [`Outfit::get_rot_eclmj2000_to_equmj2000`] – Rotation between ecliptic and equatorial J2000. + fn helio_position( + jpl: &JPLEphem, + epoch: &Epoch, + observer_geocentric_position: &ObserverGeocentricPosition, + ) -> Result; +} + +impl ResolvedObserver for Observer { + fn earth_fixed_position(&self) -> Result { + let (sin_lon, cos_lon): (NotNan, NotNan) = { + let (s, c) = self.longitude.sin_cos(); + (s.to_notnan()?, c.to_notnan()?) + }; + let erau_not_nan = ERAU.to_notnan()?; + + Ok(Vector3::new( + erau_not_nan * self.rho_cos_phi * cos_lon, + erau_not_nan * self.rho_cos_phi * sin_lon, + erau_not_nan * self.rho_sin_phi, + )) + } + + #[inline] + fn earth_fixed_velocity(&self) -> Result { + Ok(EARTH_ROTATION + .to_notnan()? + .cross(&self.earth_fixed_position()?)) + } + + fn pvobs( + tmjd: &Epoch, + ut1_provider: &Ut1Provider, + observer_fixed_vectors: &ObserverFixedCache, + ) -> Result<(ObserverGeocentricPosition, ObserverGeocentricVelocity), OutfitError> { + // Get observer position and velocity in the Earth-fixed frame + let dxbf = observer_fixed_vectors.position(); + let dvbf = observer_fixed_vectors.velocity(); + + // deviation from Orbfit, use of another conversion from MJD UTC (ET scale) to UT1 scale + // based on the hifitime crate + let mjd_ut1 = tmjd.to_ut1(ut1_provider); + let tut = mjd_ut1.to_mjd_tai_days(); + + // Compute the Greenwich sideral apparent time + let gast = gmst(tut) + equequ(tmjd.to_mjd_tt_days()); + + // Earth rotation matrix + let rot = rotmt(-gast, 2); + + // Compute the rotation matrix from equatorial mean J2000 to ecliptic mean J2000 + let rer_sys1 = RefSystem::Equt(RefEpoch::Epoch(tmjd.to_mjd_tt_days())); + let rer_sys2 = RefSystem::Eclm(RefEpoch::J2000); + let rot1 = rotpn(&rer_sys1, &rer_sys2)?; + + let rot1_mat = rot1.transpose().to_notnan()?; + let rot_mat = rot.transpose().to_notnan()?; + + let rotmat = rot1_mat * rot_mat; + + // Apply transformation to the observer position and velocity + let dx = rotmat * dxbf; + let dv = rotmat * dvbf; + + Ok((dx, dv)) + } + + fn helio_position( + jpl: &JPLEphem, + epoch: &Epoch, + observer_geocentric_position: &ObserverGeocentricPosition, + ) -> Result { + // Earth's heliocentric position + let earth_pos = jpl.earth_ephemeris(epoch, false).0.to_notnan()?; + + // Transform observer position from ecliptic to equatorial J2000 + let rot_matrix = ROT_ECLMJ2000_TO_EQUMJ2000.to_notnan()?.transpose(); + + let helio_pos = earth_pos + rot_matrix * observer_geocentric_position; + + Ok(helio_pos) + } +} diff --git a/src/observers/bimap.rs b/src/observers/bimap.rs deleted file mode 100644 index dd9ec03..0000000 --- a/src/observers/bimap.rs +++ /dev/null @@ -1,224 +0,0 @@ -use std::collections::HashMap; -use std::hash::Hash; - -#[derive(Debug, Clone)] -pub struct BiMap -where - K: Eq + Hash + Clone, - V: Eq + Hash + Clone, -{ - forward: HashMap, - reverse: HashMap, -} - -impl Default for BiMap -where - K: Eq + Hash + Clone, - V: Eq + Hash + Clone, -{ - fn default() -> Self { - Self::new() - } -} - -impl BiMap -where - K: Eq + Hash + Clone, - V: Eq + Hash + Clone, -{ - pub fn new() -> Self { - Self { - forward: HashMap::new(), - reverse: HashMap::new(), - } - } - - pub fn entry_or_insert_by_key(&mut self, key: K, value: V) -> &mut V { - self.forward.entry(key.clone()).or_insert_with(|| { - self.reverse.insert(value.clone(), key); - value - }) - } - - pub fn entry_or_insert_by_value(&mut self, value: V, key: K) -> &mut K { - self.reverse.entry(value.clone()).or_insert_with(|| { - self.forward.insert(key.clone(), value); - key - }) - } - - pub fn insert(&mut self, key: K, value: V) { - self.forward.insert(key.clone(), value.clone()); - self.reverse.insert(value, key); - } - - pub fn get_by_key(&self, key: &K) -> Option<&V> { - self.forward.get(key) - } - - pub fn get_by_value(&self, value: &V) -> Option<&K> { - self.reverse.get(value) - } - - pub fn remove_by_key(&mut self, key: &K) { - if let Some(val) = self.forward.remove(key) { - self.reverse.remove(&val); - } - } - - pub fn remove_by_value(&mut self, value: &V) { - if let Some(key) = self.reverse.remove(value) { - self.forward.remove(&key); - } - } - - pub fn len(&self) -> usize { - self.forward.len() - } - - pub fn is_empty(&self) -> bool { - self.len() == 0 - } - - // --------------------------- - // Iteration helpers (immutable) - // --------------------------- - - /// Iterate over (&K, &V) using the forward map. - /// - /// Return - /// ---------- - /// * An iterator yielding `(&K, &V)` pairs. Order is not guaranteed. - /// - /// See also - /// ------------ - /// * [`BiMap::iter_rev`] - /// * [`BiMap::keys`], [`BiMap::values`] - pub fn iter(&self) -> impl Iterator { - self.forward.iter() - } - - /// Iterate over (&V, &K) using the reverse map. - /// - /// Return - /// ---------- - /// * An iterator yielding `(&V, &K)` pairs. Order is not guaranteed. - /// - /// See also - /// ------------ - /// * [`BiMap::iter`] - pub fn iter_rev(&self) -> impl Iterator { - self.reverse.iter() - } - - /// Iterate over keys (&K). - pub fn keys(&self) -> impl Iterator { - self.forward.keys() - } - - /// Iterate over values (&V). - pub fn values(&self) -> impl Iterator { - self.forward.values() - } -} - -// --------------------------- -// IntoIterator implementations -// --------------------------- - -impl<'a, K, V> IntoIterator for &'a BiMap -where - K: Eq + Hash + Clone, - V: Eq + Hash + Clone, -{ - type Item = (&'a K, &'a V); - type IntoIter = std::collections::hash_map::Iter<'a, K, V>; - - /// Consume `&BiMap` into an iterator over `(&K, &V)` on the forward map. - fn into_iter(self) -> Self::IntoIter { - self.forward.iter() - } -} - -impl<'a, K, V> IntoIterator for &'a mut BiMap -where - K: Eq + Hash + Clone, - V: Eq + Hash + Clone, -{ - type Item = (&'a K, &'a mut V); - type IntoIter = std::collections::hash_map::IterMut<'a, K, V>; - - /// Consume `&mut BiMap` into an iterator over `(&K, &mut V)` on the forward map. - /// - /// Warning - /// ------- - /// Mutating values can desynchronize the reverse map if you change logical identity. - /// Use with care; prefer removing/re-inserting pairs instead. - fn into_iter(self) -> Self::IntoIter { - self.forward.iter_mut() - } -} - -impl IntoIterator for BiMap -where - K: Eq + Hash + Clone, - V: Eq + Hash + Clone, -{ - type Item = (K, V); - type IntoIter = std::collections::hash_map::IntoIter; - - /// Consume the bimap and iterate over owned `(K, V)` pairs using the forward map. - fn into_iter(self) -> Self::IntoIter { - self.forward.into_iter() - } -} - -#[cfg(test)] -mod bimap_iter_tests { - use super::*; - use std::collections::HashSet; - - #[test] - fn iter_and_iter_rev_cover_same_pairs() { - let mut m = BiMap::new(); - m.insert("a", 1); - m.insert("b", 2); - m.insert("c", 3); - - let fwd: HashSet<_> = m.iter().map(|(k, v)| ((*k).to_string(), *v)).collect(); - let rev: HashSet<_> = m.iter_rev().map(|(v, k)| ((*k).to_string(), *v)).collect(); - assert_eq!(fwd, rev); - } - - #[test] - fn into_iterator_by_ref_and_by_value() { - let mut m = BiMap::new(); - m.insert("x", 10); - m.insert("y", 20); - - // &BiMap - let pairs_ref: HashSet<_> = (&m) - .into_iter() - .map(|(k, v)| ((*k).to_string(), *v)) - .collect(); - assert!(pairs_ref.contains(&("x".to_string(), 10))); - assert!(pairs_ref.contains(&("y".to_string(), 20))); - - // BiMap (by value) - let pairs_val: HashSet<_> = m.into_iter().collect(); - assert!(pairs_val.contains(&("x", 10))); - assert!(pairs_val.contains(&("y", 20))); - // m is moved here; no further use - } - - #[test] - fn keys_and_values_match_len() { - let mut m = BiMap::new(); - m.insert(1, "one"); - m.insert(2, "two"); - m.insert(3, "three"); - - assert_eq!(m.len(), m.keys().count()); - assert_eq!(m.len(), m.values().count()); - } -} diff --git a/src/observers/mod.rs b/src/observers/mod.rs deleted file mode 100644 index eb0412d..0000000 --- a/src/observers/mod.rs +++ /dev/null @@ -1,1140 +0,0 @@ -//! # Observer & Site Geometry (top-level module) -//! -//! This module gathers **observer/site handling** and associated geometry utilities used in -//! orbit determination. It provides: -//! -//! - A robust [`Observer`](crate::observers::Observer) type storing **geocentric parallax coordinates** (ρ·cosφ, ρ·sinφ), -//! geodetic longitude, optional astrometric accuracies, and **precomputed body-fixed** position -//! and velocity vectors. -//! - High-level routines to compute the observer’s **geocentric PV** in the ecliptic J2000 frame -//! ([`Observer::pvobs`](crate::observers::Observer::pvobs)) and its **heliocentric equatorial position** ([`Observer::helio_position`](crate::observers::Observer::helio_position)). -//! - Helpers to convert geodetic latitude/elevation to normalized parallax coordinates -//! ([`geodetic_to_parallax`](crate::observers::geodetic_to_parallax)) and to lift optional floats into NaN-safe values -//! ([`to_opt_notnan`](crate::observers::to_opt_notnan)). -//! - A convenience function to compute **three observers’ heliocentric positions** at three epochs -//! in one call ([`helio_obs_pos`](crate::observers::helio_obs_pos)) — useful for Gauss/Vaisala IOD triplets. -//! -//! ## Frames & conventions -//! -//! - **Earth-fixed (body-fixed)**: the frame in which site coordinates and rotation rate are defined. -//! - **Ecliptic mean J2000**: default geocentric output of [`Observer::pvobs`](crate::observers::Observer::pvobs) (ICRS ecliptic plane). -//! - **Equatorial mean J2000**: default heliocentric output of [`Observer::helio_position`](crate::observers::Observer::helio_position) and -//! [`helio_obs_pos`](crate::observers::helio_obs_pos) (ICRS-aligned). -//! -//! ```text -//! Body-fixed --(Earth rotation)--> Earth-equatorial --(precession+nutation)--> Ecliptic J2000 -//! \-> Equatorial J2000 -//! ``` -//! -//! Internally, time-dependent Earth orientation uses **GMST** and the **equation of the equinoxes**, -//! and frame changes are performed via [`rotpn`](crate::ref_system::rotpn) / [`rotmt`](crate::ref_system::rotmt) utilities. -//! -//! ## Units -//! -//! - Longitudes: **degrees** (east positive). -//! - Geocentric parallax (ρ·cosφ, ρ·sinφ): **Earth radii** (dimensionless scaling of geocentric distance). -//! - Positions: **AU**. -//! - Velocities: **AU/day** (from `ω × r`, with `ω = (0, 0, 2π·1.00273790934)` rad/day). -//! - `ra_accuracy`, `dec_accuracy`: **radians**. -//! -//! ## Data flow (typical IOD usage) -//! -//! 1. Build an [`Observer`](crate::observers::Observer) from geodetic inputs (`longitude`, `latitude`, `elevation`) via -//! [`Observer::new`](crate::observers::Observer::new) (internally calls [`geodetic_to_parallax`](crate::observers::geodetic_to_parallax)) **or** from known (ρ·cosφ, ρ·sinφ) -//! via [`Observer::from_parallax`](crate::observers::Observer::from_parallax). -//! 2. Compute geocentric PV in **ecliptic J2000** with [`Observer::pvobs`](crate::observers::Observer::pvobs) (needs UT1 provider). -//! 3. Obtain Earth heliocentric state from JPL ephemerides and sum to get the observer’s -//! **heliocentric equatorial** position with [`Observer::helio_position`](crate::observers::Observer::helio_position). -//! 4. For triplets, call [`helio_obs_pos`](crate::observers::helio_obs_pos) to get the 3×3 matrix of heliocentric positions. -//! -//! ## Quick start -//! -//! ```rust,no_run -//! use hifitime::{Epoch, TimeScale}; -//! use nalgebra::{Vector3, Matrix3}; -//! use outfit::outfit::Outfit; -//! use outfit::error_models::ErrorModel; -//! use outfit::observers::{Observer, helio_obs_pos}; -//! -//! // 1) Environment (JPL ephem + UT1) and site -//! let state = Outfit::new("horizon:DE440", ErrorModel::FCCT14)?; -//! let site = Observer::new(203.74409, 20.707233557, 3067.694, Some("Pan-STARRS 1".into()), None, None)?; -//! -////! // 2) Geocentric PV (ecliptic J2000) -//! let t = Epoch::from_mjd_in_time_scale(57028.479297592596, TimeScale::TT); -//! let (_x_ecl, _v_ecl) = site.pvobs(&t, state.get_ut1_provider())?; -//! -//! // 3) Heliocentric position (equatorial J2000) -//! let r_helio_eq = site.helio_position(&state, &t, &Vector3::identity())?; -//! -//! // 4) Batch (3 observers, 3 epochs) -//! let tmjd = Vector3::new(57028.479297592596, 57049.24514759259, 57063.97711759259); -//! let R: Matrix3 = helio_obs_pos([&site, &site, &site], &tmjd, &state)?; -//! # Ok::<(), outfit::outfit_errors::OutfitError>(()) -//! ``` -//! -//! ## Design & invariants -//! -//! - [`Observer`](crate::observers::Observer) stores **precomputed body-fixed** position and velocity to avoid recomputing -//! `ω × r` and trigonometric terms at every call. This is beneficial in tight IOD loops. -//! - `NotNan` is used for fields where **NaN must be forbidden** (e.g., site geometry). -//! Use [`to_opt_notnan`](crate::observers::to_opt_notnan) for optional measurement accuracies. -//! - The geodetic-to-parallax conversion accounts for Earth oblateness via -//! [`EARTH_MAJOR_AXIS`](crate::constants::EARTH_MAJOR_AXIS) / [`EARTH_MINOR_AXIS`](crate::constants::EARTH_MINOR_AXIS). -//! -//! ## Errors -//! -//! - Constructors and helpers return [`OutfitError`](crate::outfit_errors::OutfitError) when NaNs are encountered or a frame -//! conversion fails; [`to_opt_notnan`](crate::observers::to_opt_notnan) returns `ordered_float::FloatIsNan` if given `Some(NaN)`. -//! -//! ## Testing -//! -//! The module includes unit tests for site construction, body-fixed coordinates, -//! geocentric PV against known values, and multi-epoch heliocentric positions (behind the -//! `jpl-download` feature). -//! -//! ## See also -//! ------------ -//! * [`Observer`](crate::observers::Observer) – Site container with precomputed body-fixed state. -//! * [`Observer::pvobs`](crate::observers::Observer::pvobs) – Geocentric PV in **ecliptic J2000**. -//! * [`Observer::helio_position`](crate::observers::Observer::helio_position) – Heliocentric **equatorial J2000** position. -//! * [`helio_obs_pos`](crate::observers::helio_obs_pos) – Batch heliocentric positions for triplets. -//! * [`geodetic_to_parallax`](crate::observers::geodetic_to_parallax) – Geodetic latitude/elevation → (ρ·cosφ, ρ·sinφ). -//! * [`rotpn`](crate::ref_system::rotpn), [`rotmt`](crate::ref_system::rotmt) – Reference-frame transformations. -//! * [`gmst`](crate::time::gmst), [`equequ`](crate::earth_orientation::equequ) – Earth orientation (sidereal time & equation of equinoxes). -//! * [`Outfit`](crate::outfit::Outfit) – Access to JPL ephemerides and UT1 provider. - -pub mod bimap; -pub mod observatories; - -use hifitime::ut1::Ut1Provider; -use hifitime::Epoch; -use nalgebra::{Matrix3, Vector3}; -use ordered_float::NotNan; - -use crate::constants::{Degree, Meter, EARTH_MAJOR_AXIS, EARTH_MINOR_AXIS, MJD}; -use crate::constants::{DPI, ERAU}; -use crate::earth_orientation::equequ; -use crate::outfit::Outfit; -use crate::outfit_errors::OutfitError; -use crate::ref_system::{rotmt, rotpn, RefEpoch, RefSystem}; -use crate::time::gmst; -use std::fmt; - -/// Convert an `Option` into an `Option>`, propagating `NaN` as an error. -/// -/// This helper lifts a possibly missing floating-point value into a `NotNan` container -/// while keeping the outer `Option`. If the inner value is `Some(x)` and `x.is_nan()`, -/// the function returns `Err(FloatIsNan)`. If it is `None`, the result is `Ok(None)`. -/// -/// Arguments -/// ----------------- -/// * `x`: The optional floating-point value to wrap. -/// -/// Return -/// ---------- -/// * A `Result` containing `Some(NotNan)` when `x` is finite, `Ok(None)` when `x` is `None`, -/// or an error if `x` is `NaN`. -/// -/// Errors -/// ---------- -/// * `ordered_float::FloatIsNan` if `x` is `Some(NaN)`. -/// -/// See also -/// ------------ -/// * [`ordered_float::NotNan`] – NaN-forbidding wrapper used across the crate. -#[inline] -pub fn to_opt_notnan(x: Option) -> Result>, ordered_float::FloatIsNan> { - x.map(NotNan::new).transpose() -} - -/// Observer geocentric parameters and precomputed body-fixed state. -/// -/// This struct stores: -/// - The observer's **geocentric parallax coordinates** (ρ·cosφ, ρ·sinφ), where ρ is the -/// geocentric distance in **Earth radii** and φ is the **geocentric** latitude. -/// - The **geodetic longitude** (degrees, east of Greenwich). -/// - Optional **astrometric accuracies** for right ascension and declination (radians). -/// - Precomputed **body-fixed** position and velocity vectors used in orbit determination. -/// -/// Units -/// ----- -/// * `longitude`: degrees (east positive). -/// * `rho_cos_phi`, `rho_sin_phi`: Earth radii (dimensionless scale factor ρ times trig of φ). -/// * `observer_fixed_coord`: astronomical units (AU). -/// * `observer_velocity`: AU/day (from Earth rotation cross product). -/// * `ra_accuracy`, `dec_accuracy`: radians. -/// -/// Notes -/// ----- -/// The precomputed body-fixed vectors assume a constant Earth rotation rate -/// ω = (0, 0, 2π·1.00273790934) rad/day. Position is scaled by `ERAU` (Earth radius in AU), -/// hence the resulting velocity is in AU/day. -/// -/// See also -/// ------------ -/// * [`geodetic_to_parallax`] – Converts geodetic latitude/elevation to (ρ·cosφ, ρ·sinφ). -/// * [`Observer::new`] – Construct from geodetic longitude/latitude/elevation. -/// * [`Observer::from_parallax`] – Construct directly from (ρ·cosφ, ρ·sinφ). -/// * [`crate::ref_system::rotpn`] – Reference frame rotations used elsewhere in the pipeline. -#[derive(Debug, PartialEq, Eq, Hash, Clone)] -pub struct Observer { - /// Geodetic longitude in **degrees** east of Greenwich. - pub longitude: NotNan, - - /// ρ·cosφ (geocentric latitude φ), in **Earth radii** (dimensionless scale). - pub rho_cos_phi: NotNan, - - /// ρ·sinφ (geocentric latitude φ), in **Earth radii** (dimensionless scale). - pub rho_sin_phi: NotNan, - - /// Optional human-readable site name. - pub name: Option, - - /// Right ascension measurement accuracy, in **radians** (optional). - pub ra_accuracy: Option>, - - /// Declination measurement accuracy, in **radians** (optional). - pub dec_accuracy: Option>, - - /// Precomputed **body-fixed** position of the observer in **AU**. - observer_fixed_coord: Vector3>, - - /// Precomputed **body-fixed** velocity of the observer in **AU/day**. - observer_velocity: Vector3>, -} - -impl Observer { - /// Create a new observer from geodetic coordinates. - /// - /// This constructor converts `(latitude, elevation)` into geocentric parallax - /// coordinates `(ρ·cosφ, ρ·sinφ)` using [`geodetic_to_parallax`], builds the - /// body-fixed position vector in **AU** (scaled by `ERAU`), and computes the - /// body-fixed velocity as `ω × r` with `ω = (0, 0, 2π·1.00273790934)` in rad/day, - /// yielding **AU/day**. - /// - /// Arguments - /// ----------------- - /// * `longitude`: Geodetic longitude in **degrees** (east positive). - /// * `latitude`: Geodetic latitude in **degrees**. - /// * `elevation`: Height above the reference ellipsoid in **meters**. - /// * `name`: Optional site name. - /// * `ra_accuracy`: Optional RA accuracy in **radians**. - /// * `dec_accuracy`: Optional DEC accuracy in **radians**. - /// - /// Return - /// ---------- - /// * A constructed [`Observer`] with precomputed body-fixed state. - /// - /// Errors - /// ---------- - /// * [`OutfitError`] if the inputs cannot be represented as `NotNan` (e.g., NaN encountered). - /// - /// See also - /// ------------ - /// * [`geodetic_to_parallax`] – Geodetic-to-geocentric parallax conversion. - /// * [`Observer::from_parallax`] – Build directly from (ρ·cosφ, ρ·sinφ). - /// * [`crate::ref_system::rotpn`] – Frame rotation utilities used later in the pipeline. - pub fn new( - longitude: Degree, - latitude: Degree, - elevation: Meter, - name: Option, - ra_accuracy: Option, - dec_accuracy: Option, - ) -> Result { - let (rho_cos_phi, rho_sin_phi) = geodetic_to_parallax(latitude, elevation); - - // Angular velocity of Earth rotation (rad/day) on the z-axis. - let omega: Vector3> = Vector3::new( - NotNan::new(0.0)?, - NotNan::new(0.0)?, - NotNan::new(DPI * 1.00273790934)?, - ); - - // Body-fixed position in AU from (ρ·cosφ, ρ·sinφ) scaled by Earth radius (AU). - let lon_radians = longitude.to_radians(); - let body_fixed_coord: Vector3> = Vector3::new( - NotNan::new(ERAU * rho_cos_phi * lon_radians.cos())?, - NotNan::new(ERAU * rho_cos_phi * lon_radians.sin())?, - NotNan::new(ERAU * rho_sin_phi)?, - ); - - // Body-fixed velocity from Earth rotation. - let dvbf = omega.cross(&body_fixed_coord); - - Ok(Observer { - longitude: NotNan::try_from(longitude)?, - rho_cos_phi: NotNan::try_from(rho_cos_phi)?, - rho_sin_phi: NotNan::try_from(rho_sin_phi)?, - name, - ra_accuracy: to_opt_notnan(ra_accuracy)?, - dec_accuracy: to_opt_notnan(dec_accuracy)?, - observer_fixed_coord: body_fixed_coord, - observer_velocity: dvbf, - }) - } - - /// Create a new observer from geocentric parallax coordinates. - /// - /// This constructor skips the geodetic-to-parallax conversion and directly uses - /// `(ρ·cosφ, ρ·sinφ)` to build the body-fixed position in **AU** (scaled by `ERAU`), - /// and the body-fixed velocity in **AU/day** as `ω × r` with - /// `ω = (0, 0, 2π·1.00273790934)` rad/day. - /// - /// Arguments - /// ----------------- - /// * `longitude`: Geodetic longitude in **degrees** (east positive). - /// * `rho_cos_phi`: ρ·cosφ in **Earth radii** (dimensionless). - /// * `rho_sin_phi`: ρ·sinφ in **Earth radii** (dimensionless). - /// * `name`: Optional site name. - /// * `ra_accuracy`: Optional RA accuracy in **radians**. - /// * `dec_accuracy`: Optional DEC accuracy in **radians**. - /// - /// Return - /// ---------- - /// * A constructed [`Observer`] with precomputed body-fixed state. - /// - /// Errors - /// ---------- - /// * [`OutfitError`] if inputs cannot be represented as `NotNan` (e.g., NaN encountered). - /// - /// See also - /// ------------ - /// * [`Observer::new`] – Build from geodetic latitude and elevation. - /// * [`geodetic_to_parallax`] – For the forward conversion when geodetic inputs are available. - pub fn from_parallax( - longitude: Degree, - rho_cos_phi: f64, - rho_sin_phi: f64, - name: Option, - ra_accuracy: Option, - dec_accuracy: Option, - ) -> Result { - // Angular velocity of Earth rotation (rad/day) on the z-axis. - let omega: Vector3> = Vector3::new( - NotNan::new(0.0)?, - NotNan::new(0.0)?, - NotNan::new(DPI * 1.00273790934)?, - ); - - // Body-fixed position in AU from (ρ·cosφ, ρ·sinφ) scaled by Earth radius (AU). - let lon_radians = longitude.to_radians(); - let body_fixed_coord: Vector3> = Vector3::new( - NotNan::new(ERAU * rho_cos_phi * lon_radians.cos())?, - NotNan::new(ERAU * rho_cos_phi * lon_radians.sin())?, - NotNan::new(ERAU * rho_sin_phi)?, - ); - - // Body-fixed velocity from Earth rotation. - let dvbf = omega.cross(&body_fixed_coord); - - Ok(Observer { - longitude: NotNan::try_from(longitude)?, - rho_cos_phi: NotNan::try_from(rho_cos_phi)?, - rho_sin_phi: NotNan::try_from(rho_sin_phi)?, - name, - ra_accuracy: to_opt_notnan(ra_accuracy)?, - dec_accuracy: to_opt_notnan(dec_accuracy)?, - observer_fixed_coord: body_fixed_coord, - observer_velocity: dvbf, - }) - } - - /// Get the fixed position of an observatory using its geographic coordinates - /// - /// Argument - /// -------- - /// * longitude: observer longitude in Degree - /// * latitude: observer latitude in Degree - /// * height: observer height in Degree - /// - /// Return - /// ------ - /// * observer fixed coordinates vector on the Earth (not corrected from Earth motion) - /// * units is AU - pub fn body_fixed_coord(&self) -> Vector3 { - let lon_radians = self.longitude.to_radians(); - - Vector3::new( - ERAU * self.rho_cos_phi.into_inner() * lon_radians.cos(), - ERAU * self.rho_cos_phi.into_inner() * lon_radians.sin(), - ERAU * self.rho_sin_phi.into_inner(), - ) - } - - /// Compute the observer’s geocentric position and velocity in the ecliptic J2000 frame. - /// - /// This function calculates the position and velocity of a ground-based observer relative to the Earth's - /// center of mass, accounting for Earth rotation (via GMST), nutation, and the observer’s geographic location. - /// The result is expressed in the ecliptic mean J2000 frame, suitable for use in orbital initial determination. - /// - /// Arguments - /// --------- - /// * `observer`: a reference to an [`Observer`] containing the site longitude and parallax parameters. - /// * `tmjd`: observation epoch as a [`hifitime::Epoch`] in TT. - /// * `ut1_provider`: a reference to a [`hifitime::ut1::Ut1Provider`] for accurate UT1 conversion. - /// - /// Returns - /// -------- - /// * `(dx, dv)` – Tuple of: - /// - `dx`: observer geocentric position vector in ecliptic mean J2000 frame \[AU\]. - /// - `dv`: observer velocity vector due to Earth's rotation, in the same frame \[AU/day\]. - /// - /// Remarks - /// ------- - /// * Internally, this function: - /// 1. get the body-fixed coordinates of the observer. - /// 2. get its rotational velocity: `v = ω × r`. - /// 3. Applies Earth orientation corrections using: - /// - Greenwich Mean Sidereal Time (GMST), - /// - Equation of the equinoxes, - /// - Precession and nutation transformation (`rotpn`). - /// 4. Returns position and velocity in the J2000 ecliptic frame (used in classical orbital mechanics). - /// - /// # See also - /// * [`Observer::body_fixed_coord`] – observer's base vector in Earth-fixed frame - /// * [`rotpn`] – rotation between reference frames - /// * [`gmst`], [`equequ`] – time-dependent Earth orientation - pub fn pvobs( - &self, - tmjd: &Epoch, - ut1_provider: &Ut1Provider, - ) -> Result<(Vector3, Vector3), OutfitError> { - // Get observer position and velocity in the Earth-fixed frame - let dxbf = self.observer_fixed_coord.map(|x| x.into_inner()); - let dvbf = self.observer_velocity.map(|x| x.into_inner()); - - // deviation from Orbfit, use of another conversion from MJD UTC (ET scale) to UT1 scale - // based on the hifitime crate - let mjd_ut1 = tmjd.to_ut1(ut1_provider); - let tut = mjd_ut1.to_mjd_tai_days(); - - // Compute the Greenwich sideral apparent time - let gast = gmst(tut) + equequ(tmjd.to_mjd_tt_days()); - - // Earth rotation matrix - let rot = rotmt(-gast, 2); - - // Compute the rotation matrix from equatorial mean J2000 to ecliptic mean J2000 - let rer_sys1 = RefSystem::Equt(RefEpoch::Epoch(tmjd.to_mjd_tt_days())); - let rer_sys2 = RefSystem::Eclm(RefEpoch::J2000); - let rot1 = rotpn(&rer_sys1, &rer_sys2)?; - - let rot1_mat = rot1.transpose(); - let rot_mat = rot.transpose(); - - let rotmat = rot1_mat * rot_mat; - - // Apply transformation to the observer position and velocity - let dx = rotmat * dxbf; - let dv = rotmat * dvbf; - - Ok((dx, dv)) - } - - /// Compute the observer’s heliocentric position in the **equatorial mean J2000** frame. - /// - /// This method forms the full heliocentric position of the observing site by combining: - /// - the site **geocentric** position vector at `epoch`, and - /// - the Earth’s **heliocentric** position from the JPL ephemerides. - /// - /// The input geocentric vector is assumed to be expressed in the **ecliptic mean J2000** frame - /// (AU). It is rotated to **equatorial mean J2000**, then added to Earth’s heliocentric - /// position (also in equatorial mean J2000). - /// - /// Arguments - /// ----------------- - /// * `state` – [`Outfit`] environment providing JPL ephemerides and frame rotations. - /// * `epoch` – Observation epoch in the **TT** time scale. - /// * `observer_geocentric_position` – Geocentric site position **in ecliptic mean J2000** (AU). - /// - /// Return - /// ---------- - /// * `Result, OutfitError>` – Observer’s **heliocentric** position at `epoch`, - /// in **AU**, expressed in **equatorial mean J2000**. - /// - /// Remarks - /// ------------- - /// * If your geocentric site vector is already in **equatorial** J2000, rotate it to - /// **ecliptic** before calling this method, or adapt the rotation accordingly. - /// * This routine is typically used internally when constructing per-observation geometry - /// (e.g., within `Observation::new`), ensuring consistent frames for Gauss IOD. - /// - /// See also - /// ------------ - /// * [`Observer::pvobs`] – Geocentric position (and velocity) of the site at `epoch`. - /// * [`Outfit::get_jpl_ephem`] – Access Earth’s heliocentric state from JPL ephemerides. - /// * [`Outfit::get_rot_eclmj2000_to_equmj2000`] – Rotation between ecliptic and equatorial J2000. - pub fn helio_position( - &self, - state: &Outfit, - epoch: &Epoch, - observer_geocentric_position: &Vector3, - ) -> Result, OutfitError> { - let jpl = state.get_jpl_ephem().unwrap(); - - // Earth's heliocentric position - let earth_pos = jpl.earth_ephemeris(epoch, false).0; - - // Transform observer position from ecliptic to equatorial J2000 - let rot_matrix = state.get_rot_eclmj2000_to_equmj2000().transpose(); - - Ok(earth_pos + rot_matrix * observer_geocentric_position) - } - - /// Recover geodetic latitude and ellipsoidal height (WGS-84) from parallax constants. - /// - /// Inverts the stored parallax coordinates `(ρ·cosφ, ρ·sinφ)` to the **geodetic** - /// latitude `φ` (degrees) and the ellipsoidal height `h` (meters) above the - /// WGS-84 reference ellipsoid. The computation uses **Bowring’s closed-form** - /// formula (no iteration), which is usually sufficient for double-precision - /// accuracy at the centimeter level or better. - /// - /// Units & model - /// ------------- - /// * Inputs: `ρ·cosφ` and `ρ·sinφ` are dimensionless, expressed in **Earth radii** - /// (normalized by the equatorial radius). They are scaled internally by `a` - /// (the equatorial radius) to meters. - /// * Output: latitude in **degrees**, height in **meters** (ellipsoidal height, not geoid/orthometric). - /// * Ellipsoid: WGS-84 radii from `constants.rs` (`EARTH_MAJOR_AXIS` = `a`, `EARTH_MINOR_AXIS` = `b`). - /// If you prefer exact GRS-80 reproduction, use consistent `b` there; the difference vs WGS-84 is sub-millimetric. - /// - /// Notes - /// ----- - /// * This routine **does not** compute the geodetic longitude; it only returns `(lat, h)`. - /// Your `Observer` already stores the geodetic longitude independently. - /// * Numerical robustness is good across latitudes, including near the poles. - /// * If you require bit-for-bit parity with an external reference using a different ellipsoid, - /// ensure `a`/`b` match that reference. - /// - /// Arguments - /// ----------------- - /// * None. - /// - /// Return - /// ---------- - /// * `(geodetic_latitude_deg, height_meters)` — latitude in degrees, ellipsoidal height in meters. - /// - /// See also - /// ------------ - /// * [`geodetic_to_parallax`] – Forward conversion used at construction. - /// * [`Observer::from_parallax`] – Builds an observer from `(ρ·cosφ, ρ·sinφ)`. - /// * `constants::EARTH_MAJOR_AXIS` / `constants::EARTH_MINOR_AXIS` – Ellipsoid radii used here. - pub fn geodetic_lat_height_wgs84(&self) -> (f64, f64) { - let a = EARTH_MAJOR_AXIS; - let b = EARTH_MINOR_AXIS; - let e2 = 1.0 - (b * b) / (a * a); - let ep2 = (a * a) / (b * b) - 1.0; - - let p = self.rho_cos_phi.into_inner() * a; // distance in equatorial plane [m] - let z = self.rho_sin_phi.into_inner() * a; // z [m] - - // Bowring’s formula: - let theta = (z * a).atan2(p * b); - let st = theta.sin(); - let ct = theta.cos(); - let phi = (z + ep2 * b * st.powi(3)).atan2(p - e2 * a * ct.powi(3)); - - let s = phi.sin(); - let n = a / (1.0 - e2 * s * s).sqrt(); - let h = p / phi.cos() - n; - - (phi.to_degrees(), h) - } -} - -impl fmt::Display for Observer { - /// Pretty-print an observer with optional verbose details using `{:#}` formatting. - /// - /// Default formatting (`{}`) prints a compact one-liner: - /// `Name (lon: XX.XXXXXX°, lat: YY.YYYYYY° geodetic, elev: Z.ZZ km)`. - /// - /// Alternate formatting (`{:#}`) prints a multi-line detailed block including: - /// - Parallax constants `(ρ·cosφ, ρ·sinφ)`, - /// - Geocentric latitude `φ_geo` and geocentric distance `ρ` (Earth radii), - /// - Astrometric 1-σ accuracies in arcseconds (if available). - /// - /// Arguments - /// ----------------- - /// * `self`: The observer to format. - /// - /// Return - /// ---------- - /// * A human-readable representation suitable for logs and diagnostics. - /// - /// See also - /// ------------ - /// * [`Observer::geodetic_lat_height_wgs84`] – Geodetic latitude (deg) and ellipsoidal height (m). - /// * [`geodetic_to_parallax`] – Forward conversion to `(ρ·cosφ, ρ·sinφ)`. - fn fmt(&self, f: &mut fmt::Formatter<'_>) -> fmt::Result { - // Friendly name - let name = self.name.as_deref().unwrap_or("Unnamed"); - - // Geodetic latitude (deg) and height (m -> km) - let (lat_deg, h_m) = self.geodetic_lat_height_wgs84(); - - // Geodetic longitude in degrees - let lon_deg = self.longitude.into_inner(); - - // Geocentric latitude and ρ from parallax constants - let rc = self.rho_cos_phi.into_inner(); - let rs = self.rho_sin_phi.into_inner(); - let phi_geo_deg = rs.atan2(rc).to_degrees(); - let rho_re = rc.hypot(rs); - - // Astrometric accuracies (radians -> arcseconds) - const RAD2AS: f64 = 206_264.806_247_096_36; - let ra_sigma_as = self - .ra_accuracy - .map(|v| format!("{:.3}″", v.into_inner() * RAD2AS)) - .unwrap_or_else(|| "—".to_string()); - let dec_sigma_as = self - .dec_accuracy - .map(|v| format!("{:.3}″", v.into_inner() * RAD2AS)) - .unwrap_or_else(|| "—".to_string()); - - if f.alternate() { - // Verbose, multi-line format (triggered by "{:#}") - writeln!( - f, - "{name} (lon: {lon_deg:.6}°, lat: {lat_deg:.6}° geodetic, elev: {h_m:.2} m)" - )?; - writeln!( - f, - " parallax: ρ·cosφ={rc:.9}, ρ·sinφ={rs:+.9} | φ_geo={phi_geo_deg:+.6}° ρ={rho_re:.6} RE" - )?; - write!(f, " astrometric 1σ: RA={ra_sigma_as}, DEC={dec_sigma_as}") - } else { - // Compact, single-line format (triggered by "{}") - write!( - f, - "{name} (lon: {lon_deg:.6}°, lat: {lat_deg:.6}° geodetic, elev: {h_m:.2} m)" - ) - } - } -} - -/// Convert geodetic latitude and height into normalized parallax coordinates -/// on the Earth. -/// -/// This transformation is used to compute the observer's position on Earth -/// in a way that accounts for the Earth's oblateness. The resulting values -/// are dimensionless and are expressed in units of the Earth's equatorial -/// radius (`EARTH_MAJOR_AXIS`). -/// -/// Arguments -/// --------- -/// * `lat` - Geodetic latitude of the observer in **radians**. -/// * `height` - Observer's altitude above the reference ellipsoid in **meters**. -/// -/// Returns -/// ------- -/// A tuple `(rho_cos_phi, rho_sin_phi)`: -/// * `rho_cos_phi`: normalized distance of the observer projected on -/// the Earth's equatorial plane. -/// * `rho_sin_phi`: normalized distance of the observer projected on -/// the Earth's rotation (polar) axis. -/// -/// Details -/// ------- -/// The computation uses the reference ellipsoid defined by: -/// * `EARTH_MAJOR_AXIS`: Equatorial radius (m), -/// * `EARTH_MINOR_AXIS`: Polar radius (m). -/// -/// The formula comes from standard geodetic to geocentric conversion: -/// -/// ```text -/// u = atan( (sin φ * (b/a)) / cos φ ) -/// ρ_sinφ = (b/a) * sin u + (h/a) * sin φ -/// ρ_cosφ = cos u + (h/a) * cos φ -/// ``` -/// -/// where `a` and `b` are the Earth's semi-major and semi-minor axes, -/// and `h` is the height above the ellipsoid. -/// -/// See also -/// -------- -/// * [`Observer::body_fixed_coord`] – Uses this function to compute -/// the observer's fixed position in Earth-centered coordinates. -pub fn lat_alt_to_parallax(lat: f64, height: f64) -> (f64, f64) { - // Ratio of the Earth's minor to major axis (flattening factor) - let axis_ratio = EARTH_MINOR_AXIS / EARTH_MAJOR_AXIS; - - // Compute the auxiliary angle u (parametric latitude) - // This corrects for the Earth's oblateness. - let u = (lat.sin() * axis_ratio).atan2(lat.cos()); - - // Compute the normalized distance along the polar axis - let rho_sin_phi = axis_ratio * u.sin() + (height / EARTH_MAJOR_AXIS) * lat.sin(); - - // Compute the normalized distance along the equatorial plane - let rho_cos_phi = u.cos() + (height / EARTH_MAJOR_AXIS) * lat.cos(); - - (rho_cos_phi, rho_sin_phi) -} - -/// Convert geodetic latitude (in degrees) and height (in meters) -/// into normalized parallax coordinates. -/// -/// This is a convenience wrapper around [`lat_alt_to_parallax`] that -/// performs the degrees-to-radians conversion before calling the main -/// function. -/// -/// Arguments -/// --------- -/// * `lat` - Geodetic latitude of the observer in **degrees**. -/// * `height` - Observer's altitude above the reference ellipsoid in **meters**. -/// -/// Returns -/// ------- -/// A tuple `(rho_cos_phi, rho_sin_phi)`: -/// * `rho_cos_phi`: normalized distance of the observer projected on -/// the Earth's equatorial plane. -/// * `rho_sin_phi`: normalized distance of the observer projected on -/// the Earth's rotation (polar) axis. -/// -/// Details -/// ------- -/// This function simply converts `lat` to radians and delegates the -/// computation to [`lat_alt_to_parallax`]. -/// -/// See also -/// -------- -/// * [`lat_alt_to_parallax`] – Performs the actual computation given latitude in radians. -pub fn geodetic_to_parallax(lat: f64, height: f64) -> (f64, f64) { - // Convert latitude from degrees to radians - let latitude_rad = lat.to_radians(); - - // Call the main routine that works with radians - let (rho_cos_phi, rho_sin_phi) = lat_alt_to_parallax(latitude_rad, height); - - (rho_cos_phi, rho_sin_phi) -} - -/// Compute the heliocentric positions of three observers at their respective epochs, -/// expressed in the **equatorial mean J2000** frame (ICRS-aligned). -/// -/// Overview -/// ----------------- -/// This routine builds a `3×3` matrix of observer positions by combining: -/// - the **geocentric site position** of each observer (from [`Observer::pvobs`]), -/// - the Earth’s **heliocentric barycentric position** from JPL ephemerides, -/// - a frame transformation from **ecliptic mean J2000** (site positions) to -/// **equatorial mean J2000** (final output). -/// -/// The result is a compact representation where each column corresponds to one -/// observer/epoch pair: -/// `observers[0] ↔ mjd_tt.x`, -/// `observers[1] ↔ mjd_tt.y`, -/// `observers[2] ↔ mjd_tt.z`. -/// -/// Arguments -/// ----------------- -/// * `observers` – Array of three [`Observer`] references, each encoding the site geometry -/// (longitude, normalized geocentric radius components, etc.). -/// * `mjd_tt` – [`Vector3`] of observation epochs in Terrestrial Time (TT), one per observer. -/// * `state` – [`Outfit`] environment providing: -/// - JPL planetary ephemerides (via [`Outfit::get_jpl_ephem`]), -/// - UT1 provider for Earth rotation/orientation (via [`Outfit::get_ut1_provider`]). -/// -/// Return -/// ---------- -/// * `Result, OutfitError>` – A 3×3 matrix of observer heliocentric positions, with: -/// - **Columns** = `[r₁, r₂, r₃]`, one per observer/epoch, -/// - **Units** = astronomical units (AU), -/// - **Frame** = equatorial mean J2000 (ICRS-aligned). -/// -/// Remarks -/// ------------- -/// * For each observer/time pair: -/// 1. The site’s **geocentric position** is computed via [`Observer::pvobs`] (AU, ecliptic J2000). -/// 2. Earth’s heliocentric position is retrieved from the JPL ephemeris. -/// 3. The site position is rotated into **equatorial mean J2000** using the frame rotation. -/// 4. The Earth + rotated site vectors give the full heliocentric observer position. -/// * This function is mainly used during **Gauss IOD** preparation to populate the -/// observer position matrix stored in [`GaussObs`](crate::initial_orbit_determination::gauss::GaussObs). -/// -/// See also -/// ------------ -/// * [`Observer::pvobs`] – Geocentric observer position at a given epoch (ecliptic J2000). -/// * [`Observer::helio_position`] – Per-observer heliocentric position (equatorial J2000). -/// * [`Outfit::get_jpl_ephem`] – Access to planetary ephemerides (Earth state). -/// * [`Outfit::get_ut1_provider`] – Provides Earth orientation parameters (ΔUT1). -pub fn helio_obs_pos( - observers: [&Observer; 3], - mjd_tt: &Vector3, - state: &Outfit, -) -> Result, OutfitError> { - let epochs = [ - Epoch::from_mjd_in_time_scale(mjd_tt.x, hifitime::TimeScale::TT), - Epoch::from_mjd_in_time_scale(mjd_tt.y, hifitime::TimeScale::TT), - Epoch::from_mjd_in_time_scale(mjd_tt.z, hifitime::TimeScale::TT), - ]; - - let pvobs1 = observers[0].pvobs(&epochs[0], state.get_ut1_provider())?; - let pvobs2 = observers[1].pvobs(&epochs[1], state.get_ut1_provider())?; - let pvobs3 = observers[2].pvobs(&epochs[2], state.get_ut1_provider())?; - - let positions = [ - observers[0].helio_position(state, &epochs[0], &pvobs1.0)?, - observers[1].helio_position(state, &epochs[1], &pvobs2.0)?, - observers[2].helio_position(state, &epochs[2], &pvobs3.0)?, - ]; - - Ok(Matrix3::from_columns(&positions)) -} - -#[cfg(test)] -mod observer_test { - - use crate::{error_models::ErrorModel, outfit::Outfit}; - - use super::*; - - #[test] - fn test_observer_constructor() { - let observer = Observer::new(0.0, 0.0, 0.0, None, None, None).unwrap(); - assert_eq!(observer.longitude, 0.0); - assert_eq!(observer.rho_cos_phi, 1.0); - assert_eq!(observer.rho_sin_phi, 0.0); - - let observer = Observer::new( - 289.25058, - -30.2446, - 2647., - Some("Rubin Observatory".to_string()), - Some(0.0001), - Some(0.0001), - ) - .unwrap(); - - assert_eq!(observer.longitude, 289.25058); - assert_eq!(observer.rho_cos_phi, 0.8649760504617418); - assert_eq!(observer.rho_sin_phi, -0.5009551027512434); - } - - #[test] - fn body_fixed_coord_test() { - // longitude, latitude and height of Pan-STARRS 1, Haleakala - let (lon, lat, h) = (203.744090000, 20.707233557, 3067.694); - let pan_starrs = Observer::new(lon, lat, h, None, None, None).unwrap(); - assert_eq!( - pan_starrs.body_fixed_coord(), - Vector3::new( - -0.00003653799439776371, - -0.00001607260397528885, - 0.000014988110430544328 - ) - ); - - assert_eq!( - pan_starrs.observer_fixed_coord, - Vector3::new( - NotNan::new(-0.00003653799439776371).unwrap(), - NotNan::new(-0.00001607260397528885).unwrap(), - NotNan::new(0.000014988110430544328).unwrap() - ) - ) - } - - #[test] - fn pvobs_test() { - let state = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap(); - let tmjd = 57028.479297592596; - let epoch = Epoch::from_mjd_in_time_scale(tmjd, hifitime::TimeScale::TT); - // longitude, latitude and height of Pan-STARRS 1, Haleakala - let (lon, lat, h) = (203.744090000, 20.707233557, 3067.694); - let pan_starrs = - Observer::new(lon, lat, h, Some("Pan-STARRS 1".to_string()), None, None).unwrap(); - - let (observer_position, observer_velocity) = - &pan_starrs.pvobs(&epoch, state.get_ut1_provider()).unwrap(); - - assert_eq!( - observer_position.as_slice(), - [ - -2.086211182493635e-5, - 3.718476815327979e-5, - 2.4978996447997476e-7 - ] - ); - assert_eq!( - observer_velocity.as_slice(), - [ - -0.0002143246535691577, - -0.00012059801691431748, - 5.262184624215718e-5 - ] - ); - } - - #[test] - fn geodetic_to_parallax_test() { - // latitude and height of Pan-STARRS 1, Haleakala - let (pxy1, pz1) = geodetic_to_parallax(20.707233557, 3067.694); - assert_eq!(pxy1, 0.9362410003211518); - assert_eq!(pz1, 0.35154299856304305); - } - - #[test] - #[cfg(feature = "jpl-download")] - fn test_helio_pos_obs() { - use crate::unit_test_global::OUTFIT_HORIZON_TEST; - - let tmjd = Vector3::new( - 57028.479297592596, - 57_049.245_147_592_59, - 57_063.977_117_592_59, - ); - - // longitude, latitude and height of Pan-STARRS 1, Haleakala - let (lon, lat, h) = (203.744090000, 20.707233557, 3067.694); - let pan_starrs = - Observer::new(lon, lat, h, Some("Pan-STARRS 1".to_string()), None, None).unwrap(); - - // Now we need a Vector3 with three identical copies - let observers = [&pan_starrs, &pan_starrs, &pan_starrs]; - - let helio_pos = helio_obs_pos(observers, &tmjd, &OUTFIT_HORIZON_TEST.0).unwrap(); - - assert_eq!( - helio_pos.as_slice(), - [ - -0.2645666171464416, - 0.8689351643701766, - 0.3766996211107864, - -0.5891631852137064, - 0.7238872516824697, - 0.3138186516540669, - -0.7743280306286537, - 0.5612532665812755, - 0.24333415479994636 - ] - ); - } - - #[cfg(test)] - mod geodetic_inverse_tests { - use super::*; - use crate::constants::Degree; - use approx::assert_abs_diff_eq; - - /// Round-trip a single site through (lon, lat, h) -> parallax -> inverse - /// and check that we recover the original geodetic latitude & height. - /// - /// Notes - /// ----- - /// * `Observer::new` is given `h_m` in meters (as per current API usage). - /// * `geodetic_lat_height_wgs84()` returns height in **meters**; we convert to meters. - fn roundtrip_site(name: &str, lon_deg: Degree, lat_deg: Degree, h_m: f64) { - // Build observer (forward: geodetic -> parallax is done inside `Observer::new`) - let obs = Observer::new(lon_deg, lat_deg, h_m, Some(name.to_string()), None, None) - .expect("Failed to create observer"); - - // Inverse: parallax -> geodetic (WGS-84) - let (lat_rec_deg, h_rec_m) = obs.geodetic_lat_height_wgs84(); - - // Tolerances: - // - Latitude: 1e-6 deg (~3.6 mas) – tight but should pass for double precision Bowring + 0–1 Newton step - // - Height: 1e-2 m - let tol_lat_deg = 1e-6; - let tol_h_m = 1e-2; - - assert_abs_diff_eq!(lat_rec_deg, lat_deg, epsilon = tol_lat_deg); - assert_abs_diff_eq!(h_rec_m, h_m, epsilon = tol_h_m); - } - - /// See also - /// ------------ - /// * [`Observer::new`] – Forward geodetic->parallax conversion under test by round-trip. - /// * [`Observer::from_parallax`] – Alternative constructor, if you want to inject ρ·cosφ/ρ·sinφ. - /// * `geodetic_to_parallax` – The forward routine used internally by `Observer::new`. - - #[test] - fn geodetic_roundtrip_known_observatories_wgs84() { - // NOTE: - // The heights below are commonly quoted "above sea level" (orthometric). - // For pure algorithmic round-trip testing, that's acceptable because we feed - // the same height into forward and inverse. If you want strict ellipsoidal - // (h) values, substitute official WGS-84 heights here. - let sites: &[(&str, Degree, Degree, f64)] = &[ - // name, lon_deg (E+), lat_deg (N+), height_m - ("Haleakala (PS1 I41)", -156.2575, 20.7075, 3055.0), - ("Mauna Kea (CFHT)", -155.4700, 19.8261, 4205.0), - ("ESO Paranal", -70.4025, -24.6252, 2635.0), - ("Cerro Pachon (Rubin)", -70.7366, -30.2407, 2663.0), - ("La Silla", -70.7346, -29.2613, 2400.0), - ("Kitt Peak", -111.5967, 31.9583, 2096.0), - ("Roque de los Muchachos", -17.8947, 28.7606, 2396.0), - ]; - - for (name, lon, lat, h_m) in sites.iter().copied() { - roundtrip_site(name, lon, lat, h_m); - } - } - - #[test] - fn geodetic_roundtrip_extremes_equator_and_pole() { - // Equator, sea level - roundtrip_site("Equator (0°, 0 m)", 0.0, 0.0, 0.0); - - // Near-North-Pole and Near-South-Pole with modest height - roundtrip_site("Near North Pole", 0.0, 89.999, 1000.0); - roundtrip_site("Near South Pole", 0.0, -89.999, 1000.0); - } - - #[test] - fn geodetic_roundtrip_high_altitude_and_negative() { - // Very high site (simulate balloon/aircraft) - roundtrip_site("High Alt 10 m", 10.0, 45.0, 10_000.0); - - // Negative height (below ellipsoid, synthetic but tests robustness) - roundtrip_site("Below ellipsoid -50 m", -30.0, -10.0, -50.0); - } - } - - #[cfg(test)] - mod observer_display_tests { - use super::*; - - /// Convert arcseconds to radians. - #[inline] - fn arcsec_to_rad(as_val: f64) -> f64 { - // 1 arcsec = π / (180 * 3600) rad - std::f64::consts::PI / (180.0 * 3600.0) * as_val - } - - /// Helper to build an Observer with optional RA/DEC accuracies (in arcseconds). - fn make_observer_with_acc( - name: Option<&str>, - lon_deg: f64, - lat_deg: f64, - elev_m: f64, - ra_as: Option, - dec_as: Option, - ) -> Observer { - let ra_sigma = ra_as.map(arcsec_to_rad); - let dec_sigma = dec_as.map(arcsec_to_rad); - - Observer::new( - lon_deg, - lat_deg, - elev_m, // elevation in meters - name.map(|s| s.to_string()), - ra_sigma, - dec_sigma, - ) - .expect("Failed to create Observer") - } - - /// Compact formatting must be a single line with name/lon/lat/elev. - #[test] - fn display_compact_single_line() { - let obs = make_observer_with_acc(Some("TestSite"), 10.0, 0.0, 0.0, None, None); - - let s = format!("{obs}"); - // Must not contain newlines in compact form - assert!( - !s.contains('\n'), - "Compact format should be single-line, got:\n{s}" - ); - - // Must contain expected fragments (predictable numbers) - assert!( - s.contains("TestSite (lon: 10.000000°"), - "Missing name/lon fragment. Got:\n{s}" - ); - assert!( - s.contains("lat: 0.000000° geodetic"), - "Missing geodetic latitude fragment. Got:\n{s}" - ); - assert!( - s.contains("elev: 0.00 m"), - "Missing elevation fragment (m). Got:\n{s}" - ); - } - - /// Alternate formatting must be multi-line and include parallax & uncertainties. - #[test] - fn display_verbose_multiline_with_sections() { - let obs = make_observer_with_acc(Some("VerboseSite"), -70.0, -30.0, 2400.0, None, None); - - let s = format!("{obs:#}"); - - // Must contain multiple lines and the expected section headers/fragments - assert!( - s.contains('\n'), - "Verbose format should be multi-line. Got:\n{s}" - ); - assert!( - s.starts_with("VerboseSite (lon: -70.000000°"), - "First line should start with site name and lon. Got:\n{s}" - ); - assert!( - s.contains("\n parallax: ρ·cosφ="), - "Missing 'parallax:' line. Got:\n{s}" - ); - assert!( - s.contains("φ_geo=") && s.contains("ρ="), - "Missing φ_geo/ρ fragments. Got:\n{s}" - ); - assert!( - s.contains("\n astrometric 1σ: RA=—, DEC=—"), - "Missing astrometric 1σ line with em-dashes for None. Got:\n{s}" - ); - } - - /// When RA/DEC accuracies are provided, they must be printed in arcseconds with three decimals. - #[test] - fn display_verbose_shows_ra_dec_sigmas() { - // RA = 1.0″, DEC = 2.5″ (passed in arcseconds, converted to radians internally) - let obs = make_observer_with_acc(Some("AccSite"), 0.0, 0.0, 0.0, Some(1.0), Some(2.5)); - - let s = format!("{obs:#}"); - - assert!( - s.contains("astrometric 1σ: RA=1.000″, DEC=2.500″"), - "Expected RA/DEC sigma in arcseconds with 3 decimals. Got:\n{s}" - ); - } - - /// Name fallback should be "Unnamed" when not provided. - #[test] - fn display_uses_unnamed_when_missing() { - let obs = make_observer_with_acc(None, 5.0, 0.0, 0.0, None, None); - let s = format!("{obs}"); - assert!( - s.starts_with("Unnamed (lon: 5.000000°"), - "Expected 'Unnamed' fallback. Got:\n{s}" - ); - } - - /// Basic numeric sanity: geodetic height is shown in kilometers in the display. - /// For a 3055 m elevation, we expect ~3.055 km (rounded to 2 decimals). - #[test] - fn display_elevation_shown_in_km() { - let obs = make_observer_with_acc( - Some("Haleakala-ish"), - -156.2575, - 20.7075, - 3055.0, - None, - None, - ); - - let s = format!("{obs}"); - // Check the km conversion and rounding only; don't assert on latitude value here. - assert!( - s.contains("elev: 3055.00 m"), - "Expected elevation ~3055 m rounded to 2 decimals. Got:\n{s}" - ); - - // Optional: ensure lon is printed correctly - assert!( - s.contains("lon: -156.257500°"), - "Longitude formatting mismatch. Got:\n{s}" - ); - } - } -} diff --git a/src/observers/observatories.rs b/src/observers/observatories.rs deleted file mode 100644 index 636947b..0000000 --- a/src/observers/observatories.rs +++ /dev/null @@ -1,238 +0,0 @@ -use super::bimap::BiMap; -use super::Observer; -use crate::constants::{Degree, Kilometer, MpcCodeObs}; -use std::{ - fmt, - sync::{Arc, OnceLock}, -}; - -#[derive(Debug, Clone)] -pub(crate) struct Observatories { - pub(crate) mpc_code_obs: OnceLock, - obs_to_uint16: BiMap, u16>, -} - -impl Observatories { - pub(crate) fn new() -> Self { - Observatories { - mpc_code_obs: OnceLock::new(), - obs_to_uint16: BiMap::new(), - } - } - - pub(crate) fn create_observer( - &mut self, - longitude: Degree, - latitude: Degree, - elevation: Kilometer, - name: Option, - ) -> Arc { - let obs = Observer::new(longitude, latitude, elevation, name.clone(), None, None) - .expect("Failed to create observer"); - let arc_observer = Arc::new(obs); - self.obs_to_uint16 - .entry_or_insert_by_key(arc_observer.clone(), self.obs_to_uint16.len() as u16); - arc_observer - } - - pub(crate) fn add_observer(&mut self, observer: Arc) -> u16 { - let obs_idx = self.obs_to_uint16.len() as u16; - *self.obs_to_uint16.entry_or_insert_by_key(observer, obs_idx) - } - - /// Get an observer from an observer index - /// - /// Arguments - /// --------- - /// * `observer_idx`: the observer index - /// - /// Return - /// ------ - /// * The observer - pub(crate) fn get_observer_from_uint16(&self, observer_idx: u16) -> &Observer { - self.obs_to_uint16 - .get_by_value(&observer_idx) - .unwrap_or_else(|| panic!("Observer index not found: {observer_idx}")) - } - - /// Get an observer index from an observer - /// If the observer is not already in the bimap, it is added - /// - /// Arguments - /// --------- - /// * `observer`: the observer - /// - /// Return - /// ------ - /// * The observer index - pub(crate) fn uint16_from_observer(&mut self, observer: Arc) -> u16 { - let obs_idx = self.obs_to_uint16.len() as u16; - *self.obs_to_uint16.entry_or_insert_by_key(observer, obs_idx) - } -} - -impl fmt::Display for Observatories { - fn fmt(&self, f: &mut fmt::Formatter<'_>) -> fmt::Result { - if self.obs_to_uint16.is_empty() { - if self.mpc_code_obs.get().is_none() { - writeln!(f, "No observatories defined (user or MPC).\nTrying to get an observer from the MPC or insert a new one to initialize the observatory list.")?; - return Ok(()); - } else { - writeln!(f, "No user-defined observers.")?; - } - } - - writeln!(f, "User-defined observers:")?; - for obs in self.obs_to_uint16.keys() { - let (lat, height) = obs.geodetic_lat_height_wgs84(); - - writeln!( - f, - " {} (lon: {:.6}°, lat: {:.6}°, elev: {:.2} km)", - obs.name.clone().unwrap_or_else(|| "Unnamed".to_string()), - obs.longitude, - lat, - height - )?; - } - - if let Some(mpc_code_obs) = self.mpc_code_obs.get() { - writeln!(f, "MPC observers:")?; - for (code, obs) in mpc_code_obs.iter() { - let (lat, height) = obs.geodetic_lat_height_wgs84(); - - writeln!( - f, - " {} [{}] (lon: {:.6}°, lat: {:.6}°, elev: {:.2} km)", - obs.name.clone().unwrap_or_else(|| "Unnamed".to_string()), - code, - obs.longitude, - lat, - height - )?; - } - } - - Ok(()) - } -} - -#[cfg(test)] -mod observatories_test { - use super::*; - - #[test] - fn test_observatories() { - let mut observatories = Observatories::new(); - let obs = observatories.create_observer(1.0, 2.0, 3.0, Some("Test".to_string())); - assert_eq!(obs.longitude, 1.0); - assert_eq!(obs.rho_cos_phi, 0.999395371426802); - assert_eq!(obs.rho_sin_phi, 0.0346660237964843); - assert_eq!(obs.name, Some("Test".to_string())); - assert_eq!(observatories.obs_to_uint16.len(), 1); - let observer = observatories.get_observer_from_uint16(0); - assert_eq!(observer.name, Some("Test".to_string())); - - observatories.create_observer(4.0, 5.0, 6.0, Some("Test2".to_string())); - assert_eq!(observatories.obs_to_uint16.len(), 2); - let observer = observatories.get_observer_from_uint16(1); - assert_eq!(observer.name, Some("Test2".to_string())); - } - - #[cfg(test)] - mod observatories_display_tests { - use super::*; - - /// Ensure the "user-defined" section is printed and includes both user observers. - /// - /// Notes - /// ----- - /// * We don't assume any iteration order (HashMap-backed bi-map). - /// * We check for the header and the presence of each observer line fragment. - #[test] - fn display_user_defined_only() { - let mut obs = Observatories::new(); - - // Build two user-defined observers (elevation in kilometers). - obs.create_observer(10.0, 0.0, 0.0, Some("UserA".to_string())); - obs.create_observer(20.0, 45.0, 2.0, Some("UserB".to_string())); - - let s = format!("{obs}"); - - // Header must be present - assert!( - s.starts_with("User-defined observers:\n"), - "Missing 'User-defined observers:' header. Got:\n{s}" - ); - - // Each user observer should be listed with their name and longitude fragment - assert!( - s.contains("UserA (lon: 10.000000°"), - "Missing formatted line for UserA. Got:\n{s}" - ); - assert!( - s.contains("UserB (lon: 20.000000°"), - "Missing formatted line for UserB. Got:\n{s}" - ); - - // The MPC section should not appear if not initialized - assert!( - !s.contains("MPC observers:"), - "Unexpected 'MPC observers:' section when OnceLock is unset. Got:\n{s}" - ); - } - - /// If the MPC table is initialized, ensure the "MPC observers" section appears. - /// - /// Notes - /// ----- - /// * We set the OnceLock with a single entry. - /// * We only check for presence of the section and the MPC code tag. - #[test] - fn display_includes_mpc_section_when_set() { - let mut obs = Observatories::new(); - - // One user-defined observer so the first section is non-empty. - obs.create_observer(0.0, 0.0, 0.0, Some("UserOnly".to_string())); - - // Prepare an MPC observer entry. - let mpc_site = Observer::new( - -156.2575, - 20.7075, - 3.055, - Some("Haleakala".to_string()), - None, - None, - ) - .expect("Failed to create MPC observer"); - - // Build an MpcCodeObs map with a single code. - // If your `MpcCodeObs` is a type alias, this should compile as-is. - // Example: `pub type MpcCodeObs = std::collections::HashMap` (or Arc). - let mut mpc_table: MpcCodeObs = Default::default(); - // Adjust Arc vs Observer depending on your alias: - // If it is `HashMap>`, wrap with `Arc::new(mpc_site)`. - use std::sync::Arc; - mpc_table.insert("I41".to_string(), Arc::new(mpc_site)); - - // Initialize the OnceLock (only once) - obs.mpc_code_obs - .set(mpc_table) - .expect("OnceLock was already initialized"); - - let s = format!("{obs}"); - - // MPC section header must be present now - assert!( - s.contains("MPC observers:"), - "Missing 'MPC observers:' header after setting OnceLock. Got:\n{s}" - ); - - // The code tag should appear in the MPC line - assert!( - s.contains("[I41]"), - "Missing MPC code tag '[I41]' in output. Got:\n{s}" - ); - } - } -} diff --git a/src/outfit.rs b/src/outfit.rs deleted file mode 100644 index cb3aece..0000000 --- a/src/outfit.rs +++ /dev/null @@ -1,676 +0,0 @@ -//! # Outfit: environment, ephemerides, and observatory registry -//! -//! This module defines the [`Outfit`](crate::outfit::Outfit) struct, the central façade that wires together: -//! -//! 1. **Environment state** ([`OutfitEnv`](crate::env_state::OutfitEnv)) — providers and configuration (e.g., UT1). -//! 2. **JPL ephemerides access** — lazy, cached handle over a chosen source -//! ([`EphemFileSource`](crate::jpl_ephem::download_jpl_file::EphemFileSource) → [`JPLEphem`](crate::jpl_ephem::JPLEphem)). -//! 3. **Observatory registry** — MPC Observatory Codes parsed into [`Observer`](crate::observers::Observer) instances, -//! with stable integer IDs for compact indexing and storage. -//! 4. **Astrometric error models** — per-site bias/RMS lookup for RA/DEC accuracies. -//! -//! The design emphasizes *lazy initialization* and *idempotent caching*: -//! - The ephemeris file is opened on first use via [`OnceCell`](once_cell::sync::OnceCell), then reused. -//! - The MPC observatory table is fetched and parsed once, then retained. -//! -//! ## Key responsibilities -//! -//! - Single source of truth for **JPL ephemerides** (HORIZONS/NAIF) through [`get_jpl_ephem`](crate::outfit::Outfit::get_jpl_ephem) -//! - Access to **UT1 provider** for Earth-rotation dependent calculations -//! - **MPC observatory code → Observer** resolution and the inverse (**Observer → u16 index**) -//! - Enrichment of observers with **bias/RMS** angular accuracies from the configured -//! [`ErrorModel`](crate::error_models::ErrorModel) (e.g., *FCCT14*) -//! -//! ## Typical usage -//! -//! ```rust, no_run -//! use outfit::outfit::Outfit; -//! use outfit::error_models::ErrorModel; -//! -//! // Instantiate the context with a JPL source and an error model -//! let outfit = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap(); -//! -//! // On-demand: the ephemeris is opened only once and cached -//! let jpl = outfit.get_jpl_ephem().unwrap(); -//! -//! // Resolve an observer by MPC code -//! let haleakala = outfit.get_observer_from_mpc_code(&"F51".into()); -//! ``` -//! -//! ## Notes -//! -//! - The MPC table is pulled from: -//! `https://www.minorplanetcenter.net/iau/lists/ObsCodes.html` -//! and minimally parsed from its `
` text block.
-//! - Per-site **RA/DEC accuracies** (bias+RMS) are looked up with [`get_bias_rms`](crate::error_models::get_bias_rms),
-//!   currently assuming catalog code `"c"` unless indicated otherwise (TODO).
-//!
-//! ## See also
-//! ------------
-//! * [`JPLEphem`](crate::jpl_ephem::JPLEphem) – Ephemerides access layer.
-//! * [`Observer`](crate::observers::Observer) – Geodetic/parallax observer representation with optional RA/DEC accuracies.
-//! * [`ErrorModel`](crate::error_models::ErrorModel) / [`get_bias_rms`](crate::error_models::get_bias_rms) – Site accuracy enrichment.
-//! * [`OutfitEnv`](crate::env_state::OutfitEnv) – Providers (e.g., UT1) and environment state.
-//! * [`EphemFileSource`](crate::jpl_ephem::download_jpl_file::EphemFileSource) – Source selection for JPL files (HORIZONS/NAIF).
-//!
-//! ## Panics & errors
-//!
-//! - Functions that *must* find an MPC code will `panic!` if the code is unknown.
-//!   Prefer adding a fallible variant if you need graceful handling.
-//! - I/O and parsing failures are surfaced as [`OutfitError`](crate::outfit_errors::OutfitError) where applicable.
-
-use std::{collections::HashMap, fmt, sync::Arc};
-
-use nalgebra::Matrix3;
-use once_cell::sync::OnceCell;
-
-use crate::{
-    constants::{Degree, Kilometer, MpcCode, MpcCodeObs},
-    env_state::OutfitEnv,
-    error_models::{get_bias_rms, ErrorModel, ErrorModelData},
-    jpl_ephem::download_jpl_file::EphemFileSource,
-    observers::{observatories::Observatories, Observer},
-    outfit_errors::OutfitError,
-    ref_system::{rotpn, RefEpoch, RefSystem},
-};
-
-use crate::jpl_ephem::JPLEphem;
-
-#[derive(Debug, Clone)]
-pub struct Outfit {
-    env_state: OutfitEnv,
-    observatories: Observatories,
-    jpl_source: EphemFileSource,
-    jpl_ephem: OnceCell,
-    pub error_model: ErrorModel,
-    error_model_data: ErrorModelData,
-    rot_equmj2000_to_eclmj2000: Matrix3,
-    rot_eclmj2000_to_equmj2000: Matrix3,
-}
-
-impl Outfit {
-    /// Construct a new [`Outfit`] context.
-    ///
-    /// Initializes the environment, sets the JPL ephemerides source, and loads the configured
-    /// error model from disk. The ephemeris file itself is **not** opened yet; it is lazily
-    /// initialized the first time [`get_jpl_ephem`](crate::outfit::Outfit::get_jpl_ephem) is called.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `jpl_file`: A source descriptor resolvable into an [`EphemFileSource`]
-    ///   (e.g., `"horizon:DE440"` or a NAIF path).
-    /// * `error_model`: The site accuracy model to load (e.g., [`ErrorModel::FCCT14`]).
-    ///
-    /// Return
-    /// ----------
-    /// * A new [`Outfit`] instance or an [`OutfitError`] if the error model cannot be read.
-    ///
-    /// See also
-    /// ------------
-    /// * [`get_jpl_ephem`](crate::outfit::Outfit::get_jpl_ephem) – Lazy initialization and access to the ephemeris handle.
-    /// * [`ErrorModel::read_error_model_file`](crate::error_models::ErrorModel::read_error_model_file) – Underlying loader for the model data.
-    pub fn new(jpl_file: &str, error_model: ErrorModel) -> Result {
-        let rot1 = rotpn(
-            &RefSystem::Equm(RefEpoch::J2000),
-            &RefSystem::Eclm(RefEpoch::J2000),
-        )?;
-
-        let rot2 = rotpn(
-            &RefSystem::Eclm(RefEpoch::J2000),
-            &RefSystem::Equm(RefEpoch::J2000),
-        )?;
-
-        Ok(Outfit {
-            env_state: OutfitEnv::new(),
-            observatories: Observatories::new(),
-            jpl_source: jpl_file.try_into()?,
-            jpl_ephem: OnceCell::new(),
-            error_model,
-            error_model_data: error_model.read_error_model_file()?,
-            rot_equmj2000_to_eclmj2000: rot1,
-            rot_eclmj2000_to_equmj2000: rot2,
-        })
-    }
-
-    /// Get the rotation matrix from equatorial J2000 to ecliptic J2000.
-    /// This matrix is used to transform coordinates from the equatorial frame to the ecliptic frame.
-    pub fn get_rot_equmj2000_to_eclmj2000(&self) -> &Matrix3 {
-        &self.rot_equmj2000_to_eclmj2000
-    }
-
-    pub fn get_rot_eclmj2000_to_equmj2000(&self) -> &Matrix3 {
-        &self.rot_eclmj2000_to_equmj2000
-    }
-
-    /// Get the lazily-initialized JPL ephemerides handle.
-    ///
-    /// If this is the first call, the ephemeris is opened and cached in an internal [`OnceCell`].
-    /// Subsequent calls return the same reference.
-    ///
-    /// Arguments
-    /// -----------------
-    /// *None*
-    ///
-    /// Return
-    /// ----------
-    /// * `&JPLEphem` on success, or an [`OutfitError`] if the source cannot be opened.
-    ///
-    /// See also
-    /// ------------
-    /// * [`EphemFileSource`] – Source configuration.
-    /// * [`OnceCell::get_or_try_init`] – Lazy initialization helper.
-    pub fn get_jpl_ephem(&self) -> Result<&JPLEphem, OutfitError> {
-        self.jpl_ephem
-            .get_or_try_init(|| JPLEphem::new(&self.jpl_source))
-    }
-
-    /// Access the UT1 provider from the environment.
-    ///
-    /// This is useful for Earth-rotation dependent calculations (e.g., GMST, sidereal time).
-    ///
-    /// Arguments
-    /// -----------------
-    /// *None*
-    ///
-    /// Return
-    /// ----------
-    /// * A reference to the [`hifitime::ut1::Ut1Provider`].
-    ///
-    /// See also
-    /// ------------
-    /// * [`OutfitEnv`] – Environment state and providers.
-    pub fn get_ut1_provider(&self) -> &hifitime::ut1::Ut1Provider {
-        &self.env_state.ut1_provider
-    }
-
-    /// Get the lazily built MPC observatory map (MPC code → [`Observer`]).
-    ///
-    /// The map is fetched and parsed from the MPC HTML table on first use, then cached.
-    ///
-    /// Return
-    /// ----------
-    /// * A reference to the shared map: [`MpcCodeObs`] = `HashMap>`.
-    ///
-    /// See also
-    /// ------------
-    /// * [`init_observatories`](crate::outfit::Outfit::init_observatories) – Builder invoked on first access.
-    /// * [`get_observer_from_mpc_code`](crate::outfit::Outfit::get_observer_from_mpc_code) – Convenience accessor for one site.
-    pub(crate) fn get_observatories(&self) -> &MpcCodeObs {
-        self.observatories
-            .mpc_code_obs
-            .get_or_init(|| self.init_observatories())
-    }
-
-    /// Resolve an [`Observer`] from a given MPC observatory code.
-    ///
-    /// This accessor panics if the code is unknown. Use it when unknown codes are exceptional.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `mpc_code`: The MPC observatory code (e.g., `"F51"`).
-    ///
-    /// Return
-    /// ----------
-    /// * An `Arc` for the requested site.
-    pub fn get_observer_from_mpc_code(&self, mpc_code: &MpcCode) -> Arc {
-        self.get_observatories()
-            .get(mpc_code)
-            .unwrap_or_else(|| panic!("MPC code not found: {mpc_code}"))
-            .clone()
-    }
-
-    /// Build the MPC observatory registry by fetching and parsing the MPC list.
-    ///
-    /// For each row, the routine extracts:
-    /// - Longitude (deg), ρ·cosφ, ρ·sinφ (parallax factors),
-    /// - Human-readable name,
-    /// - Optional RA/DEC accuracies derived from the loaded [`ErrorModelData`]
-    ///   via [`get_bias_rms`] (currently using catalog code `"c"`, TODO).
-    ///
-    /// Return
-    /// ----------
-    /// * A freshly constructed [`MpcCodeObs`] map.
-    ///
-    /// See also
-    /// ------------
-    /// * [`get_observatories`](crate::outfit::Outfit::get_observatories) – Lazy wrapper that caches this map.
-    /// * [`get_bias_rms`] – Site accuracy lookup by (mpc_code, catalog_code).
-    pub(crate) fn init_observatories(&self) -> MpcCodeObs {
-        let mut observatories: MpcCodeObs = HashMap::new();
-
-        let mpc_code_response = self
-            .env_state
-            .get_from_url("https://www.minorplanetcenter.net/iau/lists/ObsCodes.html");
-
-        let mpc_code_csv = mpc_code_response
-            .trim()
-            .strip_prefix("
")
-            .and_then(|s| s.strip_suffix("
"))
-            .expect("Failed to strip pre tags");
-
-        for lines in mpc_code_csv.lines().skip(2) {
-            let line = lines.trim();
-
-            if let Some((code, remain)) = line.split_at_checked(3) {
-                let remain = remain.trim_end();
-
-                let (longitude, cos, sin, name) = parse_remain(remain, code);
-
-                // TODO: support per-site catalog codes (not always "c")
-                let bias_rms =
-                    get_bias_rms(&self.error_model_data, code.to_string(), "c".to_string());
-
-                let observer = Observer::from_parallax(
-                    longitude as f64,
-                    cos as f64,
-                    sin as f64,
-                    Some(name),
-                    bias_rms.map(|(ra, _)| ra as f64),
-                    bias_rms.map(|(_, dec)| dec as f64),
-                )
-                .expect("Failed to create observer");
-                observatories.insert(code.to_string(), Arc::new(observer));
-            };
-        }
-        observatories
-    }
-
-    /// Convert an MPC code to its stable 16-bit observatory index.
-    ///
-    /// Useful for compact storage of observer references in catalogs, measurements,
-    /// and ephemeris products.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `mpc_code`: The MPC observatory code.
-    ///
-    /// Return
-    /// ----------
-    /// * The `u16` index associated with the given observer.
-    ///
-    /// See also
-    /// ------------
-    /// * [`get_observer_from_mpc_code`](crate::outfit::Outfit::get_observer_from_mpc_code) – Resolve the observer first (panic on unknown).
-    /// * [`uint16_from_observer`](crate::outfit::Outfit::uint16_from_observer) – Indexing for arbitrary/new observers.
-    pub(crate) fn uint16_from_mpc_code(&mut self, mpc_code: &MpcCode) -> u16 {
-        let observer = self.get_observer_from_mpc_code(mpc_code);
-        self.observatories.uint16_from_observer(observer)
-    }
-
-    /// Convert an [`Observer`] handle to its stable 16-bit index.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `observer`: The observer to be indexed.
-    ///
-    /// Return
-    /// ----------
-    /// * The `u16` index associated with this observer (inserting if new).
-    ///
-    /// See also
-    /// ------------
-    /// * [`get_observer_from_uint16`](crate::outfit::Outfit::get_observer_from_uint16) – Recover a reference from an index.
-    /// * [`new_observer`](crate::outfit::Outfit::new_observer) – Create and register a new custom observer.
-    pub(crate) fn uint16_from_observer(&mut self, observer: Arc) -> u16 {
-        self.observatories.uint16_from_observer(observer)
-    }
-
-    /// Recover an [`Observer`] reference from a 16-bit index.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `observer_idx`: The previously assigned index.
-    ///
-    /// Return
-    /// ----------
-    /// * A reference to the corresponding [`Observer`].
-    ///
-    /// See also
-    /// ------------
-    /// * [`uint16_from_observer`](crate::outfit::Outfit::uint16_from_observer) – Assign/lookup indices.
-    /// * [`get_observer_from_mpc_code`](crate::outfit::Outfit::get_observer_from_mpc_code) – Resolve by MPC code instead.
-    pub(crate) fn get_observer_from_uint16(&self, observer_idx: u16) -> &Observer {
-        self.observatories.get_observer_from_uint16(observer_idx)
-    }
-
-    /// Create and register a new **custom** observer.
-    ///
-    /// This helper converts geodetic inputs to the internal parallax representation
-    /// (ρ·cosφ, ρ·sinφ) and stores the new [`Observer`] with an optional display name.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `longitude`: Geodetic longitude in **degrees** (east-positive).
-    /// * `latitude`:  Geodetic latitude in **degrees**.
-    /// * `elevation`: Elevation in **kilometers** above the ellipsoid/geoid (model-dependent).
-    /// * `name`:      Optional human-readable name for the site.
-    ///
-    /// Return
-    /// ----------
-    /// * An `Arc` handle to the newly created observer.
-    pub fn new_observer(
-        &mut self,
-        longitude: Degree,
-        latitude: Degree,
-        elevation: Kilometer,
-        name: Option,
-    ) -> Arc {
-        self.observatories
-            .create_observer(longitude, latitude, elevation, name)
-    }
-
-    pub(crate) fn add_observer_internal(&mut self, observer: Arc) -> u16 {
-        self.observatories.add_observer(observer)
-    }
-
-    pub fn add_observer(&mut self, observer: Arc) {
-        self.add_observer_internal(observer);
-    }
-
-    /// Render the current observatories into a newly allocated `String`.
-    ///
-    /// This is a convenience wrapper around the `Display` implementation of
-    /// the internal struct \[`Observatories`\]. It materializes the formatted list (user-defined
-    /// observers first, then MPC sites if available) into a `String`.
-    ///
-    /// Output format
-    /// -------------
-    /// * Longitude and latitude are shown in **degrees**.
-    /// * Elevation is shown in **kilometers**.
-    /// * User-defined observers are listed first; if initialized, the
-    ///   **MPC observers** section follows.
-    /// * The relative order within each section is not guaranteed to be stable.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * None.
-    ///
-    /// Return
-    /// ----------
-    /// * A `String` containing the formatted observatories.
-    ///
-    /// See also
-    /// ------------
-    /// * [`Outfit::show_observatories`] – Allocation-free display adaptor.
-    /// * [`Observer::geodetic_lat_height_wgs84`] – Provides latitude/height used in the listing.
-    #[inline]
-    pub fn show_observatories_string(&self) -> String {
-        self.observatories.to_string()
-    }
-
-    /// Pretty-print the current set of observatories without allocating a `String`.
-    ///
-    /// Returns a lightweight `Display` adaptor over the internal \[`Observatories`\]
-    /// collection. Use with `format!`, `println!`, log macros, or any consumer of
-    /// `fmt::Display`. User-defined observers are printed first, followed by the
-    /// **MPC observers** section if the MPC table has been initialized.
-    ///
-    /// Output format
-    /// -------------
-    /// * Longitude and latitude are shown in **degrees**.
-    /// * Elevation is shown in **kilometers**.
-    /// * The relative order within each section is not guaranteed to be stable.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * None.
-    ///
-    /// Return
-    /// ----------
-    /// * An [`ObservatoriesView`] display adaptor (zero-copy) suitable for `fmt::Display`.
-    ///
-    /// See also
-    /// ------------
-    /// * [`Outfit::show_observatories_string`] – Eager, allocated `String`.
-    /// * [`Observer::geodetic_lat_height_wgs84`] – Provides latitude/height used in the listing.
-    #[inline]
-    pub fn show_observatories(&self) -> ObservatoriesView<'_> {
-        ObservatoriesView(&self.observatories)
-    }
-}
-
-/// Lightweight, zero-allocation display adaptor for the internal private struct \[`Observatories`\].
-///
-/// This type borrows the internal \[`Observatories`\] and implements `fmt::Display`,
-/// allowing you to pretty-print the full list of observers without allocating an
-/// intermediate `String`. It simply delegates to the `Display` implementation
-/// of \[`Observatories`\].
-///
-/// Output format
-/// -------------
-/// * User-defined observers are listed first.
-/// * If initialized, an **MPC observers** section follows.
-/// * Longitudes/latitudes are shown in **degrees**; elevation is shown in **kilometers**.
-/// * Relative order within each section is not guaranteed to be stable (hash-map backed).
-///
-/// Example
-/// -----------------
-/// ```rust, no_run
-/// # use outfit::outfit::Outfit;
-/// # use outfit::error_models::ErrorModel;
-/// let outfit = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
-/// // Print to stdout without allocating a String:
-/// println!("{}", outfit.show_observatories());
-/// // Or, if you need a String, use:
-/// let s = outfit.show_observatories_string();
-/// assert!(s.contains("User-defined observers:"));
-/// ```
-///
-/// Arguments
-/// -----------------
-/// * None (constructed by [`Outfit::show_observatories`]).
-///
-/// Return
-/// ----------
-/// * A display adaptor suitable for `format!`, `println!`, and any `fmt::Display` consumer.
-///
-/// See also
-/// ------------
-/// * [`Outfit::show_observatories`] – Returns this adaptor.
-/// * [`Outfit::show_observatories_string`] – Allocating `String` convenience.
-/// * [`Observer::geodetic_lat_height_wgs84`] – Provides latitude/height used in the listing.
-pub struct ObservatoriesView<'a>(&'a Observatories);
-
-impl<'a> fmt::Display for ObservatoriesView<'a> {
-    fn fmt(&self, f: &mut fmt::Formatter<'_>) -> fmt::Result {
-        // Delegate to Observatories' Display without allocating
-        write!(f, "{}", self.0)
-    }
-}
-
-/// Parse a fixed-width float slice from an MPC observatory line.
-///
-/// Arguments
-/// -----------------
-/// * `s`:    Full line (trailing part after the 3-char MPC code).
-/// * `slice`: Byte range selecting the numeric field.
-/// * `code`:  MPC code (for diagnostics).
-///
-/// Return
-/// ----------
-/// * `Ok(f32)` parsed value, or the parsing error.
-///
-/// See also
-/// ------------
-/// * [`parse_remain`] – Higher-level field extraction for one line.
-fn parse_f32(
-    s: &str,
-    slice: std::ops::Range,
-    code: &str,
-) -> Result {
-    s.get(slice)
-        .unwrap_or_else(|| panic!("Failed to parse float for observer code: {code}"))
-        .trim()
-        .parse()
-}
-
-/// Extract longitude, ρ·cosφ, ρ·sinφ, and name from a fixed-width MPC row.
-///
-/// This helper returns partial values (with zeros) if any field fails to parse,
-/// allowing the caller to still record the site name while signaling missing data
-/// implicitly through zeros.
-///
-/// Arguments
-/// -----------------
-/// * `remain`: Fixed-width tail of the line (after the 3-char MPC code).
-/// * `code`:   MPC code (for diagnostics).
-///
-/// Return
-/// ----------
-/// * `(longitude_deg, rho_cos_phi, rho_sin_phi, name)`
-fn parse_remain(remain: &str, code: &str) -> (f32, f32, f32, String) {
-    let name = remain
-        .get(27..)
-        .unwrap_or_else(|| panic!("Failed to parse name value for code: {code}"));
-
-    let Some(longitude) = parse_f32(remain, 1..10, code).ok() else {
-        return (0.0, 0.0, 0.0, name.to_string());
-    };
-
-    let Some(cos) = parse_f32(remain, 10..18, code).ok() else {
-        return (longitude, 0.0, 0.0, name.to_string());
-    };
-
-    let Some(sin) = parse_f32(remain, 18..27, code).ok() else {
-        return (longitude, cos, 0.0, name.to_string());
-    };
-    (longitude, cos, sin, name.to_string())
-}
-
-#[cfg(test)]
-mod outfit_show_observatories_tests {
-    use super::*;
-    use std::sync::Arc;
-
-    /// Build a lightweight Outfit for display tests, then add zero or more user observers.
-    ///
-    /// Notes
-    /// -----
-    /// * Uses the public `Outfit::new(...)` constructor to avoid touching private internals.
-    /// * If your `Outfit::new` signature changes, adjust here accordingly.
-    fn build_outfit_with_users(users: &[(&str, f64, f64, f64)]) -> Outfit {
-        // Pick a reasonable default error model; adjust if your API differs.
-        let mut outfit = Outfit::new("horizon:DE440", crate::error_models::ErrorModel::FCCT14)
-            .expect("Failed to construct Outfit for display tests");
-
-        for (name, lon_deg, lat_deg, elev_km) in users.iter().copied() {
-            let obs = Observer::new(
-                lon_deg,
-                lat_deg,
-                elev_km,
-                Some(name.to_string()),
-                None,
-                None,
-            )
-            .expect("Failed to create user observer");
-            // If your API differs, replace with the appropriate method to register observers:
-            outfit.add_observer(Arc::new(obs));
-        }
-        outfit
-    }
-
-    /// Ensure the string rendering equals the Display adaptor output when there are no observers.
-    #[test]
-    fn show_observatories_empty() {
-        let outfit = build_outfit_with_users(&[]);
-
-        let s_string = outfit.show_observatories_string();
-        let s_view = format!("{}", outfit.show_observatories());
-
-        assert_eq!(
-            s_string, s_view,
-            "String output and Display adaptor should match"
-        );
-        assert!(
-            s_string.starts_with("No observatories defined (user or MPC)."),
-            "Missing 'User-defined observers:' header. Got:\n{s_string}"
-        );
-        assert!(
-            !s_string.contains("MPC observers:"),
-            "Should not show 'MPC observers:' when OnceLock is unset. Got:\n{s_string}"
-        );
-    }
-
-    /// After adding user-defined observers, they should appear in the output.
-    #[test]
-    fn show_observatories_with_users() {
-        let outfit = build_outfit_with_users(&[
-            ("UserA", 10.0, 0.0, 0.0),
-            ("UserB", 20.0, 45.0, 2.0), // 2 km elevation
-        ]);
-
-        let s_string = outfit.show_observatories_string();
-        let s_view = format!("{}", outfit.show_observatories());
-
-        assert_eq!(
-            s_string, s_view,
-            "String output and Display adaptor should match"
-        );
-
-        // Headers and user names should be present
-        assert!(
-            s_string.starts_with("User-defined observers:\n"),
-            "Missing 'User-defined observers:' header. Got:\n{s_string}"
-        );
-        assert!(
-            s_string.contains("UserA (lon: 10.000000°"),
-            "Missing formatted line for UserA. Got:\n{s_string}"
-        );
-        assert!(
-            s_string.contains("UserB (lon: 20.000000°"),
-            "Missing formatted line for UserB. Got:\n{s_string}"
-        );
-    }
-
-    /// If the MPC table is initialized, the MPC section should appear.
-    ///
-    /// Notes
-    /// -----
-    /// * This test accesses the OnceLock inside `observatories` to inject a minimal MPC table.
-    /// * If your `MpcCodeObs` stores `Arc` instead of `Observer`, wrap with `Arc::new`.
-    #[test]
-    fn show_observatories_with_mpc_section() {
-        let outfit = build_outfit_with_users(&[("UserOnly", 0.0, 0.0, 0.0)]);
-
-        // Build a minimal MPC table with one entry
-        let mpc_site = Observer::new(
-            -156.2575,
-            20.7075,
-            3.055,
-            Some("Haleakala".to_string()),
-            None,
-            None,
-        )
-        .expect("Failed to create MPC observer");
-
-        // If MpcCodeObs = HashMap>, wrap with Arc::new.
-        // If it is HashMap, remove Arc::new below.
-        let mut mpc_table: crate::constants::MpcCodeObs = Default::default();
-        // Uncomment ONE of the two lines below depending on your alias:
-        // mpc_table.insert("I41".to_string(), mpc_site);                 // if value is Observer
-        mpc_table.insert("I41".to_string(), Arc::new(mpc_site)); // if value is Arc
-
-        // Initialize the OnceLock
-        outfit
-            .observatories
-            .mpc_code_obs
-            .set(mpc_table)
-            .expect("OnceLock already initialized");
-
-        let s_string = outfit.show_observatories_string();
-        let s_view = format!("{}", outfit.show_observatories());
-
-        assert_eq!(
-            s_string, s_view,
-            "String output and Display adaptor should match"
-        );
-        assert!(
-            s_string.contains("MPC observers:"),
-            "Missing 'MPC observers:' header after setting OnceLock. Got:\n{s_string}"
-        );
-        assert!(
-            s_string.contains("[I41]"),
-            "Missing MPC code tag '[I41]' in output. Got:\n{s_string}"
-        );
-    }
-}
diff --git a/src/outfit_errors.rs b/src/outfit_errors.rs
index a86ae10..c78e691 100644
--- a/src/outfit_errors.rs
+++ b/src/outfit_errors.rs
@@ -135,8 +135,10 @@
 //! * [`ParseObsError`](crate::trajectories::mpc_80col_reader::ParseObsError) – observation parsing errors.
 //! * [`roots::SearchError`] – wrapped in [`RootFindingError`](crate::outfit_errors::OutfitError::RootFindingError).
 //! * [`rand_distr::NormalError`] – wrapped in [`NoiseInjectionError`](crate::outfit_errors::OutfitError::NoiseInjectionError).
-
-use crate::trajectories::mpc_80col_reader::ParseObsError;
+use photom::{
+    observation_dataset::{ObsDatasetError, ObsId},
+    TrajId,
+};
 use thiserror::Error;
 
 #[derive(Error, Debug)]
@@ -159,7 +161,6 @@ pub enum OutfitError {
     #[error("Filesystem I/O error: {0}")]
     IoError(#[from] std::io::Error),
 
-    #[cfg(feature = "jpl-download")]
     #[error("HTTP request failed (reqwest): {0}")]
     ReqwestError(#[from] reqwest::Error),
 
@@ -187,9 +188,6 @@ pub enum OutfitError {
     #[error("Parsing error (nom): {0}")]
     NomParsingError(String),
 
-    #[error("Parsing error in 80-column observation file: {0}")]
-    Parsing80ColumnFileError(ParseObsError),
-
     #[error("Gaussian noise generation failed: {0:?}")]
     NoiseInjectionError(rand_distr::NormalError),
 
@@ -253,6 +251,24 @@ pub enum OutfitError {
 
     #[error("Non-finite score encountered: {0}")]
     NonFiniteScore(f64),
+
+    #[error("The provided observation {0} has no associated observer (ObserverId is None)")]
+    ObserverIdIsNone(ObsId),
+
+    #[error(transparent)]
+    ObsDatasetError(#[from] ObsDatasetError),
+
+    #[error("Observer dataset error: {0}")]
+    ObsDatasetErrorRef(String),
+
+    #[error("Trajectory ID not found in dataset: {0}")]
+    TrajectoryIdNotFound(TrajId),
+}
+
+impl From<&ObsDatasetError> for OutfitError {
+    fn from(e: &ObsDatasetError) -> Self {
+        OutfitError::ObsDatasetErrorRef(e.to_string())
+    }
 }
 
 impl From for OutfitError {
@@ -279,7 +295,6 @@ impl PartialEq for OutfitError {
             // Opaque external error kinds compare equal by variant only
             (UreqHttpError(_), UreqHttpError(_)) => true,
             (IoError(_), IoError(_)) => true,
-            #[cfg(feature = "jpl-download")]
             (ReqwestError(_), ReqwestError(_)) => true,
             (Parquet(_), Parquet(_)) => true,
 
@@ -291,7 +306,6 @@ impl PartialEq for OutfitError {
             (InvalidErrorModel(a), InvalidErrorModel(b)) => a == b,
             (InvalidErrorModelFilePath(a), InvalidErrorModelFilePath(b)) => a == b,
             (NomParsingError(a), NomParsingError(b)) => a == b,
-            (Parsing80ColumnFileError(a), Parsing80ColumnFileError(b)) => a == b,
             (NoiseInjectionError(a), NoiseInjectionError(b)) => a == b,
             (InvalidSpkDataType(a), InvalidSpkDataType(b)) => a == b,
             (InvalidIODParameter(a), InvalidIODParameter(b)) => a == b,
diff --git a/src/trajectories/ades_reader.rs b/src/trajectories/ades_reader.rs
deleted file mode 100644
index c89c5a2..0000000
--- a/src/trajectories/ades_reader.rs
+++ /dev/null
@@ -1,257 +0,0 @@
-use std::str::FromStr;
-
-use camino::Utf8Path;
-use hifitime::Epoch;
-use quick_xml::de::from_str;
-use serde::{Deserialize, Deserializer};
-use smallvec::SmallVec;
-
-use crate::{
-    constants::{ArcSec, ObjectNumber},
-    outfit::Outfit,
-    TrajectorySet,
-};
-
-use crate::observations::Observation;
-
-#[derive(Debug, Deserialize)]
-struct StructuredAdes {
-    #[serde(rename = "obsBlock")]
-    obs_blocks: Vec,
-}
-
-#[derive(Debug, Deserialize)]
-struct FlatAdes {
-    #[serde(rename = "optical")]
-    opticals: Vec,
-}
-
-#[derive(Debug, Deserialize)]
-struct ObsBlock {
-    #[serde(rename = "obsContext")]
-    obs_context: ObsContext,
-
-    #[serde(rename = "obsData")]
-    obs_data: ObsData,
-}
-
-#[derive(Debug, Deserialize)]
-struct ObsContext {
-    observatory: Observatory,
-}
-
-#[derive(Debug, Deserialize)]
-struct Observatory {
-    #[serde(rename = "mpcCode")]
-    mpc_code: String,
-}
-
-#[derive(Debug, Deserialize)]
-struct ObsData {
-    #[serde(rename = "optical")]
-    opticals: Vec,
-}
-
-#[derive(Debug, Deserialize)]
-struct OpticalObs {
-    #[serde(rename = "permID")]
-    perm_id: Option,
-    #[serde(rename = "provID")]
-    prov_id: Option,
-    #[serde(rename = "trkSub")]
-    trk_sub: Option,
-
-    #[serde(rename = "obsTime", deserialize_with = "deserialize_mjd")]
-    obs_time: f64,
-
-    ra: f64,
-    dec: f64,
-
-    #[serde(rename = "precRA")]
-    prec_ra: Option,
-    #[serde(rename = "precDec")]
-    prec_dec: Option,
-
-    #[serde(rename = "rmsRA")]
-    rms_ra: Option,
-    #[serde(rename = "rmsDec")]
-    rms_dec: Option,
-
-    stn: String,
-}
-
-impl OpticalObs {
-    /// Returns the trajectory ID for the optical observation.
-    /// It first checks for a `perm_id`, then a `prov_id`, and finally falls back to `trk_sub`.
-    /// If none of these are available, it panics with an error message.
-    /// The ID is parsed as a `u32` if possible, otherwise it is returned as a string.
-    ///
-    /// Return
-    /// ------
-    /// * An `ObjectNumber` representing the trajectory ID.
-    /// * If the ID is a valid `u32`, it is returned as `ObjectNumber::Int(id)`.
-    /// * If the ID is not a valid `u32`, it is returned as `ObjectNumber::String(id)`.
-    /// * If no ID is found, it panics with an error message.
-    fn get_id(&self) -> ObjectNumber {
-        let id = self
-            .perm_id
-            .clone()
-            .or_else(|| self.prov_id.clone())
-            .unwrap_or_else(|| self.trk_sub.clone().expect("No ID found"));
-        if let Ok(id) = id.parse::() {
-            ObjectNumber::Int(id)
-        } else {
-            ObjectNumber::String(id)
-        }
-    }
-
-    fn to_observation(
-        &self,
-        state: &Outfit,
-        observer_idx: u16,
-        error_ra: Option,
-        error_dec: Option,
-    ) -> Observation {
-        let error_ra = self.rms_ra.unwrap_or_else(|| {
-            self.prec_ra
-                .unwrap_or_else(|| error_ra.expect("No error for RA when parsing ADES file"))
-        });
-
-        let error_dec = self.rms_dec.unwrap_or_else(|| {
-            self.prec_dec
-                .unwrap_or_else(|| error_dec.expect("No error for Dec when parsing ADES file"))
-        });
-        Observation::new(
-            state,
-            observer_idx,
-            self.ra,
-            error_ra,
-            self.dec,
-            error_dec,
-            self.obs_time,
-        )
-        .expect("Failed to create observation from ADES")
-    }
-}
-
-/// Deserialize a date string in the format "YYYY-MM-DDTHH:MM:SS" into a floating-point number
-/// representing the Modified Julian Date (MJD).
-/// The date string is expected to be in UTC.
-///
-/// Arguments
-/// ---------
-/// * `deserializer`: The deserializer to use for the date string.
-///
-/// Return
-/// ------
-/// * A `Result` containing the parsed MJD as a `f64` or an error if the parsing fails.
-fn deserialize_mjd<'de, D>(deserializer: D) -> Result
-where
-    D: Deserializer<'de>,
-{
-    let date_str = String::deserialize(deserializer)?;
-
-    let time = Epoch::from_str(&date_str).map_err(serde::de::Error::custom)?;
-
-    Ok(time.to_mjd_utc_days())
-}
-
-/// Parses a `FlatAdes` file and populates the given `Outfit` and `TrajectorySet`.
-/// It iterates through the optical observations, extracting the observer's MPC code and
-/// creating an `Observation` for each optical observation.
-/// The observations are then added to the `TrajectorySet` using the trajectory ID.
-/// If a new observatory is found, it is added to the `Outfit` observatory set.
-///
-/// Arguments
-/// ---------
-/// * `outfit`: A mutable reference to the `Outfit` instance.
-/// * `flat_ades`: A reference to the `FlatAdes` instance.
-/// * `trajs`: A mutable reference to the `TrajectorySet` instance.
-fn parse_flat_ades(
-    outfit: &mut Outfit,
-    flat_ades: &FlatAdes,
-    trajs: &mut TrajectorySet,
-    error_ra: Option,
-    error_dec: Option,
-) {
-    for optical in &flat_ades.opticals {
-        let traj_id = optical.get_id();
-        let observer = outfit.uint16_from_mpc_code(&optical.stn);
-        let observation = optical.to_observation(outfit, observer, error_ra, error_dec);
-        trajs
-            .entry(traj_id)
-            .or_insert_with(|| SmallVec::with_capacity(10))
-            .push(observation);
-    }
-}
-
-/// Parses a `StructuredAdes` file and populates the given `Outfit` and `TrajectorySet`.
-/// It iterates through the observation blocks, extracting the observer's MPC code and
-/// creating an `Observation` for each optical observation.
-/// The observations are then added to the `TrajectorySet` using the trajectory ID.
-/// If a new observatory is found, it is added to the `Outfit` observatory set.
-///
-/// Arguments
-/// ---------
-/// * `outfit`: A mutable reference to the `Outfit` instance.
-/// * `structured_ades`: A reference to the `StructuredAdes` instance.
-/// * `trajs`: A mutable reference to the `TrajectorySet` instance.
-fn parse_structured_ades(
-    outfit: &mut Outfit,
-    structured_ades: &StructuredAdes,
-    trajs: &mut TrajectorySet,
-    error_ra: Option,
-    error_dec: Option,
-) {
-    for obs_block in &structured_ades.obs_blocks {
-        let obs_context = &obs_block.obs_context;
-        let mpc_code = &obs_context.observatory.mpc_code;
-        let observer = outfit.uint16_from_mpc_code(mpc_code);
-
-        for optical in &obs_block.obs_data.opticals {
-            let observation = optical.to_observation(outfit, observer, error_ra, error_dec);
-            let traj_id = optical.get_id();
-            trajs
-                .entry(traj_id)
-                .or_insert_with(|| SmallVec::with_capacity(10))
-                .push(observation);
-        }
-    }
-}
-
-/// Parses an ADES file and populates the given `Outfit` and `TrajectorySet`.
-/// It first attempts to parse the file as a `FlatAdes`, and if that fails, it tries to parse it as a `StructuredAdes`.
-/// If both parsing attempts fail, it panics with an error message.
-/// If new observatory are found, they are added to the `Outfit` observatory set.
-///
-/// Arguments
-/// ---------
-/// * `outfit`: A mutable reference to the `Outfit` instance.
-/// * `ades`: A reference to the ADES file path.
-/// * `trajs`: A mutable reference to the `TrajectorySet` instance.
-pub(crate) fn parse_ades(
-    outfit: &mut Outfit,
-    ades: &Utf8Path,
-    trajs: &mut TrajectorySet,
-    error_ra: Option,
-    error_dec: Option,
-) {
-    let xml = std::fs::read_to_string(ades)
-        .unwrap_or_else(|_| panic!("Failed to read ADES file: {ades}"));
-
-    match from_str::(&xml) {
-        Ok(flat_ades) => {
-            parse_flat_ades(outfit, &flat_ades, trajs, error_ra, error_dec);
-        }
-        Err(flat_err) => match from_str::(&xml) {
-            Ok(structured_ades) => {
-                parse_structured_ades(outfit, &structured_ades, trajs, error_ra, error_dec);
-            }
-            Err(structured_err) => {
-                panic!(
-                    "Failed to parse ADES file:\n- Flat error: {flat_err}\n- Structured error: {structured_err}"
-                );
-            }
-        },
-    }
-}
diff --git a/src/trajectories/batch_reader.rs b/src/trajectories/batch_reader.rs
deleted file mode 100644
index 1d7021a..0000000
--- a/src/trajectories/batch_reader.rs
+++ /dev/null
@@ -1,432 +0,0 @@
-//! # Single-Observer Astrometric Batch Ingestion
-//!
-//! This module provides the [`ObservationBatch`] type, which groups multiple
-//! astrometric detections from a **single observer** into a compact container.
-//! Such a batch can then be expanded into concrete [`Observation`]s and stored
-//! in a [`TrajectorySet`].
-//!
-//! ## Overview
-//! -----------------
-//! A wide-field survey typically delivers angle-only astrometry (RA/DEC, with
-//! per-epoch timestamps). [`ObservationBatch`] wraps such measurements, together
-//! with uniform error estimates, into a structured form ready for ingestion into
-//! orbit-determination pipelines.
-//!
-//! To actually turn batches into stored observations, use the trait
-//! [`TrajectoryFile`](crate::trajectories::trajectory_file::TrajectoryFile):
-//! - [`TrajectoryFile::new_from_vec`](crate::trajectories::trajectory_file::TrajectoryFile::new_from_vec) — build a new [`TrajectorySet`] from a batch.
-//! - [`TrajectoryFile::add_from_vec`](crate::trajectories::trajectory_file::TrajectoryFile::add_from_vec) — append a batch into an existing [`TrajectorySet`].
-//!
-//! Both methods transparently handle the internal expansion of a batch into
-//! per-sample [`Observation`]s (site position lookups, heliocentric positions,
-//! RA/DEC/error propagation, etc.).
-//!
-//! ## Units & Conventions
-//! -----------------
-//! - **Angles:** Right ascension and declination in **radians**.  
-//!   If your upstream data are in **degrees/arcseconds**, use
-//!   [`ObservationBatch::from_degrees_owned`] to convert once at construction.
-//! - **Uncertainties:** 1-σ errors in RA/DEC (radians). For arcsecond inputs,
-//!   the degree-based constructor performs the conversion for you.
-//! - **Epochs:** Times in **MJD (TT)** (days). Convert UTC/TAI upstream.
-//! - **Observer:** All rows in a batch must come from the **same** observer.
-//!
-//! ## Invariants
-//! -----------------
-//! - `trajectory_id.len() == ra.len() == dec.len() == time.len()`  
-//! - All angles and uncertainties are in **radians**.  
-//! - All epochs are in **MJD (TT)**.  
-//! - Batch content belongs to a **single observer**.
-//!
-//! ## Construction Paths
-//! -----------------
-//! - [`ObservationBatch::from_radians_borrowed`] — zero-copy when your pipeline already
-//!   provides radians and MJD (TT).
-//! - [`ObservationBatch::from_degrees_owned`] — converts degrees/arcseconds → radians
-//!   once and stores owned buffers.
-//!
-//! ## Example
-//! -----------------
-//! ```rust,no_run
-//! use std::sync::Arc;
-//! use outfit::{
-//!     Outfit, Observer, TrajectorySet, TrajectoryFile, ErrorModel,
-//!     trajectories::batch_reader::ObservationBatch,
-//! };
-//!
-//! // Inputs in degrees / arcseconds (mixed objects: 0 and 1).
-//! let traj_id = vec![0_u32, 0, 1];
-//! let ra_deg  = vec![210.01, 210.02, 211.00];
-//! let dec_deg = vec![-5.00, -4.99, -4.00];
-//! let mjd_tt  = vec![60345.12, 60345.13, 60345.20];
-//!
-//! let batch = ObservationBatch::from_degrees_owned(
-//!     &traj_id, &ra_deg, &dec_deg, 0.5, 0.5, &mjd_tt
-//! );
-//!
-//! // Global environment and observer.
-//! let mut outfit = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
-//! let observer = outfit.get_observer_from_mpc_code(&"I41".to_string());
-//!
-//! // Build a new TrajectorySet directly from the batch.
-//! let traj_set = TrajectorySet::new_from_vec(&mut outfit, &batch, observer.clone())
-//!     .expect("ingestion OK");
-//!
-//! // Or append to an existing set:
-//! let mut other = TrajectorySet::default();
-//! other.add_from_vec(&mut outfit, &batch, observer).expect("append OK");
-//! ```
-//!
-//! ## Notes
-//! -----------------
-//! - Internally, ingestion is performed by a crate-private routine
-//!   (`observation_from_batch`) which expands the batch into per-sample
-//!   [`Observation`]s and caches observer positions per epoch. Users should rely
-//!   on the public `TrajectoryFile` methods instead.
-//! - For multi-observer datasets, create one [`ObservationBatch`] per observer,
-//!   then ingest them separately.
-//!
-//! ## See also
-//! ------------
-//! * [`ObservationBatch::from_radians_borrowed`] – Zero-copy construction.  
-//! * [`ObservationBatch::from_degrees_owned`] – Convert degrees/arcseconds once.  
-//! * [`TrajectoryFile::new_from_vec`](crate::trajectories::trajectory_file::TrajectoryFile::new_from_vec) – Public entry point for batch ingestion.  
-//! * [`TrajectoryFile::add_from_vec`](crate::trajectories::trajectory_file::TrajectoryFile::add_from_vec) – Append batch into an existing set.
-use std::{borrow::Cow, sync::Arc};
-
-use ahash::RandomState;
-use hifitime::Epoch;
-use nalgebra::Vector3;
-use ordered_float::OrderedFloat;
-use smallvec::SmallVec;
-
-use crate::{
-    constants::Radian, conversion::arcsec_to_rad, observations::Observation,
-    trajectories::parquet_reader::FastHashMap, ArcSec, Degree, ObjectNumber, Observer, Outfit,
-    OutfitError, TrajectorySet, MJD,
-};
-
-/// Batch of observations from a single observer (angles in **radians**).
-///
-/// This container groups multiple astrometric measurements sharing the same
-/// observer into a single batch, ready to be expanded into
-/// [`Observation`]s and stored in a
-/// [`TrajectorySet`].
-///
-/// Each measurement includes:
-/// - A trajectory identifier (`trajectory_id`) so that a single batch can hold
-///   observations for multiple objects simultaneously.
-/// - Right ascension and declination in **radians**, with uniform 1-σ uncertainties
-///   (also in **radians**).
-/// - Epochs in **MJD (TT)** (days).
-///
-/// Fields
-/// -----------------
-/// * `trajectory_id` — Integer trajectory IDs (object numbers). Length must match `ra`/`dec`/`time`.
-/// * `ra` — Right ascension values (**radians**). Length must match `dec`, `time`, and `trajectory_id`.
-/// * `error_ra` — 1-σ uncertainty on right ascension (**radians**) applied uniformly to the batch.
-/// * `dec` — Declination values (**radians**). Length must match `ra`, `time`, and `trajectory_id`.
-/// * `error_dec` — 1-σ uncertainty on declination (**radians**) applied uniformly to the batch.
-/// * `time` — Observation epochs as **MJD (TT)** (days). Length must match `ra`/`dec`/`trajectory_id`.
-///
-/// Invariants
-/// -----------------
-/// * `trajectory_id.len() == ra.len() == dec.len() == time.len()`
-/// * Angles and uncertainties are expressed in **radians**.
-/// * Time scale is **TT** (use appropriate conversion if your source data are in UTC/TAI).
-///
-/// Construction
-/// -----------------
-/// Prefer the dedicated constructors:
-/// * [`ObservationBatch::from_radians_borrowed`] — zero-copy when your inputs are already in radians.
-/// * [`ObservationBatch::from_degrees_owned`] — converts degrees/arcseconds once into owned buffers.
-///
-/// Example
-/// -----------------
-/// ```rust, no_run
-/// # use outfit::trajectories::batch_reader::ObservationBatch;
-/// # let (traj_id, ra_deg, dec_deg, mjd) = (vec![0, 0, 1], vec![14.62, 14.63, 15.01], vec![9.98, 10.01, 11.02], vec![43785.35, 43785.36, 43785.40]);
-/// // Inputs in degrees / arcseconds (converted once to radians internally):
-/// let batch = ObservationBatch::from_degrees_owned(&traj_id, &ra_deg, &dec_deg, 0.5, 0.5, &mjd);
-///
-/// // Or, if you already have radians:
-/// // let batch = ObservationBatch::from_radians_borrowed(&ra_rad, &dec_rad, err_ra_rad, err_dec_rad, &mjd);
-/// ```
-///
-/// See also
-/// ------------
-/// * [`ObservationBatch::from_radians_borrowed`] – Borrow slices already in radians (zero-copy).
-/// * [`ObservationBatch::from_degrees_owned`] – Convert degrees/arcseconds → radians once.
-/// * [`conversion::arcsec_to_rad`](crate::conversion::arcsec_to_rad) – Arcseconds → radians helper.
-#[derive(Debug, Clone)]
-pub struct ObservationBatch<'a> {
-    pub trajectory_id: Cow<'a, [u32]>,
-
-    /// Right ascension values (**radians**). Must have the same length as `dec` and `time`.
-    pub ra: Cow<'a, [Radian]>,
-
-    /// 1-σ uncertainty on right ascension (**radians**), applied uniformly to the batch.
-    /// Note: the weighting scheme accounts for the RA geometry (e.g., cos δ factors) downstream.
-    pub error_ra: Radian,
-
-    /// Declination values (**radians**). Must have the same length as `ra` and `time`.
-    pub dec: Cow<'a, [Radian]>,
-
-    /// 1-σ uncertainty on declination (**radians**), applied uniformly to the batch.
-    pub error_dec: Radian,
-
-    /// Observation epochs as **MJD (TT)**, in days. Must have the same length as `ra`/`dec`.
-    pub time: Cow<'a, [MJD]>,
-}
-
-impl<'a> ObservationBatch<'a> {
-    /// Construct a batch by **borrowing** slices that are already in radians.
-    ///
-    /// The returned batch holds `Cow::Borrowed` views of the provided slices,
-    /// performing **no allocation** and **no unit conversion**.
-    /// Use this when your upstream pipeline already provides:
-    /// - Trajectory identifiers (`trajectory_id`)
-    /// - Right ascension / declination in **radians**
-    /// - Uncertainties in **radians**
-    /// - Epochs in **MJD (TT)**
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `trajectory_id` — Integer trajectory IDs; length must match all angle/time slices.
-    /// * `ra_rad` — Right ascension values in **radians** (borrowed).
-    /// * `dec_rad` — Declination values in **radians** (borrowed).
-    /// * `error_ra_rad` — 1-σ uncertainty on RA in **radians**, applied uniformly to the batch.
-    /// * `error_dec_rad` — 1-σ uncertainty on DEC in **radians**, applied uniformly to the batch.
-    /// * `time_mjd` — Observation epochs as **MJD (TT)** (borrowed).
-    ///
-    /// Return
-    /// ----------
-    /// * A batch borrowing the provided slices (**zero-copy**).
-    ///
-    /// Invariants
-    /// ----------
-    /// * `trajectory_id.len() == ra_rad.len() == dec_rad.len() == time_mjd.len()`
-    ///
-    /// Panics
-    /// ----------
-    /// * Debug builds only: panics if the slice lengths do not match.
-    ///
-    /// Complexity
-    /// ----------
-    /// * O(1) — no allocation, no conversion.
-    ///
-    /// See also
-    /// ------------
-    /// * [`ObservationBatch::from_degrees_owned`] – Convert degrees/arcseconds → radians and own the buffers.
-    /// * [`conversion::arcsec_to_rad`](crate::conversion::arcsec_to_rad) – Arcseconds → radians helper.
-    pub fn from_radians_borrowed(
-        trajectory_id: &'a [u32],
-        ra_rad: &'a [Radian],
-        dec_rad: &'a [Radian],
-        error_ra_rad: Radian,
-        error_dec_rad: Radian,
-        time_mjd: &'a [MJD],
-    ) -> Self {
-        debug_assert_eq!(ra_rad.len(), dec_rad.len(), "RA/DEC length mismatch");
-        debug_assert_eq!(ra_rad.len(), time_mjd.len(), "RA/time length mismatch");
-
-        Self {
-            trajectory_id: Cow::Borrowed(trajectory_id),
-            ra: Cow::Borrowed(ra_rad),
-            dec: Cow::Borrowed(dec_rad),
-            time: Cow::Borrowed(time_mjd),
-            error_ra: error_ra_rad,
-            error_dec: error_dec_rad,
-        }
-    }
-
-    /// Construct a batch from **degrees** (angles) and **arcseconds** (uncertainties),
-    /// converting to **radians** and **owning** the resulting buffers.
-    ///
-    /// Use this when your inputs come from common astrometric formats (e.g., MPC/ADES)
-    /// that report RA/DEC in degrees and uncertainties in arcseconds.
-    /// Conversion is performed **once** at construction; downstream code operates purely in radians.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `trajectory_id` — Integer trajectory IDs; length must match all angle/time slices.
-    /// * `ra_deg` — Right ascension in **degrees** (borrowed); converted to radians.
-    /// * `dec_deg` — Declination in **degrees** (borrowed); converted to radians.
-    /// * `error_ra_arcsec` — 1-σ uncertainty on RA in **arcseconds**; converted to radians.
-    /// * `error_dec_arcsec` — 1-σ uncertainty on DEC in **arcseconds**; converted to radians.
-    /// * `time_mjd` — Observation epochs as **MJD (TT)** (borrowed; cloned to owned buffer).
-    ///
-    /// Return
-    /// ----------
-    /// * A batch **owning** converted buffers (no dangling slices).
-    ///
-    /// Invariants
-    /// ----------
-    /// * `trajectory_id.len() == ra_deg.len() == dec_deg.len() == time_mjd.len()`
-    ///
-    /// Panics
-    /// ----------
-    /// * Panics if the slice lengths do not match.
-    ///
-    /// Complexity
-    /// ----------
-    /// * O(n) for the degree→radian and arcsec→radian conversions + one `to_vec()` for time.
-    ///
-    /// See also
-    /// ------------
-    /// * [`ObservationBatch::from_radians_borrowed`] – Zero-copy constructor when inputs are already in radians.
-    /// * [`conversion::arcsec_to_rad`](crate::conversion::arcsec_to_rad) – Arcseconds → radians helper.
-    pub fn from_degrees_owned(
-        trajectory_id: &'a [u32],
-        ra_deg: &[Degree],
-        dec_deg: &[Degree],
-        error_ra_arcsec: ArcSec,
-        error_dec_arcsec: ArcSec,
-        time_mjd: &[MJD],
-    ) -> Self {
-        debug_assert_eq!(ra_deg.len(), dec_deg.len(), "RA/DEC length mismatch");
-        debug_assert_eq!(ra_deg.len(), time_mjd.len(), "RA/time length mismatch");
-
-        let ra: Vec = ra_deg.iter().map(|&d| d.to_radians()).collect();
-        let dec: Vec = dec_deg.iter().map(|&d| d.to_radians()).collect();
-        let time: Vec = time_mjd.to_vec();
-
-        Self {
-            trajectory_id: Cow::Owned(trajectory_id.to_vec()),
-            ra: Cow::Owned(ra),
-            dec: Cow::Owned(dec),
-            time: Cow::Owned(time),
-            error_ra: arcsec_to_rad(error_ra_arcsec),
-            error_dec: arcsec_to_rad(error_dec_arcsec),
-        }
-    }
-}
-
-/// Expand a single-observer batch into concrete [`Observation`]s and append them into a [`TrajectorySet`].
-///
-/// This routine ingests an [`ObservationBatch`] whose angles and uncertainties are in **radians**
-/// and whose epochs are **MJD (TT)**, then materializes per-sample [`Observation`]s enriched with
-/// site geocentric and heliocentric positions. All measurements are assumed to come from the **same
-/// observer** (hence a single `observer: Arc` argument).
-///
-/// For performance, it:
-/// - resolves the observer into a compact `u16` **once** (hot path),
-/// - pre-fetches the UT1 provider **once**,
-/// - caches observer positions by epoch: **MJD(TT) → (geo_pos, helio_pos)**,
-///   so repeated timestamps incur **no extra** position computation.
-///
-/// Internally, epoch keys are wrapped in `OrderedFloat` to enable their use in a hash map
-/// (total order on `f64` while rejecting `NaN` inputs by construction).
-///
-/// Arguments
-/// -----------------
-/// * `trajectories` — Target container to receive observations, bucketed by `trajectory_id`.
-/// * `env_state` — Global [`Outfit`] state (ephemerides, EOP/UT1 providers, etc.).
-/// * `batch` — Angles and 1-σ uncertainties in **radians**; epochs as **MJD (TT)**; includes `trajectory_id`.
-/// * `observer` — The (single) observer for **all** samples in `batch`.
-///
-/// Return
-/// ----------
-/// * `Ok(())` if all observations were successfully appended into `trajectories`,
-/// * `Err(OutfitError)` if site position or heliocentric position computations fail.
-///
-/// Panics
-/// ----------
-/// * **Debug builds only**: length mismatches across `ra/dec/time/trajectory_id` trigger `debug_assert!`.
-///
-/// Complexity
-/// ----------
-/// * Time: **O(n)**, with at most **O(u)** geocentric/heliocentric computations where `u` is the number of
-///   **unique** epochs in the batch (`u ≤ n`) thanks to the epoch→position cache.
-/// * Space: **O(u)** for the epoch→position cache.
-///
-/// Notes
-/// ----------
-/// * Input angles (RA/DEC) and uncertainties **must already be in radians**. If your source is degrees/arcsec,
-///   build the batch via [`ObservationBatch::from_degrees_owned`] (conversion done once at construction).
-/// * Epochs are expected as **TT**. Convert upstream if your pipeline feeds UTC/TAI.
-/// * This function mutates `trajectories` and reads from `env_state`. If you need parallelization, consider
-///   extracting immutable position providers beforehand, or designing providers that accept shared references.
-///
-/// See also
-/// ------------
-/// * [`ObservationBatch::from_radians_borrowed`] – Zero-copy batch when inputs are already radians.
-/// * [`ObservationBatch::from_degrees_owned`] – Degree/arcsec → rad conversion once at construction.
-/// * [`parquet_to_trajset`] – Parquet ingestion using the same unit/weighting logic.
-/// * [`conversion::arcsec_to_rad`] – Arcseconds → radians helper.
-pub(crate) fn observation_from_batch(
-    trajectories: &mut TrajectorySet,
-    env_state: &mut Outfit,
-    batch: &ObservationBatch<'_>,
-    observer: Arc,
-) -> Result<(), OutfitError> {
-    // --- Fast sanity checks (debug only) ---------------------------------------
-    // All slices must be aligned one-to-one. These checks are enforced at construction
-    // time for production, but we keep them here in debug builds to catch regressions.
-    debug_assert_eq!(batch.ra.len(), batch.dec.len(), "RA/DEC length mismatch");
-    debug_assert_eq!(batch.ra.len(), batch.time.len(), "RA/time length mismatch");
-    debug_assert_eq!(
-        batch.ra.len(),
-        batch.trajectory_id.len(),
-        "RA/trajectory_id length mismatch"
-    );
-
-    // Resolve observer ID once (hot path avoids map lookups later).
-    let uint16_obs = env_state.uint16_from_observer(observer.clone());
-
-    // Pre-fetch UT1 provider once.
-    let ut1 = env_state.get_ut1_provider();
-
-    // Heuristic: many surveys repeat epochs per exposure → cache a fraction of N.
-    let n = batch.ra.len();
-    let est_cache_cap = (n / 4).clamp(64, 4096);
-    let mut pos_cache: FastHashMap, (Vector3, Vector3)> =
-        FastHashMap::with_capacity_and_hasher(est_cache_cap, RandomState::default());
-
-    // Safe and fast: iterators avoid per-iteration bounds checks
-    let ra_it = batch.ra.iter().copied();
-    let dec_it = batch.dec.iter().copied();
-    let time_it = batch.time.iter().copied();
-    let id_it = batch.trajectory_id.iter().copied();
-
-    for ((ra, dec), (mjd_tt, traj_id)) in ra_it.zip(dec_it).zip(time_it.zip(id_it)) {
-        // Use OrderedFloat to permit f64 as a key with a total order.
-        let key = OrderedFloat(mjd_tt);
-
-        // Compute (or reuse) positions at this epoch.
-        let (geo_pos, helio_pos) = if let Some(&(geo, helio)) = pos_cache.get(&key) {
-            (geo, helio)
-        } else {
-            let epoch = Epoch::from_mjd_in_time_scale(mjd_tt, hifitime::TimeScale::TT);
-
-            // Geocentric position (velocity returned but unused here).
-            let (geo, _vel) = observer.pvobs(&epoch, ut1)?;
-
-            // Heliocentric position (uses geocentric position).
-            let helio = observer.helio_position(env_state, &epoch, &geo)?;
-
-            pos_cache.insert(key, (geo, helio));
-            (geo, helio)
-        };
-
-        // Build observation and append to the right trajectory bucket.
-        let obs = Observation::with_positions(
-            uint16_obs,
-            ra,              // radians
-            batch.error_ra,  // radians
-            dec,             // radians
-            batch.error_dec, // radians
-            mjd_tt,          // MJD(TT)
-            geo_pos,
-            helio_pos,
-        );
-
-        let obj = ObjectNumber::Int(traj_id);
-        trajectories
-            .entry(obj)
-            .or_insert_with(|| SmallVec::with_capacity(32))
-            .push(obs);
-    }
-
-    Ok(())
-}
diff --git a/src/trajectories/mod.rs b/src/trajectories/mod.rs
deleted file mode 100644
index e04349f..0000000
--- a/src/trajectories/mod.rs
+++ /dev/null
@@ -1,121 +0,0 @@
-//! # Trajectories: ingestion, storage, and batch IOD
-//!
-//! High-level facilities to **ingest**, **store**, and **process** astrometric observations
-//! grouped by object. The central type is [`TrajectorySet`], a fast hash map that buckets
-//! time-ordered observations per [`ObjectNumber`]. Public helpers let you build a set from
-//! multiple formats (MPC 80-column, Parquet, ADES, or in-memory batches) and run a
-//! **Gauss-based Initial Orbit Determination (IOD)** over all objects.
-//!
-//! Modules
-//! -----------------
-//! * [`batch_reader`](crate::trajectories::batch_reader) – Zero-copy container and routines to expand single-observer batches
-//!   into concrete [`Observation`](crate::observations::Observation)s.
-//! * [`mpc_80col_reader`](crate::trajectories::mpc_80col_reader) – Minimal MPC **80-column** file reader.
-//! * [`parquet_reader`](crate::trajectories::parquet_reader) – Arrow/Parquet-based ingestion (`ra`, `dec`, `jd`, `trajectory_id`).
-//! * [`ades_reader`](crate::trajectories::ades_reader) – ADES (MPC XML/JSON) ingestion.
-//! * [`trajectory_file`](crate::trajectories::trajectory_file) – **Public** trait exposing `new_from_*` and `add_from_*` helpers
-//!   to construct/extend a [`TrajectorySet`] from the above sources.
-//! * [`trajectory_fit`](crate::trajectories::trajectory_fit) – Batch Gauss IOD over a set (`TrajectoryFit` trait, results & stats).
-//! * *(crate-private)* `progress_bar` – Optional progress UI when the `progress` feature is enabled.
-//!
-//! Data Model
-//! -----------------
-//! * **Key:** [`ObjectNumber`] (logical object identifier).
-//! * **Value:** `Observations` = `SmallVec` time-ordered per object.
-//! * **Set:** [`TrajectorySet`] = `HashMap`
-//!   for fast hashing and predictable performance on large catalogs.
-//!
-//! Ingestion Sources
-//! -----------------
-//! Use the [`trajectory_file::TrajectoryFile`](crate::trajectories::trajectory_file) trait (implemented for [`TrajectorySet`]):
-//! * **80-col MPC** — `new_from_80col`, `add_from_80col` (fail-fast on parse errors).
-//! * **Parquet** — `new_from_parquet`, `add_from_parquet` (propagate `OutfitError` on I/O/schema).
-//! * **ADES** — `new_from_ades`, `add_from_ades` (error policy handled in the parser).
-//! * **In-memory batch** (single observer) — `new_from_vec`, `add_from_vec`
-//!   using [`batch_reader::ObservationBatch`](crate::trajectories::batch_reader::ObservationBatch) (angles/σ in **radians**, epochs in **MJD (TT)**).
-//!
-//! Units & Time Scales
-//! -----------------
-//! * Internal angles are **radians**; readers convert from **degrees/arcsec** as needed.
-//! * Epochs are **MJD (TT)**; Parquet `"jd"` (assumed **TT**) is converted via
-//!   [`constants::JDTOMJD`](crate::constants::JDTOMJD).
-//! * Single-observer batches carry uniform 1-σ uncertainties (radians) applied per component.
-//!
-//! Batch IOD
-//! -----------------
-//! Use [`trajectory_fit::TrajectoryFit::estimate_all_orbits`](crate::trajectories::trajectory_fit::TrajectoryFit::estimate_all_orbits) to run Gauss IOD over the set.
-//! Returns a map `ObjectNumber → Result<(GaussResult, rms), OutfitError>`. Errors are **per-object**
-//! and do not abort other objects. A cooperative-cancel variant is also available.
-//!
-//! Performance Notes
-//! -----------------
-//! * Ingestion paths project only required columns and cache site positions by epoch.
-//! * [`TrajectorySet`] uses `ahash` for speed; no deduplication is performed on `add_*` methods.
-//! * Ordering is preserved as provided by sources; sorting by time is not enforced here.
-//!
-//! Feature Flags
-//! -----------------
-//! * `progress` — Enables a live progress bar and timing during batch IOD. See
-//!   [`trajectory_fit`](crate::trajectories::trajectory_fit) for details. The UI is crate-internal and optional.
-//!
-//! Quick-Start
-//! -----------------
-//! ```rust,no_run
-//! use rand::SeedableRng;
-//! use std::sync::Arc;
-//! use camino::Utf8Path;
-//! use outfit::{Outfit, TrajectorySet};
-//! use outfit::observers::Observer;
-//! use outfit::trajectories::trajectory_file::TrajectoryFile;
-//! use outfit::trajectories::trajectory_fit::TrajectoryFit;
-//! use outfit::initial_orbit_determination::IODParams;
-//!
-//! # fn run() -> Result<(), outfit::outfit_errors::OutfitError> {
-//! let mut state = Outfit::new("horizon:DE440", outfit::error_models::ErrorModel::FCCT14)?;
-//! let observer: Arc = state.get_observer_from_mpc_code(&"I41".into());
-//!
-//! // Ingest from Parquet, then append 80-column MPC
-//! let mut trajs: TrajectorySet = TrajectorySet::new_from_parquet(
-//!     &mut state, Utf8Path::new("obs.parquet"), observer.clone(), 0.5, 0.5, Some(8192)
-//! )?;
-//! trajs.add_from_80col(&mut state, Utf8Path::new("obs_80col.txt"));
-//!
-//! // Batch IOD
-//! let mut rng = rand::rngs::StdRng::from_os_rng();
-//! let params = IODParams::builder().max_triplets(32).build()?;
-//! let results = trajs.estimate_all_orbits(&state, &mut rng, ¶ms);
-//! # Ok(()) }
-//! ```
-//!
-//! See also
-//! ------------
-//! * [`trajectory_file`](crate::trajectories::trajectory_file) – Public ingestion API.
-//! * [`batch_reader`](crate::trajectories::batch_reader) – Batch expansion for single-observer inputs.
-//! * [`parquet_reader`](crate::trajectories::parquet_reader), [`mpc_80col_reader`](crate::trajectories::mpc_80col_reader), [`ades_reader`](crate::trajectories::ades_reader) – File readers.
-//! * [`trajectory_fit`](crate::trajectories::trajectory_fit) – Batch IOD, results, and statistics.
-//! * [`crate::observations::Observation`] – Atomic astrometric sample.
-//!
-//! ---
-use std::collections::HashMap;
-
-use ahash::RandomState;
-
-use crate::{constants::Observations, ObjectNumber};
-
-pub mod ades_reader;
-pub mod batch_reader;
-pub mod mpc_80col_reader;
-pub mod parquet_reader;
-pub mod trajectory_file;
-pub mod trajectory_fit;
-
-#[cfg(feature = "progress")]
-pub(crate) mod progress_bar;
-
-/// A full set of trajectories for multiple objects.
-///
-/// The key is the [`ObjectNumber`] (identifier of an object).
-/// The value is the list of [`Observation`](crate::observations::Observation) associated with this object.
-///
-/// Uses [`ahash`](https://docs.rs/ahash) for fast hashing.
-pub type TrajectorySet = HashMap;
diff --git a/src/trajectories/mpc_80col_reader.rs b/src/trajectories/mpc_80col_reader.rs
deleted file mode 100644
index b66a401..0000000
--- a/src/trajectories/mpc_80col_reader.rs
+++ /dev/null
@@ -1,345 +0,0 @@
-//! # MPC 80-Column Observation Reader
-//!
-//! Utilities to parse **MPC 80-column** astrometric observations and turn them into
-//! [`Observation`] values usable by the orbit-determination pipeline.
-//!
-//! ## Overview
-//! -----------------
-//! This module provides:
-//! - A small error type [`ParseObsError`] describing MPC parsing failures.
-//! - A crate-internal line parser (`from_80col`) that converts a single 80-col line
-//!   into an [`Observation`] with angles in **radians** and time in **MJD (TT)**.
-//! - A crate-visible batch routine \[`extract_80col`\] that reads an entire file,
-//!   returns all parsed [`Observation`]s, and extracts the **object number** from
-//!   the header line.
-//!
-//! The implementation enforces **MPC CCD** observations (rejects non-CCD lines) and
-//! converts RA/Dec strings using robust helpers (`parse_ra_to_deg`, `parse_dec_to_deg`),
-//! then applies uncertainty handling that accounts for `cos δ` on the RA component.
-//!
-//! ## Units & Conventions
-//! -----------------
-//! - **Input format:** MPC 80-column fixed-width ASCII lines.
-//! - **Angles:** RA/Dec are parsed from strings into **degrees**, then converted to
-//!   **radians**.
-//! - **Uncertainties:** parsed in input units (hour/deg for RA/Dec) and mapped to
-//!   **radians**; RA uncertainties are divided by `cos δ`.
-//! - **Time scale:** Observing time is parsed from fractional date and converted
-//!   to **MJD (TT)** via [`frac_date_to_mjd`].
-//! - **Observer site:** Extracted from columns 77–80 (MPC code), mapped to the
-//!   compact `u16` site id via \[`Outfit::uint16_from_mpc_code`\].
-//!
-//! ## File-Level Object Number
-//! -----------------
-//! \[`extract_80col`\] retrieves an **object number** from the first line using the
-//! conventional MPC header locations (columns `0..5` or fallback to `5..12`), trims
-//! leading zeros, and returns it as an [`ObjectNumber::String`].
-//!
-//! ## Error Handling
-//! -----------------
-//! Parser failures are wrapped into [`OutfitError::Parsing80ColumnFileError`] with a
-//! [`ParseObsError`] payload for precise diagnostics (e.g. *line too short*,
-//! *invalid RA*, *invalid date*). Non-CCD lines are filtered out by default.
-//!
-//! ## See also
-//! ------------
-//! * [`parse_ra_to_deg`] – RA string → degrees with uncertainty.
-//! * [`parse_dec_to_deg`] – Dec string → degrees with uncertainty.
-//! * [`frac_date_to_mjd`] – Fractional date → MJD (TT).
-//! * [`Observation`] – Internal astrometric sample type.
-//! * [`ObjectNumber`] – Logical object identifier.
-//! * [`Outfit`] – Global state (site registry, time scales, etc.).
-use std::ops::Range;
-
-use camino::Utf8Path;
-use thiserror::Error;
-
-use crate::{
-    constants::Observations,
-    conversion::{parse_dec_to_deg, parse_ra_to_deg},
-    observations::Observation,
-    time::frac_date_to_mjd,
-    ObjectNumber, Outfit, OutfitError, RADH, RADSEC,
-};
-
-/// Line-level parsing errors for MPC 80-column observations.
-///
-/// Variants
-/// -----------------
-/// * `TooShortLine` – The line does not reach 80 characters.
-/// * `NotCCDObs` – The line is not flagged as a CCD observation (column 15 is `'s'`).
-/// * `InvalidRA` – Failed to parse RA field (`line[32..44]`); payload carries the offending slice.
-/// * `InvalidDec` – Failed to parse Dec field (`line[44..56]`); payload carries the offending slice.
-/// * `InvalidDate` – Failed to parse fractional date (`line[15..32]`); payload carries the offending slice.
-///
-/// See also
-/// ------------
-/// * [`parse_ra_to_deg`] – Robust RA parser with uncertainty extraction.
-/// * [`parse_dec_to_deg`] – Robust Dec parser with uncertainty extraction.
-/// * [`frac_date_to_mjd`] – Converts fractional date to MJD (TT).
-#[derive(Error, Debug, PartialEq)]
-pub enum ParseObsError {
-    #[error("The line is too short")]
-    TooShortLine,
-    #[error("The line is not a CCD observation")]
-    NotCCDObs,
-    #[error("Error parsing RA: {0}")]
-    InvalidRA(String),
-    #[error("Invalid Dec value: {0}")]
-    InvalidDec(String),
-    #[error("Invalid date: {0}")]
-    InvalidDate(String),
-}
-
-/// Parse a single **MPC 80-column** line into an [`Observation`] (crate-private helper).
-///
-/// This routine enforces **CCD** observations, parses RA/Dec/time fields, maps the
-/// MPC site code to the compact observer id, and builds an [`Observation`] in **radians**
-/// with a **MJD (TT)** epoch. RA uncertainties are divided by `cos δ` to reflect
-/// the geometry on the sphere.
-///
-/// Arguments
-/// -----------------
-/// * `env_state` – Global state used to resolve MPC site codes and build observations.
-/// * `line` – A single 80-column ASCII line.
-///
-/// Return
-/// ----------
-/// * A parsed [`Observation`] or an [`OutfitError::Parsing80ColumnFileError`] on failure.
-///
-/// Panics
-/// ----------
-/// * Never panics directly; errors are surfaced as [`OutfitError`]. Bounds use fixed slices.
-///
-/// Field Layout (MPC 80-col subset used here)
-/// -----------------
-/// * `15..32` – Fractional date (UTC-like string expected by `frac_date_to_mjd`).  
-/// * `32..44` – Right ascension string (parsed by `parse_ra_to_deg`).  
-/// * `44..56` – Declination string (parsed by `parse_dec_to_deg`).  
-/// * `77..80` – MPC site code.
-///
-/// See also
-/// ------------
-/// * [`parse_ra_to_deg`] – RA parsing (degrees + uncertainty).
-/// * [`parse_dec_to_deg`] – Dec parsing (degrees + uncertainty).
-/// * [`frac_date_to_mjd`] – Fractional date → MJD (TT).
-fn from_80col(env_state: &mut Outfit, line: &str) -> Result {
-    if line.len() < 80 {
-        return Err(OutfitError::Parsing80ColumnFileError(
-            ParseObsError::TooShortLine,
-        ));
-    }
-
-    if line.chars().nth(14) == Some('s') {
-        return Err(OutfitError::Parsing80ColumnFileError(
-            ParseObsError::NotCCDObs,
-        ));
-    }
-
-    let (ra, error_ra) = parse_ra_to_deg(line[32..44].trim()).ok_or_else(|| {
-        OutfitError::Parsing80ColumnFileError(ParseObsError::InvalidRA(
-            line[32..44].trim().to_string(),
-        ))
-    })?;
-
-    let (dec, error_dec) = parse_dec_to_deg(line[44..56].trim()).ok_or_else(|| {
-        OutfitError::Parsing80ColumnFileError(ParseObsError::InvalidDec(
-            line[44..56].trim().to_string(),
-        ))
-    })?;
-
-    let time = frac_date_to_mjd(line[15..32].trim()).map_err(|_| {
-        OutfitError::Parsing80ColumnFileError(ParseObsError::InvalidDate(
-            line[15..32].trim().to_string(),
-        ))
-    })?;
-
-    let observer_id = env_state.uint16_from_mpc_code(&line[77..80].trim().into());
-    let observer = env_state.get_observer_from_uint16(observer_id);
-
-    let max_rms = |observation_error: f64, observer_error: f64, factor: f64| {
-        f64::max(observation_error, observer_error * factor)
-    };
-
-    let dec_radians = dec.to_radians();
-    let dec_rad_cos = dec_radians.cos();
-
-    let ra_error = max_rms(
-        (error_ra * RADH) / dec_rad_cos,
-        observer.ra_accuracy.map(|v| v.into_inner()).unwrap_or(0.0),
-        RADSEC / dec_rad_cos,
-    );
-
-    let dec_error = max_rms(
-        error_dec.to_radians(),
-        observer.dec_accuracy.map(|v| v.into_inner()).unwrap_or(0.0),
-        RADSEC,
-    );
-
-    let observation = Observation::new(
-        env_state,
-        observer_id,
-        ra.to_radians(),
-        ra_error,
-        dec_radians,
-        dec_error,
-        time,
-    )?;
-    Ok(observation)
-}
-
-/// Read a full **MPC 80-column** file, returning parsed observations and the object number.
-///
-/// Lines that are not CCD observations are **silently skipped**. Any other parsing error
-/// triggers a panic with context (the current strategy is fail-fast for corrupted inputs).
-/// The object number is extracted from the first line (`0..5`, fallback `5..12`), trimming
-/// leading zeros.
-///
-/// Arguments
-/// -----------------
-/// * `env_state` – Global state used to resolve MPC site codes and build observations.
-/// * `colfile` – Path to the MPC 80-column file.
-///
-/// Return
-/// ----------
-/// * A tuple `(observations, object_number)` where:
-///   - `observations` is a `Vec` with angles in **radians** and epochs in **MJD (TT)**,
-///   - `object_number` is the header-derived [`ObjectNumber::String`].
-///
-/// Panics
-/// ----------
-/// * Panics if the file cannot be read or if a non-CCD line fails to parse for reasons
-///   other than the expected `NotCCDObs` (fail-fast behavior).
-///
-/// See also
-/// ------------
-/// * [`Observation`] – Parsed astrometric sample.
-/// * [`ObjectNumber`] – Identifier extracted from header columns.
-/// * [`parse_ra_to_deg`], [`parse_dec_to_deg`], [`frac_date_to_mjd`] – Parsing helpers.
-pub(crate) fn extract_80col(
-    env_state: &mut Outfit,
-    colfile: &Utf8Path,
-) -> Result<(Observations, ObjectNumber), OutfitError> {
-    let file_content = std::fs::read_to_string(colfile)
-        .unwrap_or_else(|_| panic!("Could not read file {}", colfile.as_str()));
-
-    let first_line = file_content
-        .lines()
-        .next()
-        .unwrap_or_else(|| panic!("Could not read first line of file {}", colfile.as_str()));
-
-    fn get_object_number(line: &str, range: Range) -> String {
-        line[range].trim_start_matches('0').trim().to_string()
-    }
-
-    let mut object_number = get_object_number(first_line, 0..5);
-    if object_number.is_empty() {
-        object_number = get_object_number(first_line, 5..12);
-    }
-
-    Ok((
-        file_content
-            .lines()
-            .filter_map(|line| match from_80col(env_state, line) {
-                Ok(obs) => Some(obs),
-                Err(OutfitError::Parsing80ColumnFileError(ParseObsError::NotCCDObs)) => None,
-                Err(e) => panic!("Error parsing line: {e:?}"),
-            })
-            .collect(),
-        ObjectNumber::String(object_number),
-    ))
-}
-
-#[cfg(test)]
-#[cfg(feature = "jpl-download")]
-mod mpc_80col_test {
-    use super::*;
-
-    #[test]
-    fn test_from_80col_valid_line() {
-        use crate::unit_test_global::OUTFIT_HORIZON_TEST;
-
-        let line =
-            "     K09R05F  C2009 09 15.23433 22 52 22.62 -14 47 03.2          20.8 Vr~097wG96";
-
-        let mut env_state = OUTFIT_HORIZON_TEST.0.clone();
-        let result = from_80col(&mut env_state, line);
-
-        assert!(result.is_ok());
-        let obs = result.unwrap();
-
-        assert_eq!(
-            obs,
-            Observation {
-                observer: 0,
-                ra: 5.988124307160555,
-                error_ra: 1.2535340843609459e-6,
-                dec: -0.25803335512429054,
-                error_dec: 1.0181086985431635e-6,
-                time: 55089.23509601851,
-                observer_earth_position: [
-                    3.0499942822953885e-5,
-                    -8.594304778250371e-6,
-                    2.8491013919142154e-5
-                ]
-                .into(),
-                observer_helio_position: [
-                    0.9968138444702415,
-                    -0.12221921296802639,
-                    -0.05295724448160355
-                ]
-                .into(),
-            }
-        );
-    }
-
-    #[test]
-    fn test_from_80col_too_short_line() {
-        use crate::unit_test_global::OUTFIT_HORIZON_TEST;
-
-        let line = "short line";
-        let mut env_state = OUTFIT_HORIZON_TEST.0.clone();
-        let result = from_80col(&mut env_state, line);
-
-        assert!(matches!(
-            result,
-            Err(OutfitError::Parsing80ColumnFileError(
-                ParseObsError::TooShortLine
-            ))
-        ));
-    }
-
-    #[test]
-    fn test_from_80col_invalid_date() {
-        use crate::unit_test_global::OUTFIT_HORIZON_TEST;
-
-        let line =
-            "     K09R05F  C20xx 09 15.23433 22 52 22.62 -14 47 03.2          20.8 Vr~097wG96";
-        let mut env_state = OUTFIT_HORIZON_TEST.0.clone();
-        let result = from_80col(&mut env_state, line);
-
-        assert!(matches!(
-            result,
-            Err(OutfitError::Parsing80ColumnFileError(
-                ParseObsError::InvalidDate(_)
-            ))
-        ));
-    }
-
-    #[test]
-    fn test_from_80col_invalid_ra_dec() {
-        use crate::unit_test_global::OUTFIT_HORIZON_TEST;
-
-        let line =
-            "     K09R05F  C2009 09 15.23433 XX YY ZZ.ZZ -AA BB CC.C          20.8 Vr~097wG96";
-        let mut env_state = OUTFIT_HORIZON_TEST.0.clone();
-        let result = from_80col(&mut env_state, line);
-
-        assert!(matches!(
-            result,
-            Err(OutfitError::Parsing80ColumnFileError(
-                ParseObsError::InvalidRA(_)
-            ))
-        ));
-    }
-}
diff --git a/src/trajectories/parquet_reader.rs b/src/trajectories/parquet_reader.rs
deleted file mode 100644
index 4a16de9..0000000
--- a/src/trajectories/parquet_reader.rs
+++ /dev/null
@@ -1,362 +0,0 @@
-//! # Parquet Reader for Astrometric Observations
-//!
-//! High-throughput ingestion of angle-only astrometric detections from **Apache Parquet**
-//! into a [`TrajectorySet`]. This module focuses on a minimal, column-projected read path,
-//! converts **JD→MJD (TT)**, and constructs [`Observation`]s while caching observer positions
-//! by unique epoch to avoid repeated ephemeris calls.
-//!
-//! ## Overview
-//! -----------------
-//! The primary entry point is a crate-internal routine that reads Parquet record batches,
-//! projects only the required columns, and appends parsed samples to an existing
-//! [`TrajectorySet`]. It is typically called by higher-level, public ingestion helpers
-//! (e.g., methods exposed by a `TrajectoryFile` trait).
-//!
-//! Key design points:
-//! - **Projection-first**: materialize only the columns used by Outfit.
-//! - **Typed downcast once per batch**: avoid per-row dynamic checks.
-//! - **Fast path for non-null columns**: iterate over `&[f64]` / `&[u32]` slices.
-//! - **Epoch→position cache**: compute `(geo_pos, helio_pos)` at most once per unique MJD(TT).
-//!
-//! ## Expected Parquet Schema
-//! -----------------
-//! The input file must contain (at least) the following leaf columns:
-//! - `ra: Float64` — Right ascension in **degrees**.
-//! - `dec: Float64` — Declination in **degrees**.
-//! - `jd:  Float64` — Epoch in **Julian Date (TT)**.
-//! - `trajectory_id: UInt32` — Grouping key used as [`ObjectNumber::Int`].
-//!
-//! Columns are accessed by **name** at setup (to build the projection mask) and then by
-//! **index** in the hot loop. If a required column is missing, a clean `io::Error` is returned.
-//!
-//! ## Units & Conventions
-//! -----------------
-//! - **Angles:** `ra`, `dec` are stored in **degrees** on disk and converted to **radians**
-//!   before building [`Observation`]s.
-//! - **Uncertainties:** provided as **arcseconds** at call-site, converted to **radians** once;
-//!   applied uniformly to all rows of the file (per-component).
-//! - **Time scale:** `jd` is assumed to be **TT** on disk. It is converted to **MJD (TT)**
-//!   via subtraction by [`JDTOMJD`].
-//! - **Observer:** the file is read under a **single** [`Observer`]. If you ingest heterogeneous
-//!   observers, extend the cache key to `(observer_id, mjd_tt)` or build one cache per observer.
-//!
-//! ## Null Handling Policy
-//! -----------------
-//! Two execution paths:
-//! - **No nulls** (fast path): raw slice iteration with minimal overhead.
-//! - **With nulls** (fallback): per-row checks; incomplete rows are **skipped** to preserve
-//!   correctness. Prefer cleaning datasets upstream for best performance.
-//!
-//! ## Performance Notes
-//! -----------------
-//! - **Projection** avoids unnecessary I/O and deserialization.
-//! - **Batch size** (`8192` by default) amortizes decompression and Arrow decoding;
-//!   tune between `8k` and `64k` depending on storage/CPU.
-//! - **Caching** uses `FastHashMap, (Vector3, Vector3)>`
-//!   keyed by MJD(TT), typically yielding large savings whenever exposures share timestamps.
-//! - **Zero-ephemeris constructor**: [`Observation::with_positions`] prevents recomputing
-//!   positions during construction.
-//!
-//! ## Error Handling
-//! -----------------
-//! - I/O and schema issues surface as `io::Error` or `ParquetError` wrapped into [`OutfitError`].
-//! - Ephemeris/observer computations (`pvobs`, `helio_position`) may return [`OutfitError`].
-//! - Missing required columns produce an `io::ErrorKind::NotFound` with a clear message.
-//!
-//! > **Note**  
-//! > This reader is **crate-private** and is used under the hood by higher-level,
-//! > public ingestion helpers (e.g., methods implementing a `TrajectoryFile` trait).
-//!
-//! ## See also
-//! ------------
-//! * [`Observation::with_positions`] – Lagrange-friendly constructor with precomputed positions.
-//! * [`Observer::pvobs`] – Geocentric site position at epoch.
-//! * [`Observer::helio_position`] – Heliocentric site position at epoch.
-//! * [`JDTOMJD`] – Constant used for `JD → MJD (TT)` conversion.
-//! * [`ObjectNumber`] – Key type for per-object bucketing in [`TrajectorySet`].
-use arrow_array::Array;
-use hifitime::Epoch;
-use nalgebra::Vector3;
-use ordered_float::OrderedFloat;
-use parquet::errors::ParquetError;
-use smallvec::SmallVec;
-use std::collections::hash_map::Entry;
-use std::io;
-use std::sync::Arc;
-
-use crate::constants::ArcSec;
-use crate::conversion::arcsec_to_rad;
-use crate::observers::Observer;
-use crate::outfit::Outfit;
-use crate::outfit_errors::OutfitError;
-use crate::TrajectorySet;
-use crate::{
-    constants::{ObjectNumber, JDTOMJD},
-    observations::Observation,
-};
-use arrow_array::array::{Float64Array, UInt32Array};
-use camino::Utf8Path;
-use parquet::arrow::{arrow_reader::ParquetRecordBatchReaderBuilder, ProjectionMask};
-
-use ahash::RandomState;
-use std::collections::HashMap;
-
-pub type FastHashMap = HashMap;
-
-/// Load astrometric observations from a Parquet file into an existing [`TrajectorySet`].
-///
-/// This routine deserializes batches of observations from a Parquet file, converts
-/// Julian Dates (JD) to Modified Julian Dates (MJD; TT scale), and constructs [`Observation`]
-/// instances with the provided astrometric uncertainties. To avoid redundant and costly
-/// ephemeris computations, it caches the observer's geocentric and heliocentric positions
-/// per unique `(observer, time)` encountered during the read.
-///
-/// Arguments
-/// -----------------
-/// * `trajectories` – The mutable [`TrajectorySet`] to which observations are appended.
-/// * `env_state` – Global environment providing ephemerides, Earth orientation data,
-///   and observer definitions.
-/// * `parquet` – Path to the input Parquet file containing the columns
-///   `ra`, `dec`, `jd`, and `trajectory_id`.
-///   The `ra` and `dec` columns have to be in degrees and of type `Float64`.
-///   The `jd` column has to be in Julian Date (TT) and of type `Float64`.
-///   The `trajectory_id` column has to be of type `UInt32` and is used to group
-///   observations by object.
-/// * `observer` – The [`Observer`] associated with all observations in this file.
-/// * `error_ra` – Right ascension astrometric uncertainty (radians).
-/// * `error_dec` – Declination astrometric uncertainty (radians).
-/// * `batch_size` – Optional Arrow reader batch size (default: 8192 rows).
-///
-/// Performance notes
-/// -----------------
-/// * Projects only the required columns and accesses them by **index** to avoid
-///   per-batch name lookups.
-/// * Uses a per-file cache keyed by MJD (TT) to store `(geo_pos, helio_pos)` and
-///   reuse them across batches and rows.
-/// * Fast path when all columns are non-null: iterates over raw slices (`&[f64]`, `&[u32]`)
-///   for minimal overhead.
-/// * Downcasts to concrete Arrow arrays once per batch (not per row).
-///
-/// Return
-/// ----------
-/// * No return value. Observations are appended in-place to `trajectories`.
-///
-/// See also
-/// ------------
-/// * [`Observation::with_positions`] – Zero-ephemeris constructor used here.
-/// * [`Observer::pvobs`] – Geocentric observer position (and velocity).
-/// * [`Observer::helio_position`] – Heliocentric observer position.
-pub(crate) fn parquet_to_trajset(
-    trajectories: &mut TrajectorySet,
-    env_state: &mut Outfit,
-    parquet: &Utf8Path,
-    observer: Arc,
-    error_ra: ArcSec,
-    error_dec: ArcSec,
-    batch_size: Option,
-) -> Result<(), OutfitError> {
-    // Convert arcsecond uncertainties to radians once (cheap).
-    let error_ra_rad = arcsec_to_rad(error_ra);
-    let error_dec_rad = arcsec_to_rad(error_dec);
-
-    // Resolve observer to its compact u16 key once (hot path avoids map lookups later).
-    let uint16_obs = env_state.uint16_from_observer(observer);
-
-    // Open file and inspect Parquet metadata (I/O and schema discovery happen here).
-    let file = std::fs::File::open(parquet)?;
-    let builder = ParquetRecordBatchReaderBuilder::try_new(file)?;
-
-    let parquet_metadata = builder.metadata();
-    let schema_descr = parquet_metadata.file_metadata().schema_descr();
-
-    // Build a stable projection mask to materialize **only** the columns used by Outfit.
-    // We rely on the projection order to index columns directly in the hot loop.
-    let all_fields = schema_descr.columns();
-    let column_names = ["ra", "dec", "jd", "trajectory_id"];
-    let projection_indices: Vec = column_names
-        .iter()
-        .map(|name| {
-            all_fields
-                .iter()
-                .position(|f| f.name() == *name)
-                // If not found, surface a clean error instead of panicking.
-                .ok_or_else(|| {
-                    io::Error::new(
-                        io::ErrorKind::NotFound,
-                        format!("Column '{name}' not found in schema"),
-                    )
-                })
-        })
-        .collect::>()?;
-    let mask = ProjectionMask::leaves(schema_descr, projection_indices);
-
-    // A larger batch often amortizes decompression + Arrow deserialization cost.
-    // Tune with benches (8192–65536) depending on your I/O and CPU characteristics.
-    let batch_size = batch_size.unwrap_or(8192);
-    let reader = builder
-        .with_projection(mask)
-        .with_batch_size(batch_size)
-        .build()?;
-
-    // Pre-fetch shared providers and observer reference to avoid repeated lookups in the hot loop.
-    let ut1 = env_state.get_ut1_provider();
-    let obs_ref = env_state.get_observer_from_uint16(uint16_obs);
-
-    // Cache MJD(TT) → (geo_pos, helio_pos).
-    // Note: we assume here the file contains a **single** observer. If you ingest multiple
-    // observers, extend the key to (observer_id, time), e.g. by packing into a u64 or using a tuple.
-    let mut pos_cache: FastHashMap, (Vector3, Vector3)> =
-        FastHashMap::with_capacity_and_hasher(4096, RandomState::default());
-
-    // Iterate over Parquet record batches
-    for maybe_batch in reader {
-        // I/O boundary; failures here usually indicate corruption or incompatible schema.
-        let batch = maybe_batch.map_err(ParquetError::from)?;
-        let len = batch.num_rows();
-
-        // Projected columns by index: [0]=ra, [1]=dec, [2]=jd, [3]=trajectory_id
-        // We downcast **once** per batch (cheap) and reuse typed views in the row loop.
-        let ra_arr = batch
-            .column(0)
-            .as_any()
-            .downcast_ref::()
-            .ok_or_else(|| io::Error::new(io::ErrorKind::InvalidData, "ra must be Float64Array"))?;
-        let dec_arr = batch
-            .column(1)
-            .as_any()
-            .downcast_ref::()
-            .ok_or_else(|| {
-                io::Error::new(io::ErrorKind::InvalidData, "dec must be Float64Array")
-            })?;
-        let jd_arr = batch
-            .column(2)
-            .as_any()
-            .downcast_ref::()
-            .ok_or_else(|| io::Error::new(io::ErrorKind::InvalidData, "jd must be Float64Array"))?;
-        let tid_arr = batch
-            .column(3)
-            .as_any()
-            .downcast_ref::()
-            .ok_or_else(|| {
-                io::Error::new(
-                    io::ErrorKind::InvalidData,
-                    "trajectory_id must be UInt32Array",
-                )
-            })?;
-
-        // Fast path when all projected columns have no nulls.
-        // This unlocks tight, bounds-checked loops on `&[T]` slices without per-row Option unwrapping.
-        let no_nulls = ra_arr.nulls().is_none()
-            && dec_arr.nulls().is_none()
-            && jd_arr.nulls().is_none()
-            && tid_arr.nulls().is_none();
-
-        if no_nulls {
-            // Raw slice views (zero allocs, no per-element downcast/boxing).
-            let ra_vals: &[f64] = ra_arr.values();
-            let dec_vals: &[f64] = dec_arr.values();
-            let jd_vals: &[f64] = jd_arr.values();
-            let tid_vals: &[u32] = tid_arr.values();
-
-            // Hot loop: build `Observation`s with positions sourced from the per-file cache.
-            for i in 0..len {
-                // Convert degrees → radians (fast path: one multiply each).
-                let ra_rad = ra_vals[i].to_radians();
-                let dec_rad = dec_vals[i].to_radians();
-
-                // Convert JD → MJD(TT). Assumes `jd` is already in TT scale in the file;
-                // if not, convert scales here before caching.
-                let mjd_time = jd_vals[i] - JDTOMJD;
-                // Using OrderedFloat to allow float keys in a hash map (with a total order).
-                let key = OrderedFloat(mjd_time);
-
-                // Compute observer positions once per unique epoch.
-                // We handle errors with `?` while using the entry API (no closures returning Result).
-                let (geo_pos, helio_pos) = match pos_cache.entry(key) {
-                    Entry::Occupied(e) => *e.get(),
-                    Entry::Vacant(v) => {
-                        let epoch =
-                            Epoch::from_mjd_in_time_scale(mjd_time, hifitime::TimeScale::TT);
-
-                        // Geocentric position (velocity unused here, but available if needed).
-                        let (geo, _vel) = obs_ref.pvobs(&epoch, ut1)?;
-                        // Heliocentric position (requires geocentric as input).
-                        let helio = obs_ref.helio_position(env_state, &epoch, &geo)?;
-
-                        v.insert((geo, helio));
-                        (geo, helio)
-                    }
-                };
-
-                // Zero-ephemeris constructor: avoids recomputing positions at construction.
-                let obs = Observation::with_positions(
-                    uint16_obs,
-                    ra_rad,
-                    error_ra_rad,
-                    dec_rad,
-                    error_dec_rad,
-                    mjd_time,
-                    geo_pos,
-                    helio_pos,
-                );
-
-                // Group observations by `trajectory_id` (ObjectNumber::Int).
-                let obj = ObjectNumber::Int(tid_vals[i]);
-                trajectories
-                    .entry(obj)
-                    .or_insert_with(|| SmallVec::with_capacity(32))
-                    .push(obs);
-            }
-        } else {
-            // Safety fallback: if any column contains nulls, we check row-by-row and skip incomplete rows.
-            // This path is slower, but maintains correctness for sparse/missing data.
-            for i in 0..len {
-                if ra_arr.is_null(i)
-                    || dec_arr.is_null(i)
-                    || jd_arr.is_null(i)
-                    || tid_arr.is_null(i)
-                {
-                    continue; // Drop incomplete rows (policy: skip; alternatively, surface an error)
-                }
-
-                let ra_rad: f64 = ra_arr.value(i).to_radians();
-                let dec_rad = dec_arr.value(i).to_radians();
-                let mjd_time = jd_arr.value(i) - JDTOMJD;
-                let tid = tid_arr.value(i);
-                let key = OrderedFloat(mjd_time);
-
-                let (geo_pos, helio_pos) = match pos_cache.entry(key) {
-                    Entry::Occupied(e) => *e.get(),
-                    Entry::Vacant(v) => {
-                        let epoch =
-                            Epoch::from_mjd_in_time_scale(mjd_time, hifitime::TimeScale::TT);
-
-                        let (geo, _vel) = obs_ref.pvobs(&epoch, ut1)?;
-                        let helio = obs_ref.helio_position(env_state, &epoch, &geo)?;
-
-                        v.insert((geo, helio));
-                        (geo, helio)
-                    }
-                };
-
-                let obs = Observation::with_positions(
-                    uint16_obs,
-                    ra_rad,
-                    error_ra_rad,
-                    dec_rad,
-                    error_dec_rad,
-                    mjd_time,
-                    geo_pos,
-                    helio_pos,
-                );
-
-                trajectories
-                    .entry(ObjectNumber::Int(tid))
-                    .or_insert_with(|| SmallVec::with_capacity(32))
-                    .push(obs);
-            }
-        }
-    }
-
-    Ok(())
-}
diff --git a/src/trajectories/progress_bar.rs b/src/trajectories/progress_bar.rs
deleted file mode 100644
index 40ecba4..0000000
--- a/src/trajectories/progress_bar.rs
+++ /dev/null
@@ -1,115 +0,0 @@
-//! Lightweight iteration timing utilities.
-//!
-//! This module provides helpers to measure and report iteration times
-//! in long-running loops, e.g. when combined with a progress bar
-//! (see the `progress` feature).
-//!
-//! Components
-//! -----------------
-//! * [`IterTimer`] – Tracks per-iteration durations and computes a
-//!   smoothed **exponential moving average** (EMA).
-//!   Useful to get a stable estimate of iteration time even when
-//!   individual steps fluctuate.
-//!
-//! * [`fmt_dur`] – Human-readable formatter for [`Duration`] values,
-//!   producing strings like `"253µs"`, `"42ms"`, or `"3.14s"` depending
-//!   on the scale.
-//!
-//! Usage
-//! -----------------
-//! Typical workflow inside a loop:
-//!
-//! ```rust, no_run
-//! use std::time::Duration;
-//! use your_crate::iter_timer::{IterTimer, fmt_dur};
-//!
-//! let mut timer = IterTimer::new(0.2); // smoothing factor α = 0.2
-//!
-//! for i in 0..10 {
-//!     // ... some expensive work ...
-//!
-//!     let dt = timer.tick();
-//!     println!(
-//!         "iter {i} took {}, EMA = {}",
-//!         fmt_dur(dt),
-//!         fmt_dur(timer.avg())
-//!     );
-//! }
-//! ```
-//!
-//! Design notes
-//! -----------------
-//! * The EMA update rule is:  
-//!   `ema ← α·dt + (1–α)·ema`  
-//!   with `α ∈ (0,1]`.  
-//!   - `α = 1.0` → no smoothing (EMA = last sample).  
-//!   - small `α` → stronger smoothing, slower adaptation.
-//!
-//! * [`IterTimer::tick`] must be called at each iteration boundary.
-//!   The first tick initializes the average to the first duration.
-//!
-//! * [`IterTimer::avg`] returns the smoothed duration as a [`Duration`].
-//!
-//! * This module is enabled only with the `progress` feature.
-#[cfg(feature = "progress")]
-use std::time::{Duration, Instant};
-
-pub struct IterTimer {
-    last: Instant,
-    ema_ns: f64,
-    alpha: f64,
-    count: u64,
-}
-
-impl IterTimer {
-    pub fn new(alpha: f64) -> Self {
-        Self {
-            last: Instant::now(),
-            ema_ns: 0.0,
-            alpha,
-            count: 0,
-        }
-    }
-
-    #[inline]
-    pub fn tick(&mut self) -> Duration {
-        let now = Instant::now();
-        let dt = now.duration_since(self.last);
-        self.last = now;
-        self.count += 1;
-
-        let dt_ns = dt.as_nanos() as f64;
-        self.ema_ns = if self.count == 1 {
-            dt_ns
-        } else {
-            self.alpha * dt_ns + (1.0 - self.alpha) * self.ema_ns
-        };
-
-        dt
-    }
-
-    #[inline]
-    pub fn avg(&self) -> Duration {
-        if self.count == 0 {
-            Duration::from_nanos(0)
-        } else {
-            Duration::from_nanos(self.ema_ns as u64)
-        }
-    }
-}
-
-#[inline]
-pub fn fmt_dur(d: Duration) -> String {
-    let us = d.as_micros();
-    if us < 1_000 {
-        format!("{us}µs")
-    } else {
-        let ms = d.as_millis();
-        if ms < 1_000 {
-            format!("{ms}ms")
-        } else {
-            let s = d.as_secs_f32();
-            format!("{s:.2}s")
-        }
-    }
-}
diff --git a/src/trajectories/trajectory_file.rs b/src/trajectories/trajectory_file.rs
deleted file mode 100644
index 7a104a6..0000000
--- a/src/trajectories/trajectory_file.rs
+++ /dev/null
@@ -1,513 +0,0 @@
-//! # Trajectory ingestion and batch Initial Orbit Determination (IOD)
-//!
-//! High-level utilities to **build and extend** a [`TrajectorySet`] from multiple sources
-//! (MPC 80-column, Parquet, ADES, or in-memory batches) and to run a **Gauss-based IOD**
-//! over all trajectories.
-//!
-//! ## Overview
-//! -----------------
-//! This module exposes the [`TrajectoryFile`] trait implemented for [`TrajectorySet`].
-//! It provides:
-//! - Constructors that **create** a new set from a given source (`new_from_*`),
-//! - Appenders that **extend** an existing set (`add_from_*`),
-//! - Convenience methods to ingest **in-memory batches** (single observer) via
-//!   [`ObservationBatch`].
-//!
-//! Internally, ingestion from in-memory batches uses a crate-private routine
-//! `observation_from_batch` (unit/scale/caching logic). End users should interact only
-//! with the public `new_from_vec` / `add_from_vec` methods.
-//!
-//! ## Data model
-//! -----------------
-//! - A [`TrajectorySet`] is a `HashMap` storing a
-//!   time-ordered list of astrometric observations per object.
-//! - [`ObservationBatch`] is a thin container (borrowed/owned) for angle-only astrometry
-//!   from a **single observer** with uniform uncertainties; it is expanded into concrete
-//!   [`Observation`](crate::observations::Observation)s and grouped by `trajectory_id`.
-//! - Batch IOD returns a
-//!   [`FullOrbitResult`](crate::trajectories::trajectory_fit::FullOrbitResult), i.e. a map
-//!   `ObjectNumber → Result<(Option, f64), OutfitError>`.
-//!
-//! ## Ingestion sources & signatures
-//! -----------------
-//! **MPC 80-column**
-//! - [`TrajectoryFile::new_from_80col`] → `Self`  
-//!   Reads a file, extracts `(Observations, ObjectNumber)` and **inserts** into a new set.
-//!   **Panics** on extraction failure (internal `expect`).  
-//! - [`TrajectoryFile::add_from_80col`] → `()`  
-//!   Reads and **inserts** into an existing set. **Panics** on extraction failure.
-//!
-//! **Parquet** (`"ra"`, `"dec"`, `"jd"`, `"trajectory_id"`)
-//! - [`TrajectoryFile::new_from_parquet`] → `Result`  
-//!   Creates a new set; errors are propagated.
-//! - [`TrajectoryFile::add_from_parquet`] → `Result<(), OutfitError>`  
-//!   Appends to an existing set; errors are propagated.
-//!   *Units on disk:* `ra/dec` in **degrees**, `jd` in **JD (TT)**. Internally converted to
-//!   **radians** and **MJD (TT)** (via [`JDTOMJD`](crate::constants::JDTOMJD)). Per-file
-//!   uncertainties are passed in **arcseconds**.
-//!
-//! **ADES (MPC XML/JSON)**
-//! - [`TrajectoryFile::new_from_ades`] → `Self`  
-//! - [`TrajectoryFile::add_from_ades`] → `()`  
-//!   Both delegate to `parse_ades` and **do not return a `Result`** (errors are handled
-//!   inside the parser or may panic depending on its policy).
-//!
-//! **In-memory batches (single observer)**
-//! - [`TrajectoryFile::new_from_vec`] → `Result`  
-//! - [`TrajectoryFile::add_from_vec`] → `Result<(), OutfitError>`  
-//!   Expand an [`ObservationBatch`] (RA/DEC/σ in **radians**, epochs in **MJD (TT)**)
-//!   into per-sample [`Observation`](crate::observations::Observation)s using the shared
-//!   [`Outfit`] state and **append/group** by `trajectory_id`.
-//!
-//! ## Units & time scales
-//! -----------------
-//! - **Angles**: internal [`Observation`](crate::observations::Observation)s store RA/DEC in **radians**.  
-//!   Parquet/80-column/ADES readers perform degree→radian conversions as needed.
-//! - **Uncertainties**: expected in **arcseconds** at call-site for Parquet/ADES; for
-//!   in-memory batches they must already be in **radians** (uniform per batch).
-//! - **Times**: internal epochs are **MJD (TT)**. Parquet `"jd"` values are assumed **TT**
-//!   and converted via [`JDTOMJD`](crate::constants::JDTOMJD). 80-col/ADES readers apply their respective conversions.
-//!
-//! ## Duplicates & ordering
-//! -----------------
-//! - **No deduplication** is performed by any `add_*` method. Users must avoid re-ingesting
-//!   the same file/batch twice if duplicates are undesirable.
-//! - Observations are stored **as provided**; ordering by time is not enforced here.
-//!
-//! ## Error semantics
-//! -----------------
-//! - Methods returning `Result<_, OutfitError>` propagate I/O/schema/ephemeris errors.
-//! - `new_from_80col` / `add_from_80col` use `expect(...)` internally and therefore may **panic**
-//!   on parse/read failures (fail-fast behavior).
-//! - `new_from_ades` / `add_from_ades` currently **do not** return a `Result`; error handling
-//!   is delegated to `parse_ades` (which may log or panic depending on implementation).
-//!
-//! ## Batch IOD
-//! -----------------
-//! Use [`crate::trajectories::trajectory_fit::TrajectoryFit::estimate_all_orbits`] to run the
-//! full Gauss IOD over each `(ObjectNumber → Observations)` pair. Outcomes per object:
-//! - `Ok(Some(GaussResult))` + RMS — a viable preliminary/corrected orbit,
-//! - `Ok(None)` — pipeline executed but no acceptable solution kept,
-//! - `Err(OutfitError)` — failure **isolated** to that object.
-//!
-//! ## Example
-//! -----------------
-//! ```no_run
-//! use std::sync::Arc;
-//! use camino::Utf8Path;
-//! use rand::SeedableRng;
-//! use outfit::outfit::Outfit;
-//! use outfit::observers::Observer;
-//! use outfit::trajectories::trajectory_file::TrajectoryFile;
-//! use outfit::TrajectoryFit;
-//! use outfit::initial_orbit_determination::IODParams;
-//! use outfit::TrajectorySet;
-//!
-//! # fn demo() -> Result<(), outfit::outfit_errors::OutfitError> {
-//! let mut state = Outfit::new("horizon:DE440", outfit::error_models::ErrorModel::FCCT14)?;
-//! let observer: Arc = state.get_observer_from_mpc_code(&"I41".into());
-//!
-//! // 1) From Parquet (propagates errors)
-//! let mut trajs: TrajectorySet = TrajectorySet::new_from_parquet(
-//!     &mut state,
-//!     Utf8Path::new("observations.parquet"),
-//!     observer.clone(),
-//!     0.5, 0.5,
-//!     Some(8192),
-//! )?;
-//!
-//! // 2) From MPC 80-column (may panic on parse error)
-//! trajs.add_from_80col(&mut state, Utf8Path::new("obs_80col.txt"));
-//!
-//! // 3) Run batch IOD
-//! let mut rng = rand::rngs::StdRng::from_os_rng();
-//! let params = IODParams::builder().max_triplets(32).build()?;
-//! let results = trajs.estimate_all_orbits(&state, &mut rng, ¶ms);
-//! # Ok(()) }
-//! ```
-//!
-//! ## See also
-//! ------------
-//! * [`TrajectoryFile`] – Public ingestion API surface.
-//! * [`ObservationBatch`] – Zero-copy batch container (single observer).
-//! * [`crate::trajectories::trajectory_fit::TrajectoryFit::estimate_all_orbits`] – Batch Gauss IOD.
-//! * [`Outfit`] – Ephemerides, reference frames, and observer registry.
-use std::{collections::HashMap, sync::Arc};
-
-use super::batch_reader::observation_from_batch;
-use crate::constants::ArcSec;
-use crate::observers::Observer;
-use crate::outfit::Outfit;
-use crate::outfit_errors::OutfitError;
-use crate::trajectories::batch_reader::ObservationBatch;
-use crate::TrajectorySet;
-use camino::Utf8Path;
-
-use super::ades_reader::parse_ades;
-use super::mpc_80col_reader::extract_80col;
-use super::parquet_reader::parquet_to_trajset;
-
-/// A trait for the TrajectorySet type definition.
-/// This trait provides methods to create a TrajectorySet from different sources.
-/// It allows to create a TrajectorySet from an 80 column file, a parquet file, or an ADES file.
-/// It also allows to add observations to an existing TrajectorySet from these sources.
-/// The methods are:
-/// * `from_80col`: Create a TrajectorySet from an 80 column file.
-/// * `add_80col`: Add observations to a TrajectorySet from an 80 column file.
-/// * `new_from_vec`: Create a TrajectorySet from a vector of observations.
-/// * `add_from_vec`: Add observations to a TrajectorySet from a vector of observations.
-/// * `new_from_parquet`: Create a TrajectorySet from a parquet file.
-/// * `add_from_parquet`: Add observations to a TrajectorySet from a parquet file.
-/// * `new_from_ades`: Create a TrajectorySet from an ADES file.
-/// * `add_from_ades`: Add observations to a TrajectorySet from an ADES file.
-///
-/// Note
-/// ----
-/// * Warning: No check is done for duplicated observations for every add method.
-///   * The user shoud be careful to not add the same observation or same file twice
-pub trait TrajectoryFile {
-    /// Create a TrajectorySet from an 80 column file
-    /// The trajectory are added in place in the TrajectorySet.
-    /// If a trajectory id already exists, the observations are added to the existing trajectory.
-    ///
-    /// Arguments
-    /// ---------
-    /// * `env_state`: a mutable reference to the Outfit instance
-    /// * `colfile`: a path to an 80 column file
-    ///
-    /// Return
-    /// ------
-    /// * a TrajectorySet containing the observations from the 80 column file
-    ///
-    /// Note
-    /// ----
-    /// * The 80 column file must respect the MPC format.
-    ///   * ref: 
-    fn new_from_80col(env_state: &mut Outfit, colfile: &Utf8Path) -> Self;
-
-    /// Add a set of trajectories from an 80 column file to a TrajectorySet
-    /// The trajectory are added in place in the TrajectorySet.
-    /// If a trajectory id already exists, the observations are added to the existing trajectory.
-    ///
-    /// Arguments
-    /// ---------
-    /// * `env_state`: a mutable reference to the Outfit instance
-    /// * `colfile`: a path to an 80 column file
-    ///
-    /// Note
-    /// ----
-    /// * The 80 column file must respect the MPC format.
-    ///   * ref: 
-    fn add_from_80col(&mut self, env_state: &mut Outfit, colfile: &Utf8Path);
-
-    /// Create a new [`TrajectorySet`] from a batch of observations taken by a single observer.
-    ///
-    /// This constructor consumes an [`ObservationBatch`] and groups its observations
-    /// into trajectories, keyed by their `trajectory_id`.  
-    /// Each observation in the batch must have been recorded by the **same observer**,
-    /// but may belong to **different objects** (distinguished by `trajectory_id`).
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `env_state` — Mutable reference to the global [`Outfit`] state (used for ephemerides, UT1, etc.).
-    /// * `batch` — An [`ObservationBatch`] containing RA/DEC/epoch values (radians + MJD/TT) and trajectory IDs.
-    /// * `observer` — The observer that recorded all observations in the batch.
-    ///
-    /// Return
-    /// -----------------
-    /// * `Ok(Self)` — A new [`TrajectorySet`] containing one or more trajectories populated from the batch.
-    /// * `Err(OutfitError)` — If observation construction or position computations fail.
-    ///
-    /// Invariants
-    /// -----------------
-    /// * `batch.trajectory_id.len() == batch.ra.len() == batch.dec.len() == batch.time.len()`
-    /// * Angles and uncertainties in the batch must already be in **radians**.
-    ///
-    /// Example
-    /// -----------------
-    /// ```rust, no_run
-    /// # use outfit::trajectories::batch_reader::ObservationBatch;
-    /// # use outfit::TrajectorySet;
-    /// # use outfit::TrajectoryFile;
-    /// # use outfit::{Outfit, ErrorModel};
-    /// # use std::sync::Arc;
-    /// # let mut env = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
-    /// # let observer = env.get_observer_from_mpc_code(&"I41".to_string());
-    /// # let (traj_id, ra_deg, dec_deg, mjd) = (vec![0, 0, 1], vec![14.62, 14.63, 15.01], vec![9.98, 10.01, 11.02], vec![43785.35, 43785.36, 43785.40]);
-    /// let batch = ObservationBatch::from_degrees_owned(&traj_id, &ra_deg, &dec_deg, 0.5, 0.5, &mjd);
-    ///
-    /// // Build a trajectory set directly from the batch:
-    /// let ts = TrajectorySet::new_from_vec(&mut env, &batch, observer).unwrap();
-    /// ```
-    fn new_from_vec(
-        env_state: &mut Outfit,
-        batch: &ObservationBatch<'_>,
-        observer: Arc,
-    ) -> Result
-    where
-        Self: Sized;
-
-    /// Add the observations from a batch to an existing [`TrajectorySet`].
-    ///
-    /// This method inserts all observations from the provided [`ObservationBatch`] into
-    /// the current set, grouping them into trajectories by `trajectory_id`.
-    /// Each observation in the batch must have been recorded by the **same observer**,
-    /// but may belong to multiple distinct objects.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `env_state` — Mutable reference to the global [`Outfit`] state (used for ephemerides, UT1, etc.).
-    /// * `batch` — An [`ObservationBatch`] containing RA/DEC/epoch values (radians + MJD/TT) and trajectory IDs.
-    /// * `observer` — The observer that recorded all observations in the batch.
-    ///
-    /// Return
-    /// -----------------
-    /// * `Ok(())` — If all observations were successfully inserted into the `TrajectorySet`.
-    /// * `Err(OutfitError)` — If observation construction or position computations fail.
-    ///
-    /// Example
-    /// -----------------
-    /// ```rust, no_run
-    /// use outfit::trajectories::batch_reader::ObservationBatch;
-    /// use outfit::TrajectorySet;
-    /// use outfit::TrajectoryFile;
-    /// use outfit::{Outfit, ErrorModel};
-    /// use std::sync::Arc;
-    /// use ahash::RandomState;
-    /// use std::collections::HashMap;
-    ///
-    /// let mut env = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
-    /// let observer = env.get_observer_from_mpc_code(&"I41".to_string());
-    /// let (traj_id, ra_deg, dec_deg, mjd) = (vec![0, 0, 1], vec![14.62, 14.63, 15.01], vec![9.98, 10.01, 11.02], vec![43785.35, 43785.36, 43785.40]);
-    /// let batch = ObservationBatch::from_degrees_owned(&traj_id, &ra_deg, &dec_deg, 0.5, 0.5, &mjd);
-    ///
-    /// let mut ts = HashMap::with_hasher(RandomState::new());
-    /// ts.add_from_vec(&mut env, &batch, observer).unwrap();
-    /// ```
-    fn add_from_vec(
-        &mut self,
-        env_state: &mut Outfit,
-        batch: &ObservationBatch<'_>,
-        observer: Arc,
-    ) -> Result<(), OutfitError>;
-
-    /// Create a new [`TrajectorySet`] from a Parquet file.
-    ///
-    /// This function reads a Parquet file containing astrometric observations
-    /// and constructs a full [`TrajectorySet`]. Each observation is associated
-    /// with the provided `observer` and assigned constant uncertainties in
-    /// right ascension and declination.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `env_state` – Global environment providing ephemerides, UT1 provider, and observer mapping.
-    /// * `parquet` – Path to the input Parquet file.
-    /// * `observer` – Observer metadata (shared reference, resolved once to a compact id).
-    /// * `error_ra` – 1-σ uncertainty in right ascension \[arcsec\], applied uniformly.
-    /// * `error_dec` – 1-σ uncertainty in declination \[arcsec\], applied uniformly.
-    /// * `batch_size` – Record batch size for Parquet reader; defaults to 2048 if `None`.
-    ///
-    /// Return
-    /// ----------
-    /// * `Ok(TrajectorySet)` – A new set of trajectories populated from the file.
-    /// * `Err(OutfitError)` – If the file cannot be opened, parsed, or contains invalid data.
-    ///
-    /// Notes
-    /// ----------
-    /// * The Parquet file must contain the following columns: `"ra"`, `"dec"`, `"jd"`, `"trajectory_id"`.
-    /// * The `"jd"` values are assumed to be in TT scale and are converted internally to MJD via [`JDTOMJD`](crate::constants::JDTOMJD).
-    /// * The `ra` and `dec` columns have to be in degrees and of type `Float64`.
-    /// * The `jd` column has to be in Julian Date (TT) and of type `Float64`.
-    /// * The `trajectory_id` column has to be of type `UInt32` and is used to group
-    ///   observations by object.
-    ///
-    /// See also
-    /// ------------
-    /// * [`add_from_parquet`](crate::trajectories::trajectory_file::TrajectoryFile::add_from_parquet) – Adds observations from a Parquet file to an existing set.
-    fn new_from_parquet(
-        env_state: &mut Outfit,
-        parquet: &Utf8Path,
-        mpc_code: Arc,
-        error_ra: ArcSec,
-        error_dec: ArcSec,
-        batch_size: Option,
-    ) -> Result
-    where
-        Self: Sized;
-
-    /// Add observations from a Parquet file to an existing [`TrajectorySet`].
-    ///
-    /// This function appends new observations (grouped by `trajectory_id`)
-    /// to the current set. The same `observer` and astrometric uncertainties
-    /// are applied to all ingested rows.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `env_state` – Global environment providing ephemerides, UT1 provider, and observer mapping.
-    /// * `parquet` – Path to the input Parquet file.
-    /// * `observer` – Observer metadata (shared reference, resolved once to a compact id).
-    /// * `error_ra` – 1-σ uncertainty in right ascension \[arcsec\], applied uniformly.
-    /// * `error_dec` – 1-σ uncertainty in declination \[arcsec\], applied uniformly.
-    /// * `batch_size` – Record batch size for Parquet reader; defaults to 2048 if `None`.
-    ///
-    /// Return
-    /// ----------
-    /// * `Ok(())` – On successful ingestion, with the internal set updated in place.
-    /// * `Err(OutfitError)` – If the file cannot be opened, parsed, or contains invalid data.
-    ///
-    /// Notes
-    /// ----------
-    /// * The Parquet file must contain the following columns: `"ra"`, `"dec"`, `"jd"`, `"trajectory_id"`.
-    /// * The `"jd"` values are assumed to be in TT scale and are converted internally to MJD via [`JDTOMJD`](crate::constants::JDTOMJD).
-    /// * The `ra` and `dec` columns have to be in degrees and of type `Float64`.
-    /// * The `jd` column has to be in Julian Date (TT) and of type `Float64`.
-    /// * The `trajectory_id` column has to be of type `UInt32` and is used to group
-    ///   observations by object.
-    ///
-    /// See also
-    /// ------------
-    /// * [`new_from_parquet`](crate::trajectories::trajectory_file::TrajectoryFile::new_from_parquet) – Creates a brand new set from a Parquet file.
-    fn add_from_parquet(
-        &mut self,
-        env_state: &mut Outfit,
-        parquet: &Utf8Path,
-        observer: Arc,
-        error_ra: ArcSec,
-        error_dec: ArcSec,
-        batch_size: Option,
-    ) -> Result<(), OutfitError>;
-
-    /// Add a set of trajectories to a TrajectorySet from an ADES file
-    ///
-    /// Arguments
-    /// ---------
-    /// * `env_state`: a mutable reference to the Outfit instance
-    /// * `ades`: a path to an ADES file
-    /// * `error_ra`: the error in right ascension (if some values are given, the error ra is supposed to be the same for all observations)
-    /// * `error_dec`: the error in declination (if some values are given, the error dec is supposed to be the same for all observations)
-    ///
-    /// Note
-    /// ----
-    /// * The ADES file must respect the MPC format.
-    ///   * ref: 
-    fn new_from_ades(
-        env_state: &mut Outfit,
-        ades: &Utf8Path,
-        error_ra: Option,
-        error_dec: Option,
-    ) -> Self;
-
-    /// Create a TrajectorySet from an ADES file
-    ///
-    /// Arguments
-    /// ---------
-    /// * `env_state`: a mutable reference to the Outfit instance
-    /// * `ades`: a path to an ADES file
-    /// * `error_ra`: the error in right ascension (if some values are given, the error ra is supposed to be the same for all observations)
-    /// * `error_dec`: the error in declination (if some values are given, the error dec is supposed to be the same for all observations)
-    ///
-    /// Return
-    /// ------
-    /// * a TrajectorySet containing the observations from the ADES file
-    ///
-    /// Note
-    /// ----
-    /// * The ADES file must respect the MPC format.
-    ///   * ref: 
-    fn add_from_ades(
-        &mut self,
-        env_state: &mut Outfit,
-        ades: &Utf8Path,
-        error_ra: Option,
-        error_dec: Option,
-    );
-}
-
-impl TrajectoryFile for TrajectorySet {
-    fn new_from_vec(
-        env_state: &mut Outfit,
-        batch: &ObservationBatch<'_>,
-        observer: Arc,
-    ) -> Result {
-        let mut traj_set: TrajectorySet = HashMap::default();
-        observation_from_batch(&mut traj_set, env_state, batch, observer)?;
-        Ok(traj_set)
-    }
-
-    fn add_from_vec(
-        &mut self,
-        env_state: &mut Outfit,
-        batch: &ObservationBatch<'_>,
-        observer: Arc,
-    ) -> Result<(), OutfitError> {
-        observation_from_batch(self, env_state, batch, observer)?;
-        Ok(())
-    }
-
-    fn add_from_parquet(
-        &mut self,
-        env_state: &mut Outfit,
-        parquet: &Utf8Path,
-        observer: Arc,
-        error_ra: ArcSec,
-        error_dec: ArcSec,
-        batch_size: Option,
-    ) -> Result<(), OutfitError> {
-        parquet_to_trajset(
-            self, env_state, parquet, observer, error_ra, error_dec, batch_size,
-        )
-    }
-
-    fn new_from_parquet(
-        env_state: &mut Outfit,
-        parquet: &Utf8Path,
-        observer: Arc,
-        error_ra: ArcSec,
-        error_dec: ArcSec,
-        batch_size: Option,
-    ) -> Result
-    where
-        Self: Sized,
-    {
-        let mut trajs: TrajectorySet = HashMap::default();
-        parquet_to_trajset(
-            &mut trajs, env_state, parquet, observer, error_ra, error_dec, batch_size,
-        )?;
-        Ok(trajs)
-    }
-
-    fn new_from_80col(env_state: &mut Outfit, colfile: &Utf8Path) -> Self {
-        let mut traj_set: TrajectorySet = HashMap::default();
-        let (observations, object_number) =
-            extract_80col(env_state, colfile).expect("Failed to extract 80col data");
-        traj_set.insert(object_number, observations);
-        traj_set
-    }
-
-    fn add_from_80col(&mut self, env_state: &mut Outfit, colfile: &Utf8Path) {
-        let (observations, object_number) =
-            extract_80col(env_state, colfile).expect("Failed to extract 80col data");
-        self.insert(object_number, observations);
-    }
-
-    fn add_from_ades(
-        &mut self,
-        env_state: &mut Outfit,
-        ades: &Utf8Path,
-        error_ra: Option,
-        error_dec: Option,
-    ) {
-        parse_ades(env_state, ades, self, error_ra, error_dec);
-    }
-
-    fn new_from_ades(
-        env_state: &mut Outfit,
-        ades: &Utf8Path,
-        error_ra: Option,
-        error_dec: Option,
-    ) -> Self {
-        let mut trajs: TrajectorySet = HashMap::default();
-        parse_ades(env_state, ades, &mut trajs, error_ra, error_dec);
-        trajs
-    }
-}
diff --git a/src/trajectories/trajectory_fit.rs b/src/trajectories/trajectory_fit.rs
deleted file mode 100644
index 15f2d89..0000000
--- a/src/trajectories/trajectory_fit.rs
+++ /dev/null
@@ -1,1596 +0,0 @@
-//! # Batch Gauss IOD over Trajectory Sets
-//!
-//! Run a full **Gauss-based Initial Orbit Determination (IOD)** over a
-//! [`TrajectorySet`], collect **per-object outcomes**, and expose convenience
-//! helpers to query or extract solutions and summarize observation counts.
-//!
-//! ## Overview
-//! -----------------
-//! A [`TrajectorySet`] maps each [`ObjectNumber`] to its time-ordered
-//! [`Observations`]. This module implements the [`TrajectoryFit`] trait on
-//! `TrajectorySet`, providing:
-//!
-//! * `estimate_all_orbits` – run the Gauss IOD pipeline on **every object**,
-//! * `estimate_all_orbits_with_cancel` – same, with **cooperative cancellation**,
-//! * `total_observations` / `number_of_trajectories` – quick set-level metrics,
-//! * `obs_count_stats` – summary statistics on observation counts,
-//! * `gauss_result_for` / `take_gauss_result` – ergonomic access to results.
-//!
-//! All objects are processed with the same [`Outfit`] state (ephemerides, error
-//! model, frames), a caller-provided RNG, and a single [`IODParams`] configuration.
-//!
-//! ## Result Model
-//! -----------------
-//! Batch outcomes are returned as a [`FullOrbitResult`]:
-//!
-//! ```text
-//! ObjectNumber → Result<(GaussResult, rms: f64), OutfitError>
-//! ```
-//!
-//! * `Ok((GaussResult, rms))` – the best preliminary/corrected orbit and its RMS
-//!   of normalized astrometric residuals,
-//! * `Err(OutfitError)` – a failure **isolated** to that object (other objects
-//!   continue to be processed).
-//!
-//! Use [`gauss_result_for`] to **borrow** a solution and its RMS, or
-//! [`take_gauss_result`] to **move** them out of the map.
-//!
-//! ## Execution Modes
-//! -----------------
-//! ### Progress UI (feature: `progress`)
-//! When compiled with the `progress` feature, `estimate_all_orbits` renders a
-//! live progress bar (via `indicatif`) and reports per-iteration timing via
-//! a lightweight moving average to help diagnose throughput bottlenecks.
-//!
-//! ### Cooperative cancellation
-//! `estimate_all_orbits_with_cancel` periodically calls a user-provided
-//! closure `should_cancel()` based on **wall-clock intervals** (not iteration
-//! counts) to keep cancellation latency stable even if some objects are slow.
-//!
-//! ## Performance Notes
-//! -----------------
-//! * The loop walks the underlying map once; overall time scales with the number
-//!   of objects × the cost of `ObservationIOD::estimate_best_orbit` (triplet
-//!   enumeration, scoring, optional correction).
-//! * Results are accumulated in a `HashMap` that uses `ahash::RandomState`,
-//!   matching the default hasher used elsewhere in the crate.
-//! * No mutation of the observations themselves; only per-object IOD is performed.
-//!
-//! ## Error Semantics
-//! -----------------
-//! * Failures are **per-object**: an error for one object does **not** abort
-//!   the batch.
-//! * The returned map contains **one entry per processed object**,
-//!   each entry being either `Ok((GaussResult, rms))` or `Err(OutfitError)`.
-//!
-//! ## Examples
-//! -----------------
-//! Minimal end-to-end run (no progress UI):
-//!
-//! ```rust,no_run
-//! use rand::SeedableRng;
-//! use outfit::{Outfit, TrajectorySet};
-//! use outfit::initial_orbit_determination::IODParams;
-//! use outfit::trajectories::trajectory_fit::TrajectoryFit;
-//!
-//! # fn demo(mut trajs: TrajectorySet) -> Result<(), outfit::outfit_errors::OutfitError> {
-//! let state = Outfit::new("horizon:DE440", outfit::error_models::ErrorModel::FCCT14)?;
-//! let mut rng = rand::rngs::StdRng::from_os_rng();
-//! let params = IODParams::builder().max_triplets(32).build()?;
-//!
-//! let results = trajs.estimate_all_orbits(&state, &mut rng, ¶ms);
-//! for (obj, res) in &results {
-//!     match res {
-//!         Ok((g, rms)) => eprintln!("{obj:?}: orbit={} rms={:.4}", g, rms),
-//!         Err(e)       => eprintln!("{obj:?}: error={e}"),
-//!     }
-//! }
-//! # Ok(()) }
-//! ```
-//!
-//! Cooperative cancellation (poll every ~20 ms):
-//!
-//! ```rust,no_run
-//! use std::sync::atomic::{AtomicBool, Ordering};
-//! use outfit::trajectories::trajectory_fit::TrajectoryFit;
-//!
-//! # fn cancelable(mut trajs: outfit::TrajectorySet,
-//! #                state: &outfit::Outfit,
-//! #                rng: &mut impl rand::Rng,
-//! #                params: &outfit::IODParams,
-//! # ) -> outfit::trajectories::trajectory_fit::FullOrbitResult {
-//! let stop = AtomicBool::new(false);
-//! // … flip `stop` from another thread / signal handler …
-//!
-//! trajs.estimate_all_orbits_with_cancel(state, rng, params, || stop.load(Ordering::Relaxed))
-//! # }
-//! ```
-//!
-//! Quick stats for logging/reporting:
-//!
-//! ```rust
-//! use outfit::trajectories::trajectory_fit::TrajectoryFit;
-//!
-//! fn summarize(set: &outfit::TrajectorySet) {
-//!     let n_obj = set.number_of_trajectories();
-//!     let n_obs = set.total_observations();
-//!     if let Some(stats) = set.obs_count_stats() {
-//!         eprintln!("Trajectories: {n_obj}, Observations: {n_obs}");
-//!         eprintln!("{:#}", stats);
-//!     }
-//! }
-//! ```
-//!
-//! ## See also
-//! ------------
-//! * [`TrajectoryFit`] – Trait implemented by `TrajectorySet` for batch IOD and stats.
-//! * [`ObservationIOD::estimate_best_orbit`] – Per-object Gauss IOD (called internally).
-//! * [`GaussResult`] – Preliminary/corrected orbit container.
-//! * [`IODParams`] – Tuning for triplet generation, scoring, correction.
-//! * [`gauss_result_for`] / [`take_gauss_result`] – Accessors for the `FullOrbitResult` map.
-use std::{collections::HashMap, fmt};
-
-use ahash::RandomState;
-use rand::Rng;
-
-use crate::{
-    constants::Observations, GaussResult, IODParams, ObjectNumber, ObservationIOD, Outfit,
-    OutfitError, TrajectorySet,
-};
-
-use std::time::{Duration, Instant};
-
-#[cfg(feature = "progress")]
-use super::progress_bar::IterTimer;
-#[cfg(feature = "progress")]
-use indicatif::{ProgressBar, ProgressStyle};
-
-#[cfg(feature = "parallel")]
-use rayon::prelude::*;
-#[cfg(feature = "parallel")]
-use std::{
-    hash::{Hash, Hasher},
-    mem,
-};
-
-/// Full batch orbit determination results.
-///
-/// Each entry maps an [`ObjectNumber`] to the outcome of a full
-/// Initial Orbit Determination (IOD) attempt on its set of observations.
-///
-/// Internally, this is implemented as:
-///
-/// ```ignore
-/// HashMap, RandomState>
-/// ```
-///
-/// Return semantics
-/// -----------------
-/// * `Ok((GaussResult, f64))` – a successful IOD with its RMS of normalized residuals.
-/// * `Err(OutfitError)` – a failure isolated to that object.
-pub type FullOrbitResult =
-    HashMap, RandomState>;
-
-/// Borrow a Gauss solution (if any) and its RMS for a given key.
-///
-/// Arguments
-/// -----------------
-/// * `all`: The map of all IOD outcomes.
-/// * `key`: The object identifier.
-///
-/// Return
-/// ----------
-/// * `Ok(Some((&GaussResult, f64)))` – a solution is present for the key.
-/// * `Ok(None)` – key absent.
-/// * `Err(&OutfitError)` – the IOD attempt failed for that key.
-///
-/// See also
-/// ------------
-/// * [`GaussResult`] – Gauss IOD output structure.
-pub fn gauss_result_for<'a>(
-    all: &'a FullOrbitResult,
-    key: &ObjectNumber,
-) -> Result, &'a OutfitError> {
-    match all.get(key) {
-        None => Ok(None),
-        Some(Err(e)) => Err(e),
-        Some(Ok((g, rms))) => Ok(Some((g, *rms))),
-    }
-}
-
-/// Take ownership of the solution for `key`, removing it from the map.
-///
-/// Arguments
-/// -----------------
-/// * `all`: The map of all IOD outcomes (consumed entry will be removed).
-/// * `key`: The object identifier to extract.
-///
-/// Return
-/// ----------
-/// * `Ok(Some((GaussResult, f64)))` – ownership of the solution and its RMS.
-/// * `Ok(None)` – key absent.
-/// * `Err(OutfitError)` – the IOD attempt failed for that key.
-///
-/// See also
-/// ------------
-/// * [`gauss_result_for`] – Borrowing accessor.
-pub fn take_gauss_result(
-    all: &mut FullOrbitResult,
-    key: &ObjectNumber,
-) -> Result, OutfitError> {
-    match all.remove(key) {
-        None => Ok(None),
-        Some(Err(e)) => Err(e),
-        Some(Ok((g, rms))) => Ok(Some((g, rms))),
-    }
-}
-
-/// Summary statistics for per-trajectory observation counts.
-///
-/// Each [`TrajectorySet`] entry (one object) has an associated
-/// [`Observations`] container. This structure stores basic distribution
-/// statistics on the **number of observations per trajectory**, as
-/// returned by [`obs_count_stats`](crate::trajectories::trajectory_fit::TrajectoryFit::obs_count_stats).
-///
-/// Fields
-/// -----------------
-/// * `min` – smallest number of observations in any trajectory.
-/// * `p25` – 25th percentile (first quartile) of observation counts.
-/// * `median` – 50th percentile (second quartile).
-/// * `p95` – 95th percentile, indicating the upper tail of the distribution.
-/// * `max` – largest number of observations in any trajectory.
-///
-/// Percentiles are computed using the *nearest-rank* method:
-/// the index is `round(q × (N-1))` for quantile `q ∈ [0,1]`, clamped to valid range.
-/// This convention makes results stable even for small sample sizes.
-///
-/// Display
-/// -----------------
-/// * `format!("{}", stats)` – compact single-line summary, e.g.:
-///   ```text
-///   min=2, p25=4, median=8, p95=15, max=20
-///   ```
-///
-/// * `format!("{:#}", stats)` – pretty multi-line table, e.g.:
-///   ```text
-///   Observation count per trajectory — summary
-///   -----------------------------------------
-///   min    : 2
-///   p25    : 4
-///   median : 8
-///   p95    : 15
-///   max    : 20
-///   ```
-///
-/// See also
-/// ------------
-/// * [`obs_count_stats`](crate::trajectories::trajectory_fit::TrajectoryFit::obs_count_stats) – Computes these statistics from a [`TrajectorySet`].
-#[derive(Debug, Clone, Copy)]
-pub struct ObsCountStats {
-    pub min: usize,
-    pub p25: usize,
-    pub median: usize,
-    pub p95: usize,
-    pub max: usize,
-}
-
-impl fmt::Display for ObsCountStats {
-    /// Compact by default; pretty multi-line when using the alternate flag (`{:#}`).
-    ///
-    /// See also
-    /// ------------
-    /// * [`obs_count_stats`](crate::trajectories::trajectory_fit::TrajectoryFit::obs_count_stats) – Builder of these summary statistics.
-    fn fmt(&self, f: &mut fmt::Formatter<'_>) -> fmt::Result {
-        if f.alternate() {
-            // Pretty, multi-line, aligned output (ASCII-only for portability).
-            writeln!(f, "Observation count per trajectory — summary")?;
-            writeln!(f, "-----------------------------------------")?;
-            writeln!(f, "min    : {}", self.min)?;
-            writeln!(f, "p25    : {}", self.p25)?;
-            writeln!(f, "median : {}", self.median)?;
-            writeln!(f, "p95    : {}", self.p95)?;
-            write!(f, "max    : {}", self.max)
-        } else {
-            // Compact single-line for logs and quick prints.
-            write!(
-                f,
-                "min={}, p25={}, median={}, p95={}, max={}",
-                self.min, self.p25, self.median, self.p95, self.max
-            )
-        }
-    }
-}
-
-// ============================================================================
-// Factorized core + progress abstraction + cancel config
-// ============================================================================
-
-/// Cancellation guard polled at fixed wall-clock intervals.
-///
-/// A `CancelCfg` lets the main loop periodically check whether the user
-/// or an external controller has requested an early stop. The loop itself
-/// decides *when* to poll based on the `interval`, and *how* to react
-/// based on the `should_cancel` callback.
-///
-/// Arguments
-/// -----------------
-/// * `interval`: Minimum wall-clock delay between two cancellation checks.
-///   This prevents the loop from calling the callback at every
-///   iteration, which would be too costly.
-/// * `should_cancel`: User-provided closure returning `true` when cancellation
-///   is requested. If `true`, the loop terminates gracefully.
-///
-/// See also
-/// ------------
-/// * [`estimate_all_orbits_core`] – Main iteration loop that evaluates this configuration.
-struct CancelCfg {
-    interval: Duration,
-    should_cancel: F,
-}
-
-/// Abstract interface for reporting progress to the outside world.
-///
-/// The purpose of this trait is to **decouple the heavy numerical loop**
-/// from any particular UI backend. The core orbit determination logic
-/// always calls into a `ProgressSink`, but the actual implementation
-/// depends on the build:
-///
-/// * with the `progress` feature, it is backed by an [`indicatif`] progress bar,
-/// * otherwise, a no-op implementation is used, so the loop compiles without UI.
-///
-/// This abstraction ensures that the loop has a consistent lifecycle:
-///   1. [`start`] is called once with the total number of objects.
-///   2. [`on_iter`] is called at the beginning of each iteration (e.g. to refresh messages).
-///   3. [`inc`] is called once per completed iteration.
-///   4. [`on_interrupt`] is called right before exiting due to cancellation.
-///   5. [`finish`] is always called at the end, successful or not.
-///
-/// By default, all methods are no-ops, so implementors only override the
-/// subset they need.
-trait ProgressSink {
-    /// Called once before entering the main loop, with the total number of items.
-    fn start(&mut self, _total: u64) {}
-    /// Called at the beginning of each iteration (e.g., refresh UI or logs).
-    fn on_iter(&mut self) {}
-    /// Increment the progress by one step.
-    fn inc(&mut self) {}
-    /// Called once if the loop exits because of cancellation.
-    fn on_interrupt(&mut self) {}
-    /// Called once at the very end, regardless of success or cancellation.
-    fn finish(&mut self) {}
-}
-
-/// Default no-op implementation, used when the `progress` feature is disabled.
-impl ProgressSink for () {}
-
-/// Blanket implementation so that `&mut T` also implements [`ProgressSink`].
-///
-/// This lets tests pass `&mut MockProgress` directly, while the core API
-/// continues to accept progress sinks by value.
-impl ProgressSink for &mut T {
-    #[inline]
-    fn start(&mut self, total: u64) {
-        (**self).start(total)
-    }
-    #[inline]
-    fn on_iter(&mut self) {
-        (**self).on_iter()
-    }
-    #[inline]
-    fn inc(&mut self) {
-        (**self).inc()
-    }
-    #[inline]
-    fn on_interrupt(&mut self) {
-        (**self).on_interrupt()
-    }
-    #[inline]
-    fn finish(&mut self) {
-        (**self).finish()
-    }
-}
-
-/// Concrete type selected depending on the `progress` feature:
-/// * [`IndicatifProgress`] when enabled,
-/// * [`()`] (no-op) when disabled.
-#[cfg(feature = "progress")]
-type ProgressImpl = IndicatifProgress;
-#[cfg(not(feature = "progress"))]
-type ProgressImpl = ();
-
-/// Central loop that runs orbit estimation for each trajectory.
-///
-/// This function is the **engine** behind the public APIs:
-/// [`TrajectoryFit::estimate_all_orbits`] and
-/// [`TrajectoryFit::estimate_all_orbits_with_cancel`].
-///
-/// It consumes a [`TrajectorySet`] and tries to estimate the best orbit
-/// for each contained object. Along the way it reports progress, and it
-/// may stop early if the provided cancellation config triggers.
-///
-/// Arguments
-/// -----------------
-/// * `set`: The trajectory set to process (mutable, results are inserted).
-/// * `state`: Global environment providing ephemerides, constants, and frames.
-/// * `rng`: Random number generator used for noisy triplet realizations.
-/// * `params`: IOD parameters controlling triplet generation and scoring.
-/// * `cancel`: Optional cancellation guard (poll interval + callback).
-/// * `progress`: Progress reporting sink (indicatif bar or no-op).
-///
-/// Return
-/// ----------
-/// * A [`FullOrbitResult`], i.e. a map from object → `Ok((GaussResult, rms))`
-///   or `Err(OutfitError)` depending on whether orbit estimation succeeded.
-///
-/// See also
-/// ------------
-/// * [`TrajectoryFit::estimate_all_orbits`] – Public API without cancellation.
-/// * [`TrajectoryFit::estimate_all_orbits_with_cancel`] – Public API with cancellation.
-fn estimate_all_orbits_core(
-    set: &mut TrajectorySet,
-    state: &Outfit,
-    rng: &mut impl Rng,
-    params: &IODParams,
-    mut cancel: Option>,
-    mut progress: P,
-) -> FullOrbitResult
-where
-    F: FnMut() -> bool,
-    P: ProgressSink,
-{
-    let total = set.len() as u64;
-    progress.start(total.max(1));
-
-    let mut results: FullOrbitResult = HashMap::default();
-    let mut last_poll = Instant::now();
-
-    for (obj, observations) in set.iter_mut() {
-        // --- Timer-based cancellation (if configured)
-        if let Some(CancelCfg {
-            interval,
-            should_cancel,
-        }) = cancel.as_mut()
-        {
-            if last_poll.elapsed() >= *interval {
-                if should_cancel() {
-                    progress.on_interrupt();
-                    break;
-                }
-                last_poll = Instant::now();
-            }
-        }
-
-        progress.on_iter();
-
-        // Core work
-        let res = observations.estimate_best_orbit(state, &state.error_model, rng, params);
-        results.insert(obj.clone(), res);
-
-        progress.inc();
-    }
-
-    progress.finish();
-    results
-}
-
-// --------------------------- Progress (indicatif) ----------------------------
-#[cfg(feature = "progress")]
-mod progress_impl {
-    use super::IterTimer;
-    use super::ProgressSink;
-    use crate::trajectories::progress_bar::fmt_dur;
-
-    /// Progress sink backed by `indicatif`.
-    ///
-    /// See also
-    /// ------------
-    /// * [`estimate_all_orbits_core`] – Calls into this sink at key lifecycle moments.
-    pub(super) struct IndicatifProgress {
-        pb: super::ProgressBar,
-        it_timer: IterTimer,
-    }
-
-    impl Default for IndicatifProgress {
-        fn default() -> Self {
-            // The actual length is set in `start()`.
-            let pb = super::ProgressBar::new(1);
-            Self {
-                pb,
-                it_timer: IterTimer::new(0.2),
-            }
-        }
-    }
-
-    impl ProgressSink for IndicatifProgress {
-        fn start(&mut self, total: u64) {
-            self.pb.set_length(total.max(1));
-            self.pb.set_style(
-                super::ProgressStyle::with_template(
-                    "{bar:40.cyan/blue} {pos}/{len} ({percent:>3}%) \
-                         | {per_sec} | ETA {eta_precise} | {msg}",
-                )
-                .expect("indicatif template"),
-            );
-            self.pb
-                .enable_steady_tick(super::Duration::from_millis(200));
-        }
-
-        fn on_iter(&mut self) {
-            let last = self.it_timer.tick();
-            let avg = self.it_timer.avg();
-            self.pb
-                .set_message(format!("last: {}, avg: {}", fmt_dur(last), fmt_dur(avg)));
-        }
-
-        fn inc(&mut self) {
-            self.pb.inc(1);
-        }
-
-        fn on_interrupt(&mut self) {
-            self.pb.set_message("Interrupted");
-        }
-
-        fn finish(&mut self) {
-            self.pb.disable_steady_tick();
-            self.pb.finish_and_clear();
-        }
-    }
-}
-
-#[cfg(feature = "progress")]
-use progress_impl::IndicatifProgress;
-
-// --------------------------- Parallel features ----------------------------
-
-#[cfg(feature = "parallel")]
-/// Generate a new 64-bit pseudo-random value using the **SplitMix64** algorithm.
-/// This is a simple, fast, and reproducible way to decorrelate seeds for parallel RNGs.
-///
-/// Arguments
-/// -----------------
-/// * `x`: Input state (a `u64` value, typically a hash or a base seed).
-///
-/// Return
-/// ----------
-/// * A `u64` pseudo-random value, suitable for seeding RNGs (e.g., `StdRng`).
-///
-/// See also
-/// ------------
-/// * [`seed_for_object`] – Derives per-object seeds from a base seed and object hash.
-#[inline]
-fn splitmix64(mut x: u64) -> u64 {
-    // SplitMix64 constants and shifts from Steele et al. (2014).
-    x = x.wrapping_add(0x9E3779B97F4A7C15);
-    let mut z = x;
-    z = (z ^ (z >> 30)).wrapping_mul(0xBF58476D1CE4E5B9);
-    z = (z ^ (z >> 27)).wrapping_mul(0x94D049BB133111EB);
-    z ^ (z >> 31)
-}
-
-#[cfg(feature = "parallel")]
-/// Derive a **deterministic per-object RNG seed** from a global base seed.
-///
-/// Each object is first hashed with the crate’s default hasher (`ahash`), and the
-/// resulting 64-bit value is mixed with the base seed via [`splitmix64`].
-/// This ensures that:
-/// - Each object gets a **stable, reproducible seed** (same input → same output).
-/// - Seeds are decorrelated even across many objects.
-/// - Parallel runs remain deterministic regardless of thread scheduling.
-///
-/// Arguments
-/// -----------------
-/// * `base`: A global base seed (drawn once per batch).
-/// * `obj`: The [`ObjectNumber`] used as key to derive the per-object seed.
-///
-/// Return
-/// ----------
-/// * A `u64` deterministic RNG seed for the given object.
-///
-/// See also
-/// ------------
-/// * [`splitmix64`] – Core mixing function.
-/// * [`ObjectNumber`] – Object identifier used in Outfit (MPC number or string).
-#[inline]
-fn seed_for_object(base: u64, obj: &ObjectNumber) -> u64 {
-    // Hash object key with the same family used elsewhere (ahash).
-    let mut h = ahash::AHasher::default();
-    obj.hash(&mut h);
-    let obj_h = h.finish();
-
-    // Mix base seed and object hash through SplitMix64.
-    splitmix64(base ^ obj_h)
-}
-
-// ============================================================================
-// Public trait + factorized implementation
-// ============================================================================
-
-pub trait TrajectoryFit {
-    /// Run Gauss-based Initial Orbit Determination (IOD) for **every trajectory** in the set.
-    ///
-    /// This method iterates over each `(ObjectNumber → Observations)` entry and applies the
-    /// full IOD pipeline: candidate triplet enumeration, preliminary Gauss solution, and
-    /// scoring / selection of the best orbit. It aggregates results into a [`FullOrbitResult`].
-    ///
-    /// Mutation semantics
-    /// -----------------
-    /// * This function requires `&mut self` and may **reorder observations in-place** (e.g.,
-    ///   by time) and/or **update batch-level calibration** data (RMS scaling of quoted errors).
-    /// * The underlying astrometric measurements (RA/DEC/time) remain semantically identical,
-    ///   but their **container order** and **per-observation uncertainty metadata** may change
-    ///   due to calibration and sorting steps used by the estimator.
-    /// * If you rely on a specific iteration order elsewhere, do not assume it is preserved.
-    ///
-    /// Determinism
-    /// -----------------
-    /// * With a fixed RNG seed, the procedure is deterministic given identical inputs and params.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `state`: Global environment providing ephemerides, constants, and reference frames.
-    /// * `rng`: Random number generator used for noisy triplet realizations (e.g., [`StdRng`](rand::rngs::StdRng)).
-    /// * `params`: IOD parameters controlling triplet generation, scoring, and correction loops.
-    ///
-    /// Return
-    /// ----------
-    /// * A [`FullOrbitResult`] mapping each object to either:
-    ///   * `Ok((GaussResult, f64))` – selected orbit and its RMS,
-    ///   * `Err(OutfitError)` – diagnostic if no acceptable solution was found.
-    ///
-    /// Notes
-    /// ----------
-    /// * Failures are isolated: one object failing does not prevent others from being processed.
-    /// * Runtime scales with the number of trajectories and candidate triplets per trajectory.
-    ///
-    /// See also
-    /// ------------
-    /// * [`ObservationIOD::estimate_best_orbit`] – Per-trajectory IOD with best-orbit selection.
-    /// * [`TrajectoryFit::estimate_all_orbits_with_cancel`] – Same API with cooperative cancellation.
-    /// * [`IODParams`] – Tuning parameters for IOD batch execution.
-    fn estimate_all_orbits(
-        &mut self,
-        state: &Outfit,
-        rng: &mut impl Rng,
-        params: &IODParams,
-    ) -> FullOrbitResult;
-
-    /// Count the total number of [`Observation`](crate::observations::Observation) entries across all trajectories.
-    ///
-    /// This method iterates once over all values in the [`TrajectorySet`],
-    /// summing the length of each [`Observations`] container.
-    ///
-    /// Return
-    /// ----------
-    /// * The total number of observations across all objects.
-    fn total_observations(&self) -> usize;
-
-    /// Compute distribution statistics for the number of observations per trajectory.
-    ///
-    /// Each trajectory (one object in the [`TrajectorySet`]) has an associated
-    /// [`Observations`] container. This function collects their sizes and computes:
-    ///
-    /// * `min` – smallest number of observations in any trajectory,
-    /// * `p25` – 25th percentile (first quartile),
-    /// * `median` – 50th percentile (second quartile),
-    /// * `p95` – 95th percentile (upper tail indicator),
-    /// * `max` – largest number of observations in any trajectory.
-    ///
-    /// Percentiles are computed using the *nearest-rank* method:
-    /// the index is `round(q × (N-1))` for quantile `q ∈ [0,1]`, clamped to valid range.
-    /// This makes results robust even for small datasets.
-    ///
-    /// Return
-    /// ----------
-    /// * `None` if the set is empty.
-    /// * `Some(ObsCountStats)` containing the summary statistics otherwise.
-    ///
-    /// See also
-    /// ------------
-    /// * [`total_observations`](crate::trajectories::trajectory_fit::TrajectoryFit::total_observations) – Sum of all observations across trajectories.
-    fn obs_count_stats(&self) -> Option;
-
-    /// Return the number of distinct trajectories (objects) in the set.
-    ///
-    /// This is simply the number of keys in the underlying map.
-    ///
-    /// Return
-    /// ------
-    /// * The number of distinct trajectories (objects) in the set.
-    ///
-    /// See also
-    /// ------------
-    /// * [`total_observations`](crate::trajectories::trajectory_fit::TrajectoryFit::total_observations) – Sum of all observations across trajectories.
-    /// * [`obs_count_stats`](crate::trajectories::trajectory_fit::TrajectoryFit::obs_count_stats) – Statistics on the number of observations per trajectory.
-    fn number_of_trajectories(&self) -> usize;
-
-    /// Run Gauss-based IOD for all trajectories, with **cooperative cancellation** support.
-    ///
-    /// Behaves like [`TrajectoryFit::estimate_all_orbits`], but periodically polls a user
-    /// callback to decide whether to stop early. Returns **partial results** if cancelled.
-    ///
-    /// Mutation semantics
-    /// -----------------
-    /// * Same as the non-cancellable variant: the method may **reorder observations in-place**
-    ///   and update **per-batch calibration** (e.g., RMS alignment of quoted errors).
-    ///
-    /// Cancellation model
-    /// -----------------
-    /// * The loop polls `should_cancel` at ~20 ms wall-clock intervals. When it returns `true`,
-    ///   the loop terminates gracefully, calls `on_interrupt()` on the progress sink (if any),
-    ///   and returns the results accumulated so far.
-    ///
-    /// Determinism
-    /// -----------------
-    /// * With a fixed RNG seed, behavior is deterministic except for the **cut point** at which
-    ///   cancellation is observed (timing dependent).
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `state`: Global environment and reference frames.
-    /// * `rng`: Random number generator for noisy triplet realizations.
-    /// * `params`: IOD parameters.
-    /// * `should_cancel`: Closure polled periodically; return `true` to request early stop.
-    ///
-    /// Return
-    /// ----------
-    /// * A [`FullOrbitResult`]:
-    ///   * Complete if the loop ran to completion,
-    ///   * Partial if cancellation was triggered mid-way.
-    ///
-    /// See also
-    /// ------------
-    /// * [`TrajectoryFit::estimate_all_orbits`] – Non-cancellable variant.
-    fn estimate_all_orbits_with_cancel(
-        &mut self,
-        state: &Outfit,
-        rng: &mut impl Rng,
-        params: &IODParams,
-        should_cancel: F,
-    ) -> FullOrbitResult
-    where
-        F: FnMut() -> bool;
-
-    /// Run Gauss-based Initial Orbit Determination (IOD) over all trajectories
-    /// using **parallel batches**.
-    ///
-    /// The [`TrajectorySet`] is split into chunks of size `batch_size`. Each chunk
-    /// is assigned to a Rayon worker thread, and objects inside a chunk are processed
-    /// sequentially for cache efficiency. A single `base_seed` is drawn from `rng`,
-    /// and a stable per-object seed is derived deterministically to guarantee
-    /// reproducibility regardless of parallel scheduling.
-    ///
-    /// Threading model
-    /// -----------------
-    /// * This function uses the **global Rayon thread pool** by default.
-    /// * The number of worker threads is controlled by the environment variable
-    ///   `RAYON_NUM_THREADS`. For example:
-    ///
-    ///   ```bash
-    ///   RAYON_NUM_THREADS=4 cargo run --release
-    ///   ```
-    ///
-    ///   will cap Rayon to 4 threads across the entire program.
-    /// * If the variable is unset, Rayon defaults to the number of logical CPUs.
-    ///
-    /// Mutation semantics
-    /// -----------------
-    /// * As in the sequential version, this method may **reorder observations**
-    ///   and **update per-batch calibration** (e.g. RMS scaling of quoted errors).
-    /// * Each trajectory’s observation container is reinserted after processing,
-    ///   so `self` remains valid and complete.
-    ///
-    /// Arguments
-    /// -----------------
-    /// * `state`: Global environment (ephemerides, constants, frames).
-    /// * `rng`: Random number generator, used only once to draw a base seed.
-    /// * `params`: IOD parameters controlling triplet generation, scoring, correction.
-    /// * `batch_size`: Number of trajectories per parallel batch. Must be ≥ 1.
-    ///
-    /// Return
-    /// ----------
-    /// * A [`FullOrbitResult`] mapping each object to either:
-    ///   * `Ok((GaussResult, f64))` – best orbit and its RMS,
-    ///   * `Err(OutfitError)` – diagnostic if no acceptable orbit was found.
-    ///
-    /// See also
-    /// ------------
-    /// * [`TrajectoryFit::estimate_all_orbits`] – Sequential variant.
-    /// * [`TrajectoryFit::estimate_all_orbits_with_cancel`] – Sequential variant with cooperative cancellation.
-    #[cfg(feature = "parallel")]
-    fn estimate_all_orbits_in_batches_parallel(
-        &mut self,
-        state: &Outfit,
-        rng: &mut impl rand::Rng,
-        params: &IODParams,
-    ) -> FullOrbitResult;
-}
-
-impl TrajectoryFit for TrajectorySet {
-    fn estimate_all_orbits(
-        &mut self,
-        state: &Outfit,
-        rng: &mut impl Rng,
-        params: &IODParams,
-    ) -> FullOrbitResult {
-        // `ProgressImpl` is `IndicatifProgress` when feature=progress, `()` otherwise.
-        estimate_all_orbits_core(
-            self,
-            state,
-            rng,
-            params,
-            None:: bool>>,
-            ProgressImpl::default(),
-        )
-    }
-
-    fn estimate_all_orbits_with_cancel(
-        &mut self,
-        state: &Outfit,
-        rng: &mut impl Rng,
-        params: &IODParams,
-        mut should_cancel: F,
-    ) -> FullOrbitResult
-    where
-        F: FnMut() -> bool,
-    {
-        let cancel = CancelCfg {
-            interval: Duration::from_millis(20),
-            should_cancel: &mut should_cancel,
-        };
-        estimate_all_orbits_core(
-            self,
-            state,
-            rng,
-            params,
-            Some(cancel),
-            ProgressImpl::default(),
-        )
-    }
-
-    #[cfg(feature = "parallel")]
-    fn estimate_all_orbits_in_batches_parallel(
-        &mut self,
-        state: &Outfit,
-        rng: &mut impl rand::Rng,
-        params: &IODParams,
-    ) -> FullOrbitResult {
-        // Draw a single base seed once; per-object seeds derived deterministically.
-        let base_seed: u64 = rng.random();
-
-        // Take the whole map so we can own/mutate Observations per object off-thread.
-        let mut old: TrajectorySet = mem::take(self);
-        let mut entries: Vec<(ObjectNumber, Observations)> = old.drain().collect();
-
-        let total_items = entries.len() as u64;
-
-        // Materialize batches **by move** (no clone of Observations).
-        let mut batches: Vec> =
-            Vec::with_capacity(entries.len().div_ceil(params.batch_size.max(1)));
-        while !entries.is_empty() {
-            let take_n = entries.len().min(params.batch_size);
-            batches.push(entries.drain(..take_n).collect());
-        }
-
-        // Global progress bar (thread-safe) under the `progress` feature.
-        #[cfg(feature = "progress")]
-        let pb = {
-            use indicatif::{ProgressBar, ProgressStyle};
-            let pb = ProgressBar::new(total_items.max(1));
-            pb.set_style(
-                ProgressStyle::with_template(
-                    "{bar:40.cyan/blue} {pos}/{len} ({percent:>3}%) \
-                     | {per_sec} | ETA {eta_precise} | parallel batches",
-                )
-                .expect("indicatif template"),
-            );
-            pb.enable_steady_tick(std::time::Duration::from_millis(200));
-            pb
-        };
-
-        // Process batches in parallel; each batch processed sequentially for locality.
-        #[allow(clippy::type_complexity)]
-        let mut per_batch: Vec<
-            Vec<(
-                ObjectNumber,
-                Result<(GaussResult, f64), OutfitError>,
-                Observations,
-            )>,
-        > = batches
-            .into_par_iter()
-            .map(|mut batch| {
-                let mut out: Vec<(
-                    ObjectNumber,
-                    Result<(GaussResult, f64), OutfitError>,
-                    Observations,
-                )> = Vec::with_capacity(batch.len());
-
-                for (obj, mut obs) in batch.drain(..) {
-                    use rand::SeedableRng;
-
-                    let local_seed = seed_for_object(base_seed, &obj);
-                    let mut local_rng = rand::rngs::StdRng::seed_from_u64(local_seed);
-
-                    let res =
-                        obs.estimate_best_orbit(state, &state.error_model, &mut local_rng, params);
-
-                    // Thread-safe progress increment.
-                    #[cfg(feature = "progress")]
-                    pb.inc(1);
-
-                    out.push((obj, res, obs));
-                }
-                out
-            })
-            .collect();
-
-        // Finalize progress.
-        #[cfg(feature = "progress")]
-        {
-            pb.disable_steady_tick();
-            pb.finish_and_clear();
-        }
-
-        // Reinsert mutated observations and build results map with the same hasher.
-        let mut results: FullOrbitResult = HashMap::with_hasher(ahash::RandomState::new());
-        for batch in per_batch.drain(..) {
-            for (obj, res, obs) in batch {
-                self.insert(obj.clone(), obs);
-                results.insert(obj, res);
-            }
-        }
-        results
-    }
-
-    #[inline]
-    fn total_observations(&self) -> usize {
-        self.values().map(|obs: &Observations| obs.len()).sum()
-    }
-
-    #[inline]
-    fn number_of_trajectories(&self) -> usize {
-        self.len()
-    }
-
-    fn obs_count_stats(&self) -> Option {
-        // Collect sizes (one pass, O(N))
-        let mut counts: Vec = self.values().map(|obs| obs.len()).collect();
-        if counts.is_empty() {
-            return None;
-        }
-
-        // Sort once, O(N log N). `unstable` is fine since we only need order.
-        counts.sort_unstable();
-
-        #[inline]
-        fn q_index(n: usize, q: f64) -> usize {
-            // Nearest-rank on [0, n-1] using linear index; robust for small n.
-            let pos = q * (n as f64 - 1.0);
-            let idx = pos.round() as isize;
-            idx.clamp(0, (n as isize) - 1) as usize
-        }
-
-        let n = counts.len();
-        let min = counts[0];
-        let max = counts[n - 1];
-        let p25 = counts[q_index(n, 0.25)];
-        let median = counts[q_index(n, 0.50)];
-        let p95 = counts[q_index(n, 0.95)];
-
-        Some(ObsCountStats {
-            min,
-            p25,
-            median,
-            p95,
-            max,
-        })
-    }
-}
-
-#[cfg(test)]
-#[cfg(feature = "jpl-download")]
-mod tests_estimate_all_orbits {
-    use crate::{
-        observations::Observation, unit_test_global::OUTFIT_HORIZON_TEST, KeplerianElements,
-    };
-
-    use super::*;
-    use approx::assert_relative_eq;
-    use rand::SeedableRng;
-    use smallvec::SmallVec;
-    use std::{
-        f64::consts::PI,
-        sync::atomic::{AtomicUsize, Ordering},
-    };
-
-    // -------------------------------
-    // Test fixtures (lightweight)
-    // -------------------------------
-
-    /// Build a tiny TrajectorySet with N empty observation lists.
-    ///
-    /// Note: This assumes `TrajectorySet` is a HashMap-like structure
-    ///       and `ObjectNumber::Int(u64)` exists. Adjust if needed.
-    fn make_set(n: usize) -> TrajectorySet {
-        let mut set: TrajectorySet = std::collections::HashMap::with_hasher(RandomState::new());
-        for i in 0..n {
-            // If your ObjectNumber uses a different constructor, adjust here.
-            let key = ObjectNumber::Int(i as u32);
-            // If Observations is not a Vec, adapt this to your type.
-            let obs: Observations = Default::default();
-            set.insert(key, obs);
-        }
-        set
-    }
-
-    /// Dummy `Outfit` and `IODParams` for tests that do not reach the estimator.
-    ///
-    /// We never call the estimator in cancellation-first tests, so these values
-    /// are placeholders to satisfy the function signatures.
-    fn dummy_env() -> (Outfit, IODParams) {
-        let env = OUTFIT_HORIZON_TEST.0.clone();
-        let params = IODParams::builder()
-            .n_noise_realizations(10)
-            .noise_scale(1.0)
-            .max_obs_for_triplets(12)
-            .max_triplets(30)
-            .build()
-            .unwrap();
-        (env, params)
-    }
-
-    // -------------------------------
-    // Unit tests: cancellation logic
-    // -------------------------------
-
-    /// Cancellation fires before the first object is processed: result should be empty.
-    ///
-    /// This test calls the factorized core with `interval = 0 ms` and a callback
-    /// that immediately requests cancellation. The estimator is never invoked.
-    #[test]
-    fn core_cancel_before_any_work() {
-        let mut set = make_set(5);
-        let (env, params) = dummy_env();
-        let mut rng = rand::rngs::StdRng::seed_from_u64(42);
-
-        // Cancel immediately on the very first poll.
-        let mut cancel_called = 0usize;
-        let mut should_cancel = || {
-            cancel_called += 1;
-            true
-        };
-
-        let cancel = CancelCfg {
-            interval: Duration::from_millis(0),
-            should_cancel: &mut should_cancel,
-        };
-
-        // Use no-op progress sink: works with or without the `progress` feature.
-        let results = estimate_all_orbits_core(&mut set, &env, &mut rng, ¶ms, Some(cancel), ());
-
-        assert!(results.is_empty(), "No object should have been processed");
-        assert!(
-            cancel_called >= 1,
-            "Cancellation should have been polled at least once"
-        );
-    }
-
-    /// Cancellation after exactly one iteration: we expect exactly one entry in the map.
-    ///
-    /// IMPORTANT: This test *may* reach the estimator if the cancellation poll
-    /// happens after the first object. We therefore keep the set size to 1 so
-    /// we never process more than one. If your estimator requires real env/params,
-    /// mark this test as `#[ignore]` until you wire a small valid fixture.
-    #[test]
-    fn core_cancel_after_one_object() {
-        let mut set = make_set(2);
-        let (env, params) = dummy_env();
-        let mut rng = rand::rngs::StdRng::seed_from_u64(123);
-
-        let polls = AtomicUsize::new(0);
-        // First poll = false (let the first object run), next polls = true.
-        let mut should_cancel = || {
-            let c = polls.fetch_add(1, Ordering::Relaxed);
-            c >= 1
-        };
-
-        let cancel = CancelCfg {
-            interval: Duration::from_millis(0), // poll at every loop entry
-            should_cancel: &mut should_cancel,
-        };
-
-        let results = estimate_all_orbits_core(&mut set, &env, &mut rng, ¶ms, Some(cancel), ());
-
-        assert_eq!(
-            results.len(),
-            1,
-            "Exactly one object should have been processed before cancel"
-        );
-    }
-
-    // -------------------------------
-    // Unit tests: progress plumbing
-    // -------------------------------
-
-    /// Mock progress sink to observe lifecycle calls.
-    #[derive(Default)]
-    struct MockProgress {
-        started_with: Option,
-        it_calls: usize,
-        inc_calls: usize,
-        interrupted: bool,
-        finished: bool,
-    }
-
-    impl ProgressSink for MockProgress {
-        fn start(&mut self, total: u64) {
-            self.started_with = Some(total);
-        }
-        fn on_iter(&mut self) {
-            self.it_calls += 1;
-        }
-        fn inc(&mut self) {
-            self.inc_calls += 1;
-        }
-        fn on_interrupt(&mut self) {
-            self.interrupted = true;
-        }
-        fn finish(&mut self) {
-            self.finished = true;
-        }
-    }
-
-    /// Progress sink should receive `start`, `on_interrupt`, and `finish` when cancelling before work.
-    #[test]
-    fn progress_calls_when_cancelled_immediately() {
-        let mut set = make_set(3);
-        let (env, params) = dummy_env();
-        let mut rng = rand::rngs::StdRng::seed_from_u64(7);
-
-        let mut should_cancel = || true;
-        let cancel = CancelCfg {
-            interval: Duration::from_millis(0),
-            should_cancel: &mut should_cancel,
-        };
-
-        let mut mock = MockProgress::default();
-        let results =
-            estimate_all_orbits_core(&mut set, &env, &mut rng, ¶ms, Some(cancel), &mut mock);
-
-        assert!(results.is_empty());
-        assert_eq!(mock.started_with, Some(3));
-        assert!(mock.interrupted, "on_interrupt() must be called");
-        assert!(mock.finished, "finish() must be called");
-        // No iteration advanced, so no inc() and on_iter() expected.
-        assert_eq!(mock.it_calls, 0);
-        assert_eq!(mock.inc_calls, 0);
-    }
-
-    // -------------------------------
-    // Integration tests
-    // -------------------------------
-
-    #[inline]
-    fn angle_abs_diff(a: f64, b: f64) -> f64 {
-        let tau = 2.0 * PI;
-        let mut d = (a - b) % tau;
-        if d > PI {
-            d -= tau;
-        }
-        if d < -PI {
-            d += tau;
-        }
-        d.abs()
-    }
-
-    pub fn assert_keplerian_approx_eq(
-        got: &KeplerianElements,
-        exp: &KeplerianElements,
-        abs_eps: f64,
-        rel_eps: f64,
-    ) {
-        // Scalars (non-angular)
-        assert_relative_eq!(
-            got.reference_epoch,
-            exp.reference_epoch,
-            epsilon = abs_eps,
-            max_relative = rel_eps
-        );
-        assert_relative_eq!(
-            got.semi_major_axis,
-            exp.semi_major_axis,
-            epsilon = abs_eps,
-            max_relative = rel_eps
-        );
-        assert_relative_eq!(
-            got.eccentricity,
-            exp.eccentricity,
-            epsilon = abs_eps,
-            max_relative = rel_eps
-        );
-
-        // Angles (radians), compare with wrap-around
-        for (name, g, e) in [
-            ("inclination", got.inclination, exp.inclination),
-            (
-                "ascending_node_longitude",
-                got.ascending_node_longitude,
-                exp.ascending_node_longitude,
-            ),
-            (
-                "periapsis_argument",
-                got.periapsis_argument,
-                exp.periapsis_argument,
-            ),
-            ("mean_anomaly", got.mean_anomaly, exp.mean_anomaly),
-        ] {
-            let diff = angle_abs_diff(g, e);
-            // Allow absolute OR relative tolerance (whichever is larger).
-            let tol = abs_eps.max(rel_eps * e.abs());
-            assert!(
-            diff <= tol,
-            "Angle {name:?} differs too much: |Δ| = {diff:.6e} > tol {tol:.6e} (got={g:.15}, exp={e:.15})"
-        );
-        }
-    }
-
-    /// Estimate on an empty-observation set should return one entry per object with errors.
-    #[test]
-    fn public_no_progress_runs_all_objects() {
-        let mut set = OUTFIT_HORIZON_TEST.1.clone();
-
-        // TODO: replace with real constructors in your codebase:
-        let (env, params) = dummy_env();
-        let mut rng = rand::rngs::StdRng::seed_from_u64(777);
-
-        use super::TrajectoryFit;
-        let results = set.estimate_all_orbits(&env, &mut rng, ¶ms);
-
-        let string_id = "K09R05F";
-        let orbit = gauss_result_for(&results, &string_id.into())
-            .unwrap()
-            .unwrap()
-            .0
-            .as_inner()
-            .as_keplerian()
-            .unwrap();
-
-        let expected = KeplerianElements {
-            reference_epoch: 57049.25533417104,
-            semi_major_axis: 1.8017448718161189,
-            eccentricity: 0.283572382702194,
-            inclination: 0.2026747553253312,
-            ascending_node_longitude: 0.0079836299943183,
-            periapsis_argument: 1.245049339166438,
-            mean_anomaly: 0.4406946018418537,
-        };
-
-        assert_keplerian_approx_eq(orbit, &expected, 1e-6, 1e-6);
-    }
-
-    /// Public cancellation API should return a partial map when cancelling quickly.
-    #[test]
-    fn public_with_cancel_returns_partial() {
-        let mut set = OUTFIT_HORIZON_TEST.1.clone();
-
-        // TODO: replace with real constructors in your codebase:
-        let (env, params) = dummy_env();
-        let mut rng = rand::rngs::StdRng::seed_from_u64(42);
-
-        use super::TrajectoryFit;
-        // Callback cancels immediately; public API polls every ~20ms.
-        // Depending on estimator speed, a few items may slip in before first poll.
-        let results = set.estimate_all_orbits_with_cancel(&env, &mut rng, ¶ms, || true);
-
-        assert!(
-            results.len() <= 50,
-            "Result map cannot exceed the number of objects"
-        );
-        assert!(
-            !results.is_empty(),
-            "Depending on timing, a few items may be processed before first poll"
-        );
-    }
-
-    // -------------------------------
-    // Accessor helpers tests
-    // -------------------------------
-
-    /// `gauss_result_for` should distinguish: missing key, error entry, ok entry.
-    #[test]
-    fn gauss_accessors_err_and_missing() {
-        let mut all: FullOrbitResult = HashMap::with_hasher(RandomState::new());
-        let k1 = ObjectNumber::Int(1);
-        let k2 = ObjectNumber::Int(2);
-
-        // Insert an error entry for k1. Construct an OutfitError if you have a cheap variant.
-        // If construction is non-trivial, you can skip inserting and just test "missing".
-        all.insert(
-            k1.clone(),
-            Err(OutfitError::InvalidIODParameter("test".into())),
-        );
-
-        // Missing key:
-        assert!(matches!(gauss_result_for(&all, &k2), Ok(None)));
-
-        // Error key:
-        match gauss_result_for(&all, &k1) {
-            Err(e) => {
-                // Just check we got *some* error reference back.
-                let _ = format!("{e}");
-            }
-            other => panic!("expected Err(&OutfitError), got {other:?}"),
-        }
-
-        // Take on missing:
-        assert!(matches!(take_gauss_result(&mut all, &k2), Ok(None)));
-
-        // Take on error:
-        match take_gauss_result(&mut all, &k1) {
-            Err(e) => {
-                let _ = format!("{e}");
-            }
-            other => panic!("expected Err(OutfitError), got {other:?}"),
-        }
-    }
-
-    /// Stats over per-trajectory observation counts.
-    #[test]
-    fn obs_count_stats_basic() {
-        use std::collections::HashMap;
-
-        // Helper: build a dummy Observation for tests only.
-        #[inline]
-        fn dummy_observation() -> Observation {
-            // SAFETY (tests only):
-            // This assumes `Observation` is plain-old-data (floats, ints) and `Copy`,
-            // i.e. no heap-owned fields (String, Vec, Arc, etc.) and no Drop.
-            // Si ce n’est pas vrai dans ton code, remplace cette fonction par
-            // un vrai constructeur de test qui remplit des champs plausibles.
-            assert_is_copy::();
-            unsafe { std::mem::MaybeUninit::::zeroed().assume_init() }
-        }
-
-        // Compile-time check: force `Observation: Copy` pour que le zero-init soit sûr.
-        #[inline(always)]
-        fn assert_is_copy() {}
-
-        // Cas vide.
-        let set = make_set(0);
-        assert!(set.obs_count_stats().is_none(), "Empty set → None");
-
-        // Build uneven counts: 2, 4, 8, 16, 16
-        let mut set: TrajectorySet = HashMap::with_hasher(RandomState::new());
-
-        let mut push_n = |id: u32, n: usize| {
-            let mut v: Observations = SmallVec::with_capacity(n);
-            for _ in 0..n {
-                v.push(dummy_observation());
-            }
-            set.insert(ObjectNumber::Int(id), v);
-        };
-
-        push_n(1, 2);
-        push_n(2, 4);
-        push_n(3, 8);
-        push_n(4, 16);
-        push_n(5, 16);
-
-        let stats = set.obs_count_stats().expect("non-empty");
-        assert_eq!(stats.min, 2);
-        assert_eq!(stats.max, 16);
-        assert_eq!(stats.median, 8);
-        assert_eq!(stats.p25, 4);
-        assert_eq!(stats.p95, 16);
-    }
-
-    #[cfg(test)]
-    #[cfg(feature = "parallel")]
-    mod tests_estimate_orbit_parallel_batches {
-        use super::*;
-        use ahash::RandomState;
-        use rand::SeedableRng;
-
-        // Reuse helpers and fixtures style from your existing tests.
-        // If these are private in another module, duplicate minimal versions here.
-
-        /// Build a tiny TrajectorySet with N empty observation lists.
-        ///
-        /// Note: This assumes `TrajectorySet` is a HashMap-like structure
-        ///       and `ObjectNumber::Int(u32)` exists. Adjust if needed.
-        fn make_set(n: usize) -> TrajectorySet {
-            let mut set: TrajectorySet = std::collections::HashMap::with_hasher(RandomState::new());
-            for i in 0..n {
-                set.insert(ObjectNumber::Int(i as u32), Default::default());
-            }
-            set
-        }
-
-        #[inline]
-        fn total_obs(set: &TrajectorySet) -> usize {
-            set.values().map(|v: &Observations| v.len()).sum()
-        }
-
-        // -------------------------------
-        // Unit tests: basic shape/edges
-        // -------------------------------
-
-        /// Parallel-batched IOD over an empty set should return an empty map.
-        #[test]
-        fn parallel_batches_empty_set_is_empty() {
-            let mut set = make_set(0);
-
-            // Dummy env/params: estimator is never reached for empty set.
-            // If you need to compile without jpl, use the same `dummy_env()` strategy as your seq tests.
-            let env = dummy_env().0;
-            let params = IODParams::builder().batch_size(1024).build().unwrap();
-
-            let mut rng = rand::rngs::StdRng::seed_from_u64(1);
-            let results = set.estimate_all_orbits_in_batches_parallel(&env, &mut rng, ¶ms);
-            assert!(results.is_empty(), "Empty input → empty results");
-            assert_eq!(set.len(), 0, "Set remains empty");
-        }
-
-        /// Batch-size boundaries (1 and very large) should produce exactly one entry per object.
-        ///
-        /// We don't assert on Ok/Err, only that every object was processed and observations were reintegrated.
-        #[test]
-        fn parallel_batches_size_edges_cover_all_objects() {
-            for &batch_size in &[1usize, 10_000usize] {
-                let mut set = make_set(7);
-
-                // Build a dummy env that lets the code run without panicking even if estimator errs.
-                // The estimator may return Err for empty observations — it's fine for this test.
-                let env = dummy_env().0;
-                let params = IODParams::builder().batch_size(batch_size).build().unwrap();
-
-                let before_n = set.len();
-                let before_tot = total_obs(&set);
-
-                let mut rng = rand::rngs::StdRng::seed_from_u64(42);
-                let results = set.estimate_all_orbits_in_batches_parallel(&env, &mut rng, ¶ms);
-
-                assert_eq!(results.len(), before_n, "Exactly one entry per object");
-                assert_eq!(set.len(), before_n, "All objects reinserted in set");
-                assert_eq!(
-                    total_obs(&set),
-                    before_tot,
-                    "Total number of observations is preserved (reorder/calibration only)"
-                );
-            }
-        }
-
-        /// Using the same input and RNG seed must be deterministic across runs, regardless of scheduling.
-        /// This checks **one specific object** for identical formatted outcome (Ok/Err shape and RMS).
-        #[test]
-        fn parallel_batches_deterministic_across_runs_with_same_seed() {
-            // Small synthetic set; estimator likely returns Err for empty observations.
-            // Determinism check focuses on the *presence* and *shape* of results.
-            let build_set = || make_set(5);
-            let env = dummy_env().0;
-            let params = IODParams::builder().batch_size(2).build().unwrap();
-
-            let key = ObjectNumber::Int(2);
-
-            let run_once = |seed: u64| {
-                let mut set = build_set();
-                let mut rng = rand::rngs::StdRng::seed_from_u64(seed);
-                let results = set.estimate_all_orbits_in_batches_parallel(&env, &mut rng, ¶ms);
-                // Record a stable string representation for that key.
-                match results.get(&key) {
-                    None => "None".to_string(),
-                    Some(Ok((_g, rms))) => format!("Ok rms={rms:.12e}"),
-                    Some(Err(e)) => format!("Err: {e}"),
-                }
-            };
-
-            let a = run_once(0xDEADBEEF);
-            let b = run_once(0xDEADBEEF);
-            assert_eq!(a, b, "Same seed/input → identical outcome formatting");
-        }
-
-        // -------------------------------
-        // Integration tests with JPL env
-        // -------------------------------
-
-        mod with_ephem {
-            use super::*;
-            use approx::assert_relative_eq;
-
-            use crate::unit_test_global::OUTFIT_HORIZON_TEST;
-
-            /// Parallel batched results should match the known-good orbit (as in the sequential test).
-            #[test]
-            fn parallel_batches_return_orbit() {
-                // Use the same fixture you use elsewhere.
-                let mut set = OUTFIT_HORIZON_TEST.1.clone();
-                let (env, params) = {
-                    // If you have a helper `dummy_env()` in the seq tests, keep the same one:
-                    let env = OUTFIT_HORIZON_TEST.0.clone();
-                    let params = IODParams::builder()
-                        .n_noise_realizations(10)
-                        .noise_scale(1.0)
-                        .max_obs_for_triplets(12)
-                        .max_triplets(30)
-                        .batch_size(1)
-                        .build()
-                        .unwrap();
-                    (env, params)
-                };
-                let mut rng = rand::rngs::StdRng::seed_from_u64(42);
-
-                // Choose a batch size that is neither 1 nor huge to exercise chunking logic.
-                let results = set.estimate_all_orbits_in_batches_parallel(&env, &mut rng, ¶ms);
-
-                // Same canonical object as in your sequential test:
-                let string_id = "K09R05F";
-                let orbit = gauss_result_for(&results, &string_id.into());
-
-                assert!(orbit.is_ok(), "Result entry should be Ok");
-            }
-
-            /// Parallel batched determinism across different batch sizes.
-            ///
-            /// With same RNG seed + inputs, changing only `batch_size` should not affect results.
-            #[test]
-            fn parallel_batches_results_independent_of_batch_size() {
-                let mut set1 = OUTFIT_HORIZON_TEST.1.clone();
-                let mut set2 = OUTFIT_HORIZON_TEST.1.clone();
-                let (env, params) = {
-                    let env = OUTFIT_HORIZON_TEST.0.clone();
-                    let params = IODParams::builder()
-                        .n_noise_realizations(10)
-                        .noise_scale(1.0)
-                        .max_obs_for_triplets(12)
-                        .max_triplets(30)
-                        .batch_size(64)
-                        .build()
-                        .unwrap();
-                    (env, params)
-                };
-
-                let seed = 0xABCDEF0123456789;
-                let mut rng1 = rand::rngs::StdRng::seed_from_u64(seed);
-                let mut rng2 = rand::rngs::StdRng::seed_from_u64(seed);
-
-                let res1 = set1.estimate_all_orbits_in_batches_parallel(&env, &mut rng1, ¶ms);
-
-                let params2 = IODParams {
-                    batch_size: 4096,
-                    ..params.clone()
-                };
-
-                let res2 = set2.estimate_all_orbits_in_batches_parallel(&env, &mut rng2, ¶ms2);
-
-                // Compare a known object Keplerian solution (same as above).
-                let key = "K09R05F".into();
-                let k1 = gauss_result_for(&res1, &key)
-                    .unwrap()
-                    .unwrap()
-                    .0
-                    .as_inner()
-                    .as_keplerian()
-                    .unwrap();
-                let k2 = gauss_result_for(&res2, &key)
-                    .unwrap()
-                    .unwrap()
-                    .0
-                    .as_inner()
-                    .as_keplerian()
-                    .unwrap();
-
-                // Tight numerical equality (same seed → same triplet noise → identical orbit).
-                assert_relative_eq!(k1.reference_epoch, k2.reference_epoch, epsilon = 0.0);
-                assert_relative_eq!(k1.semi_major_axis, k2.semi_major_axis, epsilon = 0.0);
-                assert_relative_eq!(k1.eccentricity, k2.eccentricity, epsilon = 0.0);
-                assert_relative_eq!(k1.inclination, k2.inclination, epsilon = 0.0);
-                assert_relative_eq!(
-                    k1.ascending_node_longitude,
-                    k2.ascending_node_longitude,
-                    epsilon = 0.0
-                );
-                assert_relative_eq!(k1.periapsis_argument, k2.periapsis_argument, epsilon = 0.0);
-                assert_relative_eq!(k1.mean_anomaly, k2.mean_anomaly, epsilon = 0.0);
-            }
-        }
-    }
-}
diff --git a/src/trajectory.rs b/src/trajectory.rs
new file mode 100644
index 0000000..bea91cf
--- /dev/null
+++ b/src/trajectory.rs
@@ -0,0 +1,810 @@
+use std::ops::ControlFlow;
+
+use nalgebra::Vector3;
+use photom::{observation_dataset::observation::Observation, Radians};
+
+use crate::{
+    cache::OutfitCache,
+    initial_orbit_determination::{gauss::GaussObs, triplet_generation::generate_triplets},
+    obs_dataset::IODRMS,
+    observation_ephemeris::ObservationEphemeris,
+    EquinoctialElements, GaussResult, IODParams, JPLEphem, OutfitError,
+};
+
+pub(crate) trait TrajectoryFit {
+    /// Extract astrometric uncertainties (RA and DEC) for a set of three observations.
+    ///
+    /// Given a triplet of observation indices, this function retrieves the corresponding
+    /// astrometric errors in right ascension and declination from the observation set.
+    ///
+    /// # Arguments
+    ///
+    /// - `idx_obs` - A vector of three indices referring to the observations used in the triplet.
+    ///
+    /// # Returns
+    ///
+    /// - A tuple of two `Vector3`:
+    ///   - The first vector contains the RA uncertainties in radians.
+    ///   - The second vector contains the DEC uncertainties in radians.
+    ///
+    /// # Panics
+    ///
+    /// This function will panic if any index in `idx_obs` is out of bounds of the observation set.
+    fn extract_errors(&self, idx_obs: Vector3) -> (Vector3, Vector3);
+
+    /// Compute **time-feasible, best-K** triplets of observations for Gauss IOD,
+    /// leveraging a lazy **index stream** and a bounded **max-heap** on spacing weight.
+    ///
+    /// Overview
+    /// -----------------
+    /// This method is a convenience wrapper around [`generate_triplets`]. It operates
+    /// directly on `self` (the current observation set) and returns up to `max_triplet`
+    /// **best-scored** candidates for the Gauss preliminary solution. Internally it:
+    ///
+    /// 1) Uses a `TripletIndexGenerator` that:
+    ///    - sorts epochs in place,
+    ///    - downsamples to at most `max_obs_for_triplets` (uniform with edges),
+    ///    - lazily **streams reduced indices** `(first, middle, last)` constrained by:
+    ///      `dt_min ≤ t[last] − t[first] ≤ dt_max`.
+    /// 2) Scores each feasible triplet with [`triplet_weight`](crate::observations::triplets_iod::triplet_weight) against `optimal_interval_time`.
+    /// 3) Keeps only the **K** smallest weights in a bounded **max-heap** (best-K selection).
+    /// 4) Materializes the survivors as [`GaussObs`] by (re)borrowing `self` immutably.
+    ///
+    /// Compared to brute-force `O(n³)`, the time-windowed enumeration drives the effective
+    /// cost toward ~`O(n²)` in typical time distributions, plus `O(n log K)` for heap updates.
+    ///
+    /// Arguments
+    /// -----------------
+    /// * `dt_min` – Minimum allowed timespan `[same units as Observation::time]` between the first and last epoch of a triplet.
+    /// * `dt_max` – Maximum allowed timespan between the first and last epoch of a triplet.
+    /// * `optimal_interval_time` – Target per-gap spacing (e.g., days) used by [`triplet_weight`](crate::observations::triplets_iod::triplet_weight).
+    /// * `max_obs_for_triplets` – Upper bound on observations kept after downsampling (uniform with endpoints).
+    /// * `max_triplet` – Number `K` of best-scoring triplets to return.
+    ///
+    /// Return
+    /// ----------
+    /// * A `Vec` of length `≤ max_triplet`, **sorted by increasing weight**
+    ///   (best geometric spacing first), ready to be passed to `GaussObs::prelim_orbit`.
+    ///
+    /// Remarks
+    /// -------------
+    /// * Sorting is **in-place**; call sites should not rely on original ordering afterward.
+    /// * The generator avoids overlapping borrows of `self`; only the final K triplets are materialized.
+    /// * For robustness studies, each returned triplet can be expanded with
+    ///   `GaussObs::realizations_iter` (lazy Monte-Carlo noise).
+    ///
+    /// Complexity
+    /// -----------------
+    /// * Enumeration: ~`O(n²)` (per-anchor time window).
+    /// * Selection: `O(n log K)` (bounded max-heap).
+    /// * Space: `O(1)` per yielded candidate; only K triplets are allocated at the end.
+    ///
+    /// See also
+    /// ------------
+    /// * [`generate_triplets`] – Low-level function performing the selection (index stream + heap + materialization).
+    /// * [`TripletIndexGenerator`](crate::observations::triplets_generator::TripletIndexGenerator) – Lazy stream of reduced indices constrained by `(dt_min, dt_max)`.
+    /// * [`triplet_weight`](crate::observations::triplets_iod::triplet_weight) – Spacing heuristic around `optimal_interval_time`.
+    /// * [`GaussObs::realizations_iter`] – On-the-fly noisy realizations for a given triplet.
+    fn compute_triplets(&self, cache: &OutfitCache, params: &IODParams) -> Vec;
+
+    /// Select the interval of observations for RMS calculation.
+    ///
+    /// This function selects the interval of observations for RMS calculation based on the provided triplet.
+    /// It computes the maximum allowed interval and finds the start and end indices of the observations
+    /// within that interval.
+    ///
+    /// Arguments
+    /// ---------
+    /// * `triplets`: A reference to a `GaussObs` representing the triplet of observations.
+    /// * `extf`: A `f64` representing the external factor for the interval calculation.
+    /// * `dtmax`: A `f64` representing the maximum allowed interval.
+    ///
+    /// Return
+    /// ------
+    /// * A `Result` containing a tuple of start and end indices of the observations within the interval,
+    ///   or an `OutfitError` if an error occurs.
+    fn select_rms_interval(
+        &self,
+        triplets: &GaussObs,
+        params: &IODParams,
+    ) -> Result<(usize, usize), OutfitError>;
+
+    /// Evaluate the orbit quality by computing the RMS of normalized astrometric residuals
+    /// over a time window centered on a Gauss triplet.
+    ///
+    /// Scientific context
+    /// -------------------
+    /// This function measures how well a preliminary orbit reproduces the observed
+    /// astrometry (RA, DEC). It computes the **root-mean-square (RMS)** of the
+    /// normalized residuals between predicted and observed positions, aggregated over
+    /// a set of observations surrounding a Gauss triplet.
+    ///
+    /// Interval selection
+    /// -------------------
+    /// The observation arc is defined by:
+    /// * `extf` – fractional extension factor applied around the triplet center,
+    /// * `dtmax` – absolute maximum time span (days) allowed for the arc.
+    ///
+    /// The effective interval is determined by
+    /// [`select_rms_interval`](Self::select_rms_interval), which returns the first
+    /// and last indices of the observations to include.
+    ///
+    /// Computation
+    /// ------------
+    /// * Each observation contributes a squared normalized residual
+    ///   from [`Observation::ephemeris_error`](crate::observations::Observation::ephemeris_error).
+    /// * The final RMS is
+    ///
+    /// ```text
+    /// RMS = √[ (1 / (2N)) · Σᵢ (ΔRAᵢ² + ΔDECᵢ²) ]
+    /// ```
+    ///
+    /// where `N` is the number of observations in the selected interval.
+    ///
+    /// Pruning mode
+    /// ------------
+    /// If `prune_if_rms_ge` is set:
+    /// * The summation stops early once the partial RMS reaches the threshold,
+    ///   returning the pruning value directly.
+    /// * If `prune_if_rms_ge = ∞`, no early exit occurs (equivalent to no pruning).
+    ///
+    /// Arguments
+    /// ----------
+    /// * `state` – Global context providing ephemerides, Earth orientation, and time conversion.
+    /// * `triplets` – The Gauss triplet that defined the preliminary orbit.
+    /// * `orbit_element` – The orbit (in equinoctial elements) to be tested against the arc.
+    /// * `extf` – Fractional time extension of the interval around the triplet.
+    /// * `dtmax` – Maximum arc duration (days).
+    /// * `prune_if_rms_ge` – Optional RMS cutoff for early termination (see *Pruning mode*).
+    ///
+    /// Return
+    /// -------
+    /// * `Ok(rms)` – RMS of the normalized astrometric residuals (radians).
+    /// * `Err(OutfitError)` – If interval selection fails or propagation/ephemeris lookup fails.
+    ///
+    /// Units
+    /// -------
+    /// * The returned RMS is dimensionless but expressed in **radians**.
+    fn rms_orbit_error(
+        &self,
+        cache: &OutfitCache,
+        jpl: &JPLEphem,
+        triplets: &GaussObs,
+        orbit_element: &EquinoctialElements,
+        params: &IODParams,
+        prune_if_rms_ge: Option,
+    ) -> Result;
+
+    /// Estimate the best-fitting preliminary orbit from a full set of astrometric observations.
+    ///
+    /// This method searches for the best preliminary orbit by evaluating a limited number of
+    /// observation triplets generated from the dataset. The process includes:
+    ///
+    /// 1. **Error calibration**:
+    ///    Observations are first preprocessed with [`ObservationsExt::apply_batch_rms_correction`] to account for
+    ///    temporal clustering and observer-specific error models.
+    ///
+    /// 2. **Triplet generation**:
+    ///    Candidate triplets are generated using [`ObservationsExt::compute_triplets`], which:
+    ///      * Sorts observations by time,
+    ///      * Optionally downsamples the dataset to at most `params.max_obs_for_triplets` points
+    ///        (uniform in time, always keeping the first and last),
+    ///      * Filters valid triplets according to `params.dt_min`, `params.dt_max_triplet`,
+    ///        and `params.optimal_interval_time`.
+    ///
+    /// 3. **Monte Carlo noise sampling**:
+    ///    For each triplet, `params.n_noise_realizations` perturbed versions are created using
+    ///    Gaussian noise scaled by `params.noise_scale` times the nominal astrometric uncertainties.
+    ///
+    /// 4. **Orbit estimation and selection**:
+    ///    For each (possibly perturbed) triplet, a preliminary orbit is computed with the Gauss method.
+    ///    The resulting orbit is evaluated over the full set of observations using [`ObservationsExt::rms_orbit_error`].
+    ///    The orbit with the smallest RMS is returned.
+    ///
+    /// # Arguments
+    ///
+    /// * `state` –
+    ///   Global [`Outfit`] state, providing ephemerides and time conversions.
+    /// * `error_model` –
+    ///   The astrometric error model (typically per-band or per-observatory).
+    /// * `rng` –
+    ///   A random number generator used to draw Gaussian perturbations.
+    /// * `params` –
+    ///   Parameters controlling the initial orbit determination, including:
+    ///     * `n_noise_realizations`: number of noisy triplet variants generated per original triplet,
+    ///     * `noise_scale`: scaling factor for the noise,
+    ///     * `extf`: extrapolation factor for RMS evaluation,
+    ///     * `dtmax`: maximum time interval for RMS evaluation,
+    ///     * `dt_min`, `dt_max_triplet`, `optimal_interval_time`: constraints on triplet spans,
+    ///     * `max_obs_for_triplets`: maximum number of observations to keep when building triplets,
+    ///     * `max_triplets`: maximum number of triplets to process,
+    ///     * `gap_max`: maximum allowed time gap within a batch for RMS corrections.
+    ///
+    /// # Returns
+    ///
+    /// * `Ok((Some(best_orbit), best_rms))` – The best preliminary orbit found and its RMS.
+    /// * `Ok((None, f64::MAX))` – No valid orbit could be estimated.
+    /// * `Err(e)` – An error occurred during orbit estimation or RMS evaluation.
+    ///
+    /// # Notes
+    ///
+    /// - RMS values are computed with [`ObservationsExt::rms_orbit_error`], which accounts for
+    ///   light-time correction and ephemeris propagation.
+    /// - Each triplet can produce several preliminary orbit candidates due to
+    ///   noise realizations.
+    /// - The `max_obs_for_triplets` parameter is crucial for large datasets,
+    ///   as it avoids the combinatorial explosion of triplets.
+    ///
+    /// # See also
+    ///
+    /// * [`ObservationsExt::compute_triplets`] – Selects triplets from the observation set.
+    /// * [`GaussObs::generate_noisy_realizations`] – Creates perturbed triplets with Gaussian noise.
+    /// * [`GaussObs::prelim_orbit`] – Computes a preliminary orbit from a single triplet.
+    /// * [`ObservationsExt::rms_orbit_error`] – Measures the goodness-of-fit of an orbit against observations.
+    /// * [`IODParams`] – Configuration options for the IOD process.
+    fn estimate_best_orbit(
+        &self,
+        cache: &OutfitCache,
+        jpl: &JPLEphem,
+        params: &IODParams,
+        rng: &mut impl rand::Rng,
+    ) -> Result<(GaussResult, IODRMS), OutfitError>;
+}
+
+impl TrajectoryFit for Vec<&Observation> {
+    fn extract_errors(&self, idx_obs: Vector3) -> (Vector3, Vector3) {
+        let [i, j, k] = [idx_obs[0], idx_obs[1], idx_obs[2]];
+        let [c1, c2, c3] = [
+            self[i].equ_coord(),
+            self[j].equ_coord(),
+            self[k].equ_coord(),
+        ];
+        (
+            Vector3::new(c1.ra_error, c2.ra_error, c3.ra_error),
+            Vector3::new(c1.dec_error, c2.dec_error, c3.dec_error),
+        )
+    }
+
+    fn compute_triplets(&self, cache: &OutfitCache, params: &IODParams) -> Vec {
+        generate_triplets(self, cache, params)
+    }
+
+    fn select_rms_interval(
+        &self,
+        triplets: &GaussObs,
+        params: &IODParams,
+    ) -> Result<(usize, usize), OutfitError> {
+        let nobs = self.len();
+
+        let idx_obs1 = triplets.idx_obs[0];
+        let obs1 = self
+            .get(idx_obs1)
+            .ok_or(OutfitError::ObservationNotFound(idx_obs1))?;
+
+        let idx_obs3 = triplets.idx_obs[2];
+        let obs3 = self
+            .get(idx_obs3)
+            .ok_or(OutfitError::ObservationNotFound(idx_obs3))?;
+
+        let first_obs = self.first().ok_or(OutfitError::ObservationNotFound(0))?;
+        let last_obs = self
+            .last()
+            .ok_or(OutfitError::ObservationNotFound(nobs - 1))?;
+
+        // Step 1: Compute the maximum allowed interval
+        let mut dt = if params.extf >= 0.0 {
+            (obs3.mjd_tt() - obs1.mjd_tt()) * params.extf
+        } else {
+            10.0 * (last_obs.mjd_tt() - first_obs.mjd_tt())
+        };
+
+        if params.dtmax >= 0.0 {
+            dt = dt.max(params.dtmax);
+        }
+
+        let mut i_start = 0;
+
+        for i in (0..=idx_obs1).rev() {
+            if let Some(obs_i) = self.get(i) {
+                if obs1.mjd_tt() - obs_i.mjd_tt() > dt {
+                    break;
+                }
+                i_start = i;
+            }
+        }
+
+        let mut i_end = nobs - 1;
+
+        for i in idx_obs3..nobs {
+            if let Some(obs_i) = self.get(i) {
+                if obs_i.mjd_tt() - obs3.mjd_tt() > dt {
+                    break;
+                }
+                i_end = i;
+            }
+        }
+
+        Ok((i_start, i_end))
+    }
+
+    fn rms_orbit_error(
+        &self,
+        cache: &OutfitCache,
+        jpl: &JPLEphem,
+        triplets: &GaussObs,
+        orbit_element: &EquinoctialElements,
+        params: &IODParams,
+        prune_if_rms_ge: Option,
+    ) -> Result {
+        // Select the time interval [start_obs_rms, end_obs_rms] over which the RMS
+        // error is evaluated. The interval depends on the triplet and on external
+        // filtering parameters (extf, dtmax).
+        let (start_obs_rms, end_obs_rms) = self.select_rms_interval(triplets, params)?;
+
+        // Number of observations contributing to the RMS
+        let n_obs = (end_obs_rms - start_obs_rms + 1) as f64;
+
+        // Denominator of the RMS formula: here weighted by 2.0 for consistency
+        // with the convention used elsewhere in the code.
+        let denom = 2.0 * n_obs;
+
+        // =========================================================================
+        // Case 1: No pruning → behave like the "classical" RMS definition
+        // =========================================================================
+        if prune_if_rms_ge.is_none() {
+            // Accumulate the squared ephemeris errors for each observation
+            let sum = self[start_obs_rms..=end_obs_rms]
+                .iter()
+                .map(|obs| obs.ephemeris_error(cache, jpl, orbit_element))
+                // try_fold propagates errors from ephemeris_error while summing
+                .try_fold(0.0, |acc, term| term.map(|v| acc + v))?;
+
+            // Final RMS = sqrt( sum / denom )
+            return Ok((sum / denom).sqrt());
+        }
+
+        // =========================================================================
+        // Case 2: Pruning enabled → early stop if RMS exceeds a threshold
+        // =========================================================================
+        let prune = prune_if_rms_ge.unwrap();
+
+        // Convert the RMS cutoff into a sum cutoff:
+        // RMS² = sum / denom  →  stop if sum ≥ (prune² * denom).
+        let sum_cutoff = if prune.is_finite() {
+            prune * prune * denom
+        } else {
+            f64::INFINITY // "no real cutoff" if prune = ∞
+        };
+
+        // Iterate over observations and accumulate squared errors.
+        // We use ControlFlow to allow early exit:
+        //   - Continue(sum): keep summing,
+        //   - Break(value):  stop early and return the pruning threshold.
+        let folded: ControlFlow = self[start_obs_rms..=end_obs_rms]
+            .iter()
+            .map(|obs| obs.ephemeris_error(cache, jpl, orbit_element))
+            .try_fold(0.0, |acc, term| match term {
+                Ok(v) => {
+                    let new_sum = acc + v;
+                    if new_sum >= sum_cutoff {
+                        // Early exit: threshold reached, return directly
+                        ControlFlow::Break(prune)
+                    } else {
+                        ControlFlow::Continue(new_sum)
+                    }
+                }
+                // In case of error in ephemeris_error, also exit with pruning value.
+                Err(_) => ControlFlow::Break(prune),
+            });
+
+        // Final RMS depending on whether we exited early or not
+        match folded {
+            ControlFlow::Continue(sum) => Ok((sum / denom).sqrt()),
+            ControlFlow::Break(rms) => Ok(rms),
+        }
+    }
+
+    fn estimate_best_orbit(
+        &self,
+        cache: &OutfitCache,
+        jpl: &JPLEphem,
+        params: &IODParams,
+        rng: &mut impl rand::Rng,
+    ) -> Result<(GaussResult, IODRMS), OutfitError> {
+        // Placeholder for the actual orbit estimation logic.
+        // This would involve:
+        // 1. Extracting the relevant observations for this trajectory.
+        // 2. Applying the Gauss method to compute the initial orbit.
+        // 3. Calculating the RMS of normalized residuals.
+        // 4. Returning either a successful result or an error.
+
+        let triplets = self.compute_triplets(cache, params);
+
+        if triplets.is_empty() {
+            let span = if self.is_empty() {
+                0.0
+            } else {
+                self.last().unwrap().mjd_tt() - self.first().unwrap().mjd_tt()
+            };
+            return Err(OutfitError::NoFeasibleTriplets {
+                span,
+                n_obs: self.len(),
+                dt_min: params.dt_min,
+                dt_max: params.dt_max_triplet,
+            });
+        }
+
+        // Current best (lowest) RMS and its orbit.
+        // Using +∞ avoids Option branching in the hot path.
+        let mut best_rms = f64::INFINITY;
+        let mut best_orbit: Option = None;
+
+        // Keep the last encountered error so that we can report something meaningful if *all* fail.
+        // We don't clone: we keep only the most recent error by moving it in.
+        let mut last_error: Option = None;
+
+        // For diagnostics, count how many realizations we actually attempted.
+        let mut n_attempts: usize = 0;
+
+        for triplet in triplets {
+            // Extract 1-σ astrometric uncertainties for the three obs of this triplet.
+            let (error_ra, error_dec) = self.extract_errors(triplet.idx_obs);
+
+            // --- Stage 4: For each (lazy) noisy realization of this triplet...
+            // The iterator yields the original triplet first, then noisy copies.
+            for realization in triplet.realizations_iter(
+                &error_ra,
+                &error_dec,
+                params.n_noise_realizations,
+                params.noise_scale,
+                rng,
+            ) {
+                n_attempts += 1;
+
+                // 4.a) Preliminary Gauss solution on the current realization.
+                let gauss_res = match realization.prelim_orbit(params) {
+                    Ok(res) => res,
+                    Err(e) => {
+                        // Record the failure and continue exploring.
+                        last_error = Some(e);
+                        continue;
+                    }
+                };
+
+                // 4.b) Convert to the element set required by the scorer.
+                let equinoctial_elements = gauss_res.get_orbit().to_equinoctial()?;
+
+                // 4.c) Score orbit vs. full observation set (RMS residual).
+                let rms = match self.rms_orbit_error(
+                    cache,
+                    jpl,
+                    &realization,
+                    &equinoctial_elements,
+                    params,
+                    Some(best_rms),
+                ) {
+                    Ok(v) => {
+                        if !v.is_finite() {
+                            last_error = Some(OutfitError::NonFiniteScore(v));
+                            continue;
+                        } else {
+                            v
+                        }
+                    }
+                    Err(e) => {
+                        last_error = Some(e);
+                        continue;
+                    }
+                };
+
+                // 4.d) Keep the best candidate so far.
+                if rms < best_rms {
+                    best_rms = rms;
+                    best_orbit = Some(gauss_res);
+                }
+            }
+        }
+
+        // --- Stage 5: If at least one candidate succeeded, return the best; otherwise, propagate an error.
+        if let Some(orbit) = best_orbit {
+            Ok((orbit, best_rms))
+        } else {
+            // If nothing succeeded, propagate a structured error with the last underlying cause.
+            // Fallback to a domain-specific unit error if we never captured any (e.g., no attempts).
+            let root_cause = match last_error {
+                Some(e) => e,
+                None => panic!("In estimate_best_orbit: no error captured but best_orbit is None, this should not happen"),
+            };
+            Err(OutfitError::NoViableOrbit {
+                cause: Box::new(root_cause),
+                attempts: n_attempts,
+            })
+        }
+    }
+}
+
+#[cfg(test)]
+mod test_obs_ext {
+    use nalgebra::Matrix3;
+    use photom::observer::error_model::{ModelCorrection, ObsErrorModel};
+
+    use crate::{
+        initial_orbit_determination::IODParamsBuilder,
+        orbit_type::orbit_type_test::approx_equal,
+        test_fixture::{DATASET_2015AB, JPL_EPHEM_HORIZON, UT1_PROVIDER},
+        KeplerianElements, OrbitalElements,
+    };
+
+    use approx::assert_relative_eq;
+    use rand::{rngs::StdRng, SeedableRng};
+
+    use super::*;
+
+    #[test]
+    fn test_select_rms_interval() {
+        let traj = DATASET_2015AB
+            .materialize_trajectory("K09R05F")
+            .unwrap()
+            .collect_into_vec();
+        let traj_len = traj.len();
+
+        let cache = OutfitCache::build(&DATASET_2015AB, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap();
+
+        let iod_params = IODParams {
+            dt_min: 0.03,
+            dt_max_triplet: 150.0,
+            optimal_interval_time: 20.0,
+            max_obs_for_triplets: traj_len,
+            max_triplets: 10,
+            extf: -1.0,
+            dtmax: 30.,
+            ..Default::default()
+        };
+
+        let triplets = traj.compute_triplets(&cache, &iod_params);
+        let (u1, u2) = traj
+            .select_rms_interval(triplets.first().unwrap(), &iod_params)
+            .unwrap();
+
+        assert_eq!(u1, 0);
+        assert_eq!(u2, 36);
+
+        let new_params = IODParamsBuilder::from_params(iod_params)
+            .extf(10.)
+            .build()
+            .unwrap();
+
+        let (u1, u2) = traj
+            .select_rms_interval(triplets.first().unwrap(), &new_params)
+            .unwrap();
+
+        assert_eq!(u1, 14);
+        assert_eq!(u2, 36);
+
+        let new_params = IODParamsBuilder::from_params(new_params)
+            .extf(0.001)
+            .dtmax(3.)
+            .build()
+            .unwrap();
+
+        let (u1, u2) = traj
+            .select_rms_interval(triplets.first().unwrap(), &new_params)
+            .unwrap();
+
+        assert_eq!(u1, 17);
+        assert_eq!(u2, 33);
+    }
+
+    #[test]
+    fn test_rms_trajectory() {
+        let iod_params = IODParams {
+            extf: -1.0,
+            dtmax: 30.,
+            ..Default::default()
+        };
+
+        let corrected_dataset = DATASET_2015AB
+            .clone()
+            .with_error_model(ObsErrorModel::FCCT14)
+            .apply_batch_rms_correction(iod_params.gap_max);
+
+        let traj = corrected_dataset
+            .materialize_trajectory("K09R05F")
+            .unwrap()
+            .collect_into_vec();
+
+        let cache =
+            OutfitCache::build(&corrected_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap();
+
+        let triplets = GaussObs {
+            idx_obs: Vector3::new(34, 35, 36),
+            ra: [[
+                1.789_797_623_341_267,
+                1.789_865_909_348_251,
+                1.7899347771316527,
+            ]]
+            .into(),
+            dec: [[
+                0.779_178_052_350_181,
+                0.779_086_664_971_291_9,
+                0.778_996_538_107_973_6,
+            ]]
+            .into(),
+            time: [[
+                57070.238017592594,
+                57_070.250_007_592_59,
+                57070.262067592594,
+            ]]
+            .into(),
+            observer_helio_position: Matrix3::zeros(),
+        };
+
+        let kepler = KeplerianElements {
+            reference_epoch: 57_049.242_334_573_75,
+            semi_major_axis: 1.8017360713154256,
+            eccentricity: 0.283_559_145_668_705_7,
+            inclination: 0.20267383288689386,
+            ascending_node_longitude: 7.955_979_023_693_781E-3,
+            periapsis_argument: 1.2451951387589135,
+            mean_anomaly: 0.44054589015887125,
+        };
+
+        let rms = traj
+            .rms_orbit_error(
+                &cache,
+                &JPL_EPHEM_HORIZON,
+                &triplets,
+                &kepler.into(),
+                &iod_params,
+                None,
+            )
+            .unwrap();
+
+        assert_eq!(rms, 68.88650730830162);
+    }
+
+    mod proptests_extract_errors {
+        use super::*;
+        use photom::{
+            coordinates::equatorial::EquCoord,
+            observation_dataset::{observation::ObservationInput, ObsDataset},
+            observer::dataset::ObserverId,
+            photometry::{Filter, Photometry},
+        };
+        use proptest::prelude::*;
+
+        fn arb_equ_coord() -> impl Strategy {
+            (
+                0.0..(2.0 * std::f64::consts::PI),
+                0.0..0.01f64,
+                (-std::f64::consts::FRAC_PI_2)..std::f64::consts::FRAC_PI_2,
+                0.0..0.01f64,
+            )
+                .prop_map(|(ra, ra_error, dec, dec_error)| EquCoord {
+                    ra,
+                    ra_error,
+                    dec,
+                    dec_error,
+                })
+        }
+
+        fn make_obs_dataset_with_coords(coords: Vec) -> ObsDataset {
+            let inputs: Vec = coords
+                .into_iter()
+                .enumerate()
+                .map(|(i, equ_coord)| {
+                    ObservationInput::new(
+                        i as u64,
+                        equ_coord,
+                        Photometry {
+                            magnitude: 20.0,
+                            error: 0.1,
+                            filter: Filter::Int(0),
+                        },
+                        59000.0,
+                        Some(ObserverId::MpcCode(*b"F51")),
+                    )
+                })
+                .collect();
+
+            ObsDataset::default().push_observation(inputs).unwrap().0
+        }
+
+        proptest! {
+            /// `extract_errors` must return the `ra_error` and `dec_error` of each
+            /// indexed observation, in the correct vector positions.
+            #[test]
+            fn proptest_extract_errors_returns_correct_components(
+                coord0 in arb_equ_coord(),
+                coord1 in arb_equ_coord(),
+                coord2 in arb_equ_coord(),
+            ) {
+                let dataset = make_obs_dataset_with_coords(vec![coord0, coord1, coord2]);
+                let obs: Vec<&Observation> = (0..3)
+                    .map(|i| dataset.get_observation(i).unwrap())
+                    .collect();
+
+                let idx = Vector3::new(0usize, 1, 2);
+                let (ra_errors, dec_errors) = obs.extract_errors(idx);
+
+                prop_assert_eq!(ra_errors[0], coord0.ra_error);
+                prop_assert_eq!(ra_errors[1], coord1.ra_error);
+                prop_assert_eq!(ra_errors[2], coord2.ra_error);
+                prop_assert_eq!(dec_errors[0], coord0.dec_error);
+                prop_assert_eq!(dec_errors[1], coord1.dec_error);
+                prop_assert_eq!(dec_errors[2], coord2.dec_error);
+            }
+
+            /// The index order passed to `extract_errors` must determine which
+            /// observation's error ends up at which vector position.
+            #[test]
+            fn proptest_extract_errors_respects_index_order(
+                coord0 in arb_equ_coord(),
+                coord1 in arb_equ_coord(),
+                coord2 in arb_equ_coord(),
+            ) {
+                let dataset = make_obs_dataset_with_coords(vec![coord0, coord1, coord2]);
+                let obs: Vec<&Observation> = (0..3)
+                    .map(|i| dataset.get_observation(i).unwrap())
+                    .collect();
+
+                // Permuted index: (2, 0, 1)
+                let idx = Vector3::new(2usize, 0, 1);
+                let (ra_errors, dec_errors) = obs.extract_errors(idx);
+
+                prop_assert_eq!(ra_errors[0], coord2.ra_error);
+                prop_assert_eq!(ra_errors[1], coord0.ra_error);
+                prop_assert_eq!(ra_errors[2], coord1.ra_error);
+                prop_assert_eq!(dec_errors[0], coord2.dec_error);
+                prop_assert_eq!(dec_errors[1], coord0.dec_error);
+                prop_assert_eq!(dec_errors[2], coord1.dec_error);
+            }
+        }
+    }
+
+    #[test]
+    fn test_estimate_best_orbit() {
+        let mut rng = StdRng::seed_from_u64(42_u64); // seed for reproducibility
+
+        let iod_params = IODParams::default();
+
+        let corrected_dataset = DATASET_2015AB
+            .clone()
+            .with_error_model(ObsErrorModel::FCCT14)
+            .apply_batch_rms_correction(iod_params.gap_max);
+
+        let traj = corrected_dataset
+            .materialize_trajectory("K09R05F")
+            .unwrap()
+            .collect_into_vec();
+
+        let iod_params = IODParamsBuilder::from_params(iod_params)
+            .n_noise_realizations(5)
+            .max_obs_for_triplets(traj.len())
+            .build()
+            .unwrap();
+
+        let cache =
+            OutfitCache::build(&corrected_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap();
+
+        let (best_orbit, best_rms) = traj
+            .estimate_best_orbit(&cache, &JPL_EPHEM_HORIZON, &iod_params, &mut rng)
+            .unwrap();
+
+        let binding = best_orbit;
+        let orbit = binding.get_orbit();
+
+        let expected_orbit = OrbitalElements::Keplerian(KeplerianElements {
+            reference_epoch: 57049.22904488294,
+            semi_major_axis: 1.801748431600605,
+            eccentricity: 0.283572284127787,
+            inclination: 0.20266779609836036,
+            ascending_node_longitude: 0.008022659889281067,
+            periapsis_argument: 1.245060173584828,
+            mean_anomaly: 0.44047943792316746,
+        });
+
+        assert!(approx_equal(orbit, &expected_orbit, 1e-14));
+        assert_relative_eq!(best_rms, 55.14810894219461, epsilon = 1e-14);
+    }
+}
diff --git a/tests/outfit_struct_test.rs b/tests/outfit_struct_test.rs
deleted file mode 100644
index 2e9c42c..0000000
--- a/tests/outfit_struct_test.rs
+++ /dev/null
@@ -1,18 +0,0 @@
-use outfit::{error_models::ErrorModel, outfit::Outfit};
-
-#[test]
-fn test_outfit_observer_management() {
-    let mut outfit = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
-
-    let obs1 = outfit.new_observer(51.58206, -73.06644, 100., Some("Test Observer 1".into()));
-    assert_eq!(obs1.name, Some("Test Observer 1".to_string()));
-    assert_eq!(obs1.longitude, 51.58206);
-    assert_eq!(obs1.rho_cos_phi, 0.29216347396649495);
-    assert_eq!(obs1.rho_sin_phi, -0.9531782585730825);
-
-    let obs2 = outfit.new_observer(52.58206, 23.4587, 1423., Some("Test Observer 2".into()));
-    assert_eq!(obs2.name, Some("Test Observer 2".to_string()));
-    assert_eq!(obs2.longitude, 52.58206);
-    assert_eq!(obs2.rho_cos_phi, 0.9180389162887692);
-    assert_eq!(obs2.rho_sin_phi, 0.39572170773696747);
-}
diff --git a/tests/reader_80col_test.rs b/tests/reader_80col_test.rs
deleted file mode 100644
index 1582ef6..0000000
--- a/tests/reader_80col_test.rs
+++ /dev/null
@@ -1,57 +0,0 @@
-use camino::Utf8Path;
-use outfit::constants::ObjectNumber;
-use outfit::error_models::ErrorModel;
-use outfit::outfit::Outfit;
-use outfit::trajectories::trajectory_file::TrajectoryFile;
-use outfit::TrajectorySet;
-
-#[test]
-fn test_80col_reader() {
-    let mut env_state = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
-
-    let path_file = Utf8Path::new("tests/data/33803.obs");
-    let mut traj_set = TrajectorySet::new_from_80col(&mut env_state, path_file);
-
-    let obs_33803 = traj_set.get(&ObjectNumber::String("33803".into())).unwrap();
-    assert_eq!(traj_set.len(), 1);
-    assert_eq!(obs_33803.len(), 129);
-    assert_eq!(obs_33803[0].time, 60324.52016874074);
-    assert_eq!(obs_33803[0].ra, 3.5491391785131814);
-    assert_eq!(obs_33803[0].dec, -0.15949710761897423);
-    assert_eq!(
-        obs_33803[0].get_observer(&env_state).name,
-        Some("Mt. Lemmon Survey".to_string())
-    );
-
-    let path_file = Utf8Path::new("tests/data/8467.obs");
-    traj_set.add_from_80col(&mut env_state, path_file);
-    assert_eq!(traj_set.len(), 2);
-    let obs_8467 = traj_set.get(&ObjectNumber::String("8467".into())).unwrap();
-    assert_eq!(obs_8467.len(), 61);
-    assert_eq!(obs_8467[0].time, 60647.053230740734);
-    assert_eq!(obs_8467[0].ra, 0.10365423161131723);
-    assert_eq!(obs_8467[0].dec, 0.1400047372376524);
-    assert_eq!(
-        obs_8467[0].get_observer(&env_state).name,
-        Some("ATLAS Chile, Rio Hurtado".to_string())
-    );
-
-    let path_file = Utf8Path::new("tests/data/K25D50B.obs");
-    traj_set.add_from_80col(&mut env_state, path_file);
-    assert_eq!(traj_set.len(), 3);
-    let obs_k25 = traj_set
-        .get(&ObjectNumber::String("K25D50B".into()))
-        .unwrap();
-    assert_eq!(obs_k25.len(), 20);
-    assert_eq!(obs_k25[0].time, 60732.28129074074);
-    assert_eq!(obs_k25[0].ra, 2.6992652800547146);
-    assert_eq!(obs_k25[0].dec, 0.5231308334332919);
-    assert_eq!(
-        obs_k25[0].get_observer(&env_state).name,
-        Some("Kitt Peak-Bok".to_string())
-    );
-    assert_eq!(
-        obs_k25[19].get_observer(&env_state).name,
-        Some("Steward Observatory, Kitt Peak-Spacewatch".to_string())
-    );
-}
diff --git a/tests/test_gauss_iod.rs b/tests/test_gauss_iod.rs
index fbaec35..c470136 100644
--- a/tests/test_gauss_iod.rs
+++ b/tests/test_gauss_iod.rs
@@ -1,66 +1,62 @@
-#![cfg(feature = "jpl-download")]
-
 mod common;
 
 use approx::assert_relative_eq;
-use camino::Utf8Path;
-use outfit::constants::ObjectNumber;
-use outfit::error_models::ErrorModel;
-use outfit::initial_orbit_determination::gauss_result::GaussResult;
+use hifitime::ut1::Ut1Provider;
 use outfit::initial_orbit_determination::IODParams;
-use outfit::observations::observations_ext::ObservationIOD;
+use outfit::jpl_ephem::download_jpl_file::EphemFileSource;
+use outfit::obs_dataset::FitIOD;
 use outfit::orbit_type::keplerian_element::KeplerianElements;
 use outfit::orbit_type::OrbitalElements;
-use outfit::outfit::Outfit;
-use outfit::outfit_errors::OutfitError;
-use outfit::trajectories::trajectory_file::TrajectoryFile;
-use outfit::TrajectorySet;
+use outfit::JPLEphem;
+use photom::observation_dataset::ObsDataset;
 use rand::rngs::StdRng;
 use rand::SeedableRng;
 
 use crate::common::approx_equal;
 
-fn run_iod(
-    env_state: &mut Outfit,
-    traj_set: &mut TrajectorySet,
-    traj_number: &ObjectNumber,
-) -> Result<(GaussResult, f64), OutfitError> {
-    let obs = traj_set.get_mut(traj_number).unwrap();
-    let mut rng = StdRng::seed_from_u64(42_u64); // seed for reproducibility
-
-    let default = IODParams::builder()
-        .n_noise_realizations(10)
-        .noise_scale(1.1)
-        .max_obs_for_triplets(obs.len())
-        .max_triplets(30)
-        .build()?;
-
-    obs.estimate_best_orbit(env_state, &ErrorModel::FCCT14, &mut rng, &default)
-}
-
 #[test]
 
 fn test_gauss_iod() {
     let test_max_relative = 1e-11;
     let test_epsilon = 1e-11;
 
-    let mut env_state = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
+    let ut1_provider = Ut1Provider::download_from_jpl("latest_eop2.long")
+        .expect("Download of the JPL short time scale UT1 data failed");
 
-    let path_file = Utf8Path::new("tests/data/2015AB.obs");
-    let mut traj_set = TrajectorySet::new_from_80col(&mut env_state, path_file);
+    let jpl_file: EphemFileSource = "naif:DE440"
+        .try_into()
+        .expect("Failed to parse JPL ephemeris source");
+    let jpl_ephem = JPLEphem::new(&jpl_file).expect("Failed to load JPL ephemeris from Naif");
 
-    let path_file = Utf8Path::new("tests/data/8467.obs");
-    traj_set.add_from_80col(&mut env_state, path_file);
+    let (obs_dataset, errors) = ObsDataset::from_mpc_80_col_files(&[
+        "tests/data/2015AB.obs",
+        "tests/data/8467.obs",
+        "tests/data/33803.obs",
+    ]);
 
-    let path_file = Utf8Path::new("tests/data/33803.obs");
-    traj_set.add_from_80col(&mut env_state, path_file);
+    if !errors.is_empty() {
+        panic!("Failed to load observation datasets: {:?}", errors);
+    }
 
-    let (best_orbit, best_rms) = run_iod(
-        &mut env_state,
-        &mut traj_set,
-        &ObjectNumber::String("K09R05F".into()),
-    )
-    .unwrap();
+    let default = IODParams::builder()
+        .n_noise_realizations(10)
+        .noise_scale(1.1)
+        .max_obs_for_triplets(130) // number of observation for the largest trajectory in the dataset
+        .max_triplets(30)
+        .build()
+        .unwrap();
+
+    let mut full_orbit = obs_dataset
+        .fit_full_iod(
+            &jpl_ephem,
+            &ut1_provider,
+            &default,
+            &mut StdRng::seed_from_u64(42),
+        )
+        .unwrap();
+
+    let (best_orbit, best_rms) = full_orbit.remove(&"K09R05F".into()).unwrap().unwrap();
+    let orbit = best_orbit.get_orbit();
 
     let expected_orbit = OrbitalElements::Keplerian(KeplerianElements {
         reference_epoch: 57049.22904452732,
@@ -72,8 +68,6 @@ fn test_gauss_iod() {
         mean_anomaly: 0.44069989140091426,
     });
 
-    let orbit = best_orbit.get_orbit();
-
     assert!(approx_equal(&expected_orbit, orbit, test_epsilon));
     assert_relative_eq!(
         best_rms,
@@ -82,13 +76,6 @@ fn test_gauss_iod() {
         max_relative = test_max_relative
     );
 
-    let (best_orbit, best_rms) = run_iod(
-        &mut env_state,
-        &mut traj_set,
-        &ObjectNumber::String("8467".into()),
-    )
-    .unwrap();
-
     let expected_orbit = OrbitalElements::Keplerian(KeplerianElements {
         reference_epoch: 60672.24113100201,
         semi_major_axis: 3.189546977249391,
@@ -99,6 +86,7 @@ fn test_gauss_iod() {
         mean_anomaly: 4.85070383704545,
     });
 
+    let (best_orbit, best_rms) = full_orbit.remove(&"8467".into()).unwrap().unwrap();
     let orbit = best_orbit.get_orbit();
 
     assert!(approx_equal(&expected_orbit, orbit, test_epsilon));
@@ -109,13 +97,6 @@ fn test_gauss_iod() {
         max_relative = test_max_relative
     );
 
-    let (best_orbit, best_rms) = run_iod(
-        &mut env_state,
-        &mut traj_set,
-        &ObjectNumber::String("33803".into()),
-    )
-    .unwrap();
-
     let expected_orbit = OrbitalElements::Keplerian(KeplerianElements {
         reference_epoch: 60465.26778016307,
         semi_major_axis: 2.192136202201971,
@@ -126,6 +107,7 @@ fn test_gauss_iod() {
         mean_anomaly: 4.9466622638827324,
     });
 
+    let (best_orbit, best_rms) = full_orbit.remove(&"33803".into()).unwrap().unwrap();
     let orbit = best_orbit.get_orbit();
 
     assert!(approx_equal(&expected_orbit, orbit, test_epsilon));
diff --git a/tests/test_read_ades.rs b/tests/test_read_ades.rs
deleted file mode 100644
index 32d9d32..0000000
--- a/tests/test_read_ades.rs
+++ /dev/null
@@ -1,56 +0,0 @@
-use camino::Utf8Path;
-use outfit::constants::ObjectNumber;
-use outfit::error_models::ErrorModel;
-use outfit::outfit::Outfit;
-use outfit::trajectories::trajectory_file::TrajectoryFile;
-use outfit::TrajectorySet;
-
-#[test]
-fn test_read_ades() {
-    let mut outfit = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
-
-    let mut traj_set = TrajectorySet::new_from_ades(
-        &mut outfit,
-        Utf8Path::new("tests/data/example_ades.xml"),
-        None,
-        None,
-    );
-    assert_eq!(traj_set.len(), 4);
-    assert_eq!(traj_set.get(&ObjectNumber::Int(1234457)).unwrap().len(), 1);
-
-    traj_set.add_from_ades(
-        &mut outfit,
-        Utf8Path::new("tests/data/example_ades2.xml"),
-        None,
-        None,
-    );
-
-    assert_eq!(traj_set.len(), 7);
-    let traj = traj_set
-        .get(&ObjectNumber::String("2016 RD34".into()))
-        .unwrap();
-    assert_eq!(traj.len(), 2);
-    let obs = traj.first().unwrap().get_observer(&outfit);
-    assert_eq!(
-        *obs.name.as_ref().unwrap(),
-        "University of Hawaii 88-inch telescope, Maunakea".to_string()
-    );
-
-    traj_set.add_from_ades(
-        &mut outfit,
-        Utf8Path::new("tests/data/flat_ades.xml"),
-        None,
-        None,
-    );
-    assert_eq!(traj_set.len(), 41);
-
-    let traj = traj_set
-        .get(&ObjectNumber::String("D/1993 F2-W".into()))
-        .unwrap();
-
-    assert_eq!(traj.len(), 1);
-    assert_eq!(
-        traj.first().unwrap().get_observer(&outfit).name,
-        Some("La Palma".into())
-    );
-}

From 7b935f7d15f613a6a6a5e8c9393817756648684a Mon Sep 17 00:00:00 2001
From: Roman 
Date: Thu, 30 Apr 2026 09:20:50 +0200
Subject: [PATCH 02/47] fix some tests

---
 src/cache/observer_centric_cache.rs | 11 +++++++++--
 src/cache/observer_fixed_cache.rs   |  1 +
 src/jpl_ephem/download_jpl_file.rs  | 16 ----------------
 3 files changed, 10 insertions(+), 18 deletions(-)

diff --git a/src/cache/observer_centric_cache.rs b/src/cache/observer_centric_cache.rs
index aa48a9a..cc4375f 100644
--- a/src/cache/observer_centric_cache.rs
+++ b/src/cache/observer_centric_cache.rs
@@ -154,8 +154,15 @@ mod observer_test {
 
     #[test]
     fn test_helio_pos_obs() {
-        let (lon, lat, h) = (203.744090000, 20.707233557, 3067.694);
-        let pan_starrs = to_observer(lon, lat, h, Some("Pan-STARRS 1".to_string()), None, None);
+        let (lon, lat, h) = (203.744090000_f64, 20.707233557_f64, 3067.694_f64);
+        let pan_starrs = to_observer(
+            lon.to_radians(),
+            lat.to_radians(),
+            h,
+            Some("Pan-STARRS 1".to_string()),
+            None,
+            None,
+        );
         let observer_fixed_cache: ObserverFixedCache = (&pan_starrs).try_into().unwrap();
 
         let cases = [
diff --git a/src/cache/observer_fixed_cache.rs b/src/cache/observer_fixed_cache.rs
index 09b1664..16dc251 100644
--- a/src/cache/observer_fixed_cache.rs
+++ b/src/cache/observer_fixed_cache.rs
@@ -13,6 +13,7 @@ pub type ObserverFixedPosition = Vector3>;
 /// Precomputed **body-fixed** velocity of the observer in **AU/day**.
 pub type ObserverFixedVelocity = Vector3>;
 
+#[derive(Debug)]
 pub struct ObserverFixedCache {
     observer_fixed_positions: ObserverFixedPosition,
     observer_fixed_velocities: ObserverFixedVelocity,
diff --git a/src/jpl_ephem/download_jpl_file.rs b/src/jpl_ephem/download_jpl_file.rs
index 8e14321..fceac47 100644
--- a/src/jpl_ephem/download_jpl_file.rs
+++ b/src/jpl_ephem/download_jpl_file.rs
@@ -380,19 +380,3 @@ impl TryFrom for EphemFilePath {
         }
     }
 }
-
-#[cfg(test)]
-mod jpl_reader_test {
-    /// If `jpl-download` is **not** enabled, requesting a missing file must error.
-    #[test]
-    fn test_no_feature_download_jpl_ephem() {
-        use super::*;
-        let file_source = "naif:DE442".try_into().unwrap();
-
-        let result = EphemFilePath::get_ephemeris_file(&file_source);
-        assert!(
-            result.is_err(),
-            "feature jpl-download is enabled, weird ..."
-        );
-    }
-}

From 6090998210e793d155586ce495698269c905e4d6 Mon Sep 17 00:00:00 2001
From: Roman 
Date: Fri, 1 May 2026 09:09:50 +0200
Subject: [PATCH 03/47] change rms and estimate_best_orbit tests according to
 the changes when parsing the astrometric error from a 80 column MPC file made
 in the photom crate

---
 src/obs_dataset.rs           |  2 ++
 src/observation_ephemeris.rs | 34 +++++++++++++++++++++++++---------
 src/trajectory.rs            | 28 +++++++++++++++++-----------
 3 files changed, 44 insertions(+), 20 deletions(-)

diff --git a/src/obs_dataset.rs b/src/obs_dataset.rs
index 74aa411..bb9a538 100644
--- a/src/obs_dataset.rs
+++ b/src/obs_dataset.rs
@@ -10,6 +10,8 @@ use crate::{
     cache::OutfitCache, trajectory::TrajectoryFit, GaussResult, IODParams, JPLEphem, OutfitError,
 };
 
+/// Type alias for the RMS of normalized residuals from an IOD fit.
+/// This is a single scalar value representing the overall fit quality of the IOD solution.
 pub type IODRMS = f64;
 
 /// Full batch orbit determination results.
diff --git a/src/observation_ephemeris.rs b/src/observation_ephemeris.rs
index 824ed13..aa93df8 100644
--- a/src/observation_ephemeris.rs
+++ b/src/observation_ephemeris.rs
@@ -672,6 +672,7 @@ mod test_observations_ephemeris {
             dec_error: f64,
             t_obs: f64,
             mpc_code: MpcCode,
+            apply_model_errors: bool,
         ) -> (ObsDataset, OutfitCache) {
             let observation_input = ObservationInput::new(
                 0,
@@ -694,8 +695,13 @@ mod test_observations_ephemeris {
                 .push_observation(vec![observation_input])
                 .unwrap()
                 .0
-                .with_error_model(ObsErrorModel::FCCT14)
-                .apply_model_errors();
+                .with_error_model(ObsErrorModel::FCCT14);
+
+            let obs_dataset = if apply_model_errors {
+                obs_dataset.apply_model_errors()
+            } else {
+                obs_dataset
+            };
 
             let cache =
                 OutfitCache::build(&obs_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap();
@@ -750,6 +756,7 @@ mod test_observations_ephemeris {
                 1.259_582_891_829_317_7E-6,
                 57070.262067592594,
                 *b"F51",
+                false,
             );
 
             let equinoctial_element = EquinoctialElements {
@@ -773,7 +780,7 @@ mod test_observations_ephemeris {
             let equinoctial = simple_equinoctial(t_obs);
 
             let (obs_dataset, cache) =
-                make_obs_dataset_and_cache_mpc(0.0, 1e-6, 0.0, 1e-6, t_obs, *b"F51");
+                make_obs_dataset_and_cache_mpc(0.0, 1e-6, 0.0, 1e-6, t_obs, *b"F51", true);
 
             let obs = obs_dataset.get_observation(0).unwrap();
             let (alpha, delta) = obs
@@ -781,7 +788,7 @@ mod test_observations_ephemeris {
                 .unwrap();
 
             let (obs_dataset_match, cache_match) =
-                make_obs_dataset_and_cache_mpc(alpha, 1e-6, delta, 1e-6, t_obs, *b"F51");
+                make_obs_dataset_and_cache_mpc(alpha, 1e-6, delta, 1e-6, t_obs, *b"F51", true);
 
             let obs_match = obs_dataset_match.get_observation(0).unwrap();
             let error = obs_match
@@ -797,15 +804,22 @@ mod test_observations_ephemeris {
             let equinoctial = simple_equinoctial(t_obs);
 
             let (obs_dataset, cache) =
-                make_obs_dataset_and_cache_mpc(0.0, 1e-3, 0.0, 1e-3, t_obs, *b"F51");
+                make_obs_dataset_and_cache_mpc(0.0, 1e-3, 0.0, 1e-3, t_obs, *b"F51", true);
 
             let obs = obs_dataset.get_observation(0).unwrap();
             let (alpha, delta) = obs
                 .compute_apparent_position(&cache, &JPL_EPHEM_HORIZON, &equinoctial)
                 .unwrap();
 
-            let (obs_dataset_offset, cache_offset) =
-                make_obs_dataset_and_cache_mpc(alpha + 1e-3, 1e-3, delta, 1e-3, t_obs, *b"F51");
+            let (obs_dataset_offset, cache_offset) = make_obs_dataset_and_cache_mpc(
+                alpha + 1e-3,
+                1e-3,
+                delta,
+                1e-3,
+                t_obs,
+                *b"F51",
+                true,
+            );
 
             let obs_offset = obs_dataset_offset.get_observation(0).unwrap();
             let err = obs_offset
@@ -821,7 +835,7 @@ mod test_observations_ephemeris {
             let equinoctial = simple_equinoctial(t_obs);
 
             let (obs_dataset, cache) =
-                make_obs_dataset_and_cache_mpc(0.0, 1e-6, 0.0, 1e-6, t_obs, *b"F51");
+                make_obs_dataset_and_cache_mpc(0.0, 1e-6, 0.0, 1e-6, t_obs, *b"F51", true);
 
             let obs = obs_dataset.get_observation(0).unwrap();
             let (alpha, delta) = obs
@@ -835,6 +849,7 @@ mod test_observations_ephemeris {
                 1e-6,
                 t_obs,
                 *b"F51",
+                true,
             );
 
             let obs_wrapped = obs_dataset_wrapped.get_observation(0).unwrap();
@@ -851,7 +866,7 @@ mod test_observations_ephemeris {
             let equinoctial = simple_equinoctial(t_obs);
 
             let (obs_dataset, cache) =
-                make_obs_dataset_and_cache_mpc(0.0, 1.0, 0.0, 1.0, t_obs, *b"F51");
+                make_obs_dataset_and_cache_mpc(0.0, 1.0, 0.0, 1.0, t_obs, *b"F51", true);
 
             let obs = obs_dataset.get_observation(0).unwrap();
             let (alpha, delta) = obs
@@ -865,6 +880,7 @@ mod test_observations_ephemeris {
                 10.0,
                 t_obs,
                 *b"F51",
+                true,
             );
 
             let obs_large = obs_dataset_large.get_observation(0).unwrap();
diff --git a/src/trajectory.rs b/src/trajectory.rs
index bea91cf..d471376 100644
--- a/src/trajectory.rs
+++ b/src/trajectory.rs
@@ -542,13 +542,19 @@ mod test_obs_ext {
 
     #[test]
     fn test_select_rms_interval() {
-        let traj = DATASET_2015AB
+        let corrected_dataset = DATASET_2015AB
+            .clone()
+            .with_error_model(ObsErrorModel::FCCT14)
+            .apply_model_errors();
+
+        let traj = corrected_dataset
             .materialize_trajectory("K09R05F")
             .unwrap()
             .collect_into_vec();
         let traj_len = traj.len();
 
-        let cache = OutfitCache::build(&DATASET_2015AB, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap();
+        let cache =
+            OutfitCache::build(&corrected_dataset, &JPL_EPHEM_HORIZON, &UT1_PROVIDER).unwrap();
 
         let iod_params = IODParams {
             dt_min: 0.03,
@@ -660,7 +666,7 @@ mod test_obs_ext {
             )
             .unwrap();
 
-        assert_eq!(rms, 68.88650730830162);
+        assert_eq!(rms, 153.84607281520138);
     }
 
     mod proptests_extract_errors {
@@ -795,16 +801,16 @@ mod test_obs_ext {
         let orbit = binding.get_orbit();
 
         let expected_orbit = OrbitalElements::Keplerian(KeplerianElements {
-            reference_epoch: 57049.22904488294,
-            semi_major_axis: 1.801748431600605,
-            eccentricity: 0.283572284127787,
-            inclination: 0.20266779609836036,
-            ascending_node_longitude: 0.008022659889281067,
-            periapsis_argument: 1.245060173584828,
-            mean_anomaly: 0.44047943792316746,
+            reference_epoch: 57049.22904475403,
+            semi_major_axis: 1.8017609974509807,
+            eccentricity: 0.2835733667643381,
+            inclination: 0.20267686119302475,
+            ascending_node_longitude: 0.00799201841873464,
+            periapsis_argument: 1.245034216916367,
+            mean_anomaly: 0.4405089048961484,
         });
 
         assert!(approx_equal(orbit, &expected_orbit, 1e-14));
-        assert_relative_eq!(best_rms, 55.14810894219461, epsilon = 1e-14);
+        assert_relative_eq!(best_rms, 222.16583195747745, epsilon = 1e-14);
     }
 }

From 040a53cea4233d6a5c2e7cd0ee912e33d79f506c Mon Sep 17 00:00:00 2001
From: Roman 
Date: Tue, 19 May 2026 09:24:43 +0200
Subject: [PATCH 04/47] derive debug for cache structures, fix non-determinism
 for full iod with rng per traj, fix inconsistency index due to a sort by time
 in the apply_batch_rms_correction method within the photom crate

---
 Cargo.toml                          |   1 +
 src/cache/mod.rs                    |   1 +
 src/cache/observer_centric_cache.rs |   1 +
 src/constants.rs                    |   7 ++
 src/obs_dataset.rs                  |  36 ++++++++--
 src/observer_extension.rs           |   2 +-
 tests/test_cache_consistency.rs     | 107 ++++++++++++++++++++++++++++
 tests/test_gauss_iod.rs             |  59 +++++++--------
 8 files changed, 177 insertions(+), 37 deletions(-)
 create mode 100644 tests/test_cache_consistency.rs

diff --git a/Cargo.toml b/Cargo.toml
index 150d3bb..8d94981 100644
--- a/Cargo.toml
+++ b/Cargo.toml
@@ -54,6 +54,7 @@ roots = { version = "0.0.8", default-features = false }
 rand = { version = "0.9.2", default-features = false, features = [
     "std_rng",
     "os_rng",
+    "small_rng"
 ] }
 rand_distr = { version = "0.5.1", default-features = false }
 
diff --git a/src/cache/mod.rs b/src/cache/mod.rs
index 345c720..2110e15 100644
--- a/src/cache/mod.rs
+++ b/src/cache/mod.rs
@@ -22,6 +22,7 @@ use crate::{
 /// Built once before any trajectory fitting. Each entry is keyed by the
 /// observation's [`ObsIndex`], which is stable for the lifetime of the
 /// [`ObsDataset`].
+#[derive(Debug)]
 pub struct OutfitCache {
     /// len == number of observations in the dataset. Indexed by [`ObsIndex`].
     observer_centric: CentricObserverCache,
diff --git a/src/cache/observer_centric_cache.rs b/src/cache/observer_centric_cache.rs
index cc4375f..feee960 100644
--- a/src/cache/observer_centric_cache.rs
+++ b/src/cache/observer_centric_cache.rs
@@ -17,6 +17,7 @@ pub type ObserverGeocentricVelocity = Vector3>;
 pub type ObserverHeliocentricPosition = Vector3>;
 
 /// Geocentric and heliocentric observer positions for a single observation epoch.
+#[derive(Debug)]
 pub struct ObserverCentricCache {
     pub geo_position: ObserverGeocentricPosition,
     pub geo_velocity: ObserverGeocentricVelocity,
diff --git a/src/constants.rs b/src/constants.rs
index 1e81aff..820a71d 100644
--- a/src/constants.rs
+++ b/src/constants.rs
@@ -75,10 +75,15 @@ pub const VLIGHT_AU: f64 = VLIGHT / AU * SECONDS_PER_DAY;
 // Angular velocity of Earth rotation (rad/day) on the z-axis.
 pub const EARTH_ROTATION: Vector3 = Vector3::new(0.0, 0.0, DPI * 1.00273790934);
 
+/// Hard coded rotation matrices for coordinate transformations between mean equatorial J2000 and mean ecliptic J2000 frames.
+/// Can be computed using the rotpn function in the ref_system module
+
 /// Rotation matrix from mean equatorial J2000 to mean ecliptic J2000.
 ///
 /// Rotation of $-\varepsilon$ around the X-axis, where $\varepsilon$ is the
 /// obliquity of the ecliptic at J2000.
+/// 
+/// call rotpn(RefSystem::Equm(RefEpoch::J2000), RefSystem::Eclm(RefEpoch::J2000)) for same computed result
 pub const ROT_EQUMJ2000_TO_ECLMJ2000: Matrix3 = Matrix3::new(
     1.00000000000000000e0,
     0.00000000000000000e0,
@@ -94,6 +99,8 @@ pub const ROT_EQUMJ2000_TO_ECLMJ2000: Matrix3 = Matrix3::new(
 /// Rotation matrix from mean ecliptic J2000 to mean equatorial J2000.
 ///
 /// Transpose (inverse) of [`ROT_EQUMJ2000_TO_ECLMJ2000`].
+/// 
+/// call rotpn(RefSystem::Eclm(RefEpoch::J2000), RefSystem::Equm(RefEpoch::J2000)) for same computed result
 pub const ROT_ECLMJ2000_TO_EQUMJ2000: Matrix3 = Matrix3::new(
     1.00000000000000000e0,
     0.00000000000000000e0,
diff --git a/src/obs_dataset.rs b/src/obs_dataset.rs
index bb9a538..8892dca 100644
--- a/src/obs_dataset.rs
+++ b/src/obs_dataset.rs
@@ -2,9 +2,10 @@ use ahash::AHashMap;
 use hifitime::ut1::Ut1Provider;
 use photom::{
     observation_dataset::{observation::Observation, ObsDataset},
-    observer::error_model::ModelCorrection,
+    observer::error_model::{ModelCorrection, ObsErrorModel},
     TrajId,
 };
+use rand::{rngs::SmallRng, SeedableRng};
 
 use crate::{
     cache::OutfitCache, trajectory::TrajectoryFit, GaussResult, IODParams, JPLEphem, OutfitError,
@@ -37,6 +38,7 @@ pub trait FitIOD {
         jpl: &JPLEphem,
         ut1_provider: &Ut1Provider,
         params: &IODParams,
+        error_model: ObsErrorModel,
         rng: &mut impl rand::Rng,
     ) -> Result;
 
@@ -46,6 +48,7 @@ pub trait FitIOD {
         jpl: &JPLEphem,
         ut1_provider: &Ut1Provider,
         params: &IODParams,
+        error_model: ObsErrorModel,
         rng: &mut impl rand::Rng,
     ) -> Result<(GaussResult, IODRMS), OutfitError>;
 }
@@ -57,10 +60,11 @@ impl FitIOD for ObsDataset {
         jpl: &JPLEphem,
         ut1_provider: &Ut1Provider,
         params: &IODParams,
+        error_model: ObsErrorModel,
         rng: &mut impl rand::Rng,
     ) -> Result<(GaussResult, IODRMS), OutfitError> {
         let corrected_dataset = self
-            .apply_model_errors()
+            .with_error_model(error_model)
             .apply_batch_rms_correction(params.gap_max);
 
         let cache = OutfitCache::build(&corrected_dataset, jpl, ut1_provider)?;
@@ -73,22 +77,40 @@ impl FitIOD for ObsDataset {
         jpl: &JPLEphem,
         ut1_provider: &Ut1Provider,
         params: &IODParams,
+        error_model: ObsErrorModel,
         rng: &mut impl rand::Rng,
     ) -> Result {
         let corrected_dataset = self
+            .with_error_model(error_model)
             .apply_model_errors()
             .apply_batch_rms_correction(params.gap_max);
 
         let cache = OutfitCache::build(&corrected_dataset, jpl, ut1_provider)?;
 
+        // Draw a single base seed from the caller's RNG.
+        // All per-trajectory RNGs are derived from this seed → deterministic
+        // regardless of trajectory ordering or parallelism.
+        let base_seed: u64 = rng.random();
+
         let results: FullOrbitResult = corrected_dataset
             .iter_traj_id()
             .into_iter()
             .flatten()
-            .map(|traj| {
-                println!("Fitting IOD for Trajectory ID: {}", traj);
-                let result = fit_single_traj(traj, &corrected_dataset, &cache, jpl, params, rng);
-                (traj.clone(), result)
+            .map(|traj_id| {
+                // Derive a per-trajectory seed from the base seed and the trajectory ID.
+                // Two trajectories with different IDs always get independent sequences.
+                let traj_seed = base_seed ^ traj_id.stable_hash();
+                let mut local_rng = SmallRng::seed_from_u64(traj_seed);
+
+                let result = fit_single_traj(
+                    &traj_id,
+                    &corrected_dataset,
+                    &cache,
+                    jpl,
+                    params,
+                    &mut local_rng,
+                );
+                (traj_id.clone(), result)
             })
             .collect();
 
@@ -108,7 +130,7 @@ fn fit_single_traj(
         .materialize_trajectory(traj)
         .ok_or_else(|| OutfitError::TrajectoryIdNotFound(traj.clone()))?;
 
-    let mut obs_vec_refs: Vec<&Observation> = materialized_traj.iter().collect();
+    let mut obs_vec_refs: Vec<&Observation> = materialized_traj.collect_into_vec();
     obs_vec_refs.sort_by(|a, b| a.mjd_tt().total_cmp(&b.mjd_tt()));
 
     obs_vec_refs.estimate_best_orbit(cache, jpl, params, rng)
diff --git a/src/observer_extension.rs b/src/observer_extension.rs
index ad6329b..17cdaea 100644
--- a/src/observer_extension.rs
+++ b/src/observer_extension.rs
@@ -18,7 +18,7 @@ use crate::{
     JPLEphem, OutfitError,
 };
 
-pub(crate) trait ResolvedObserver {
+pub trait ResolvedObserver {
     /// Get the fixed position of an observatory using its geographic coordinates
     ///
     /// Return
diff --git a/tests/test_cache_consistency.rs b/tests/test_cache_consistency.rs
new file mode 100644
index 0000000..c91ac24
--- /dev/null
+++ b/tests/test_cache_consistency.rs
@@ -0,0 +1,107 @@
+use approx::assert_abs_diff_eq;
+use camino::Utf8Path;
+use hifitime::ut1::Ut1Provider;
+use nalgebra::Vector3;
+use outfit::{
+    cache::OutfitCache, jpl_ephem::download_jpl_file::EphemFileSource, IODParams, JPLEphem,
+};
+use photom::{
+    observation_dataset::ObsDataset,
+    observer::error_model::{ModelCorrection, ObsErrorModel},
+};
+
+const POSITION_EPSILON: f64 = 1e-12;
+
+struct CacheFixture {
+    ut1_provider: Ut1Provider,
+    jpl_ephem: JPLEphem,
+    default_params: IODParams,
+}
+
+impl CacheFixture {
+    fn new() -> Self {
+        let ut1_provider = Ut1Provider::download_from_jpl("latest_eop2.long")
+            .expect("Download of the JPL short time scale UT1 data failed");
+
+        let jpl_file: EphemFileSource = "horizon:DE440"
+            .try_into()
+            .expect("Failed to parse JPL ephemeris source");
+        let jpl_ephem =
+            JPLEphem::new(&jpl_file).expect("Failed to load JPL ephemeris from Horizon");
+
+        Self {
+            ut1_provider,
+            jpl_ephem,
+            default_params: IODParams::default(),
+        }
+    }
+
+    fn build_cache>(&self, paths: &[P]) -> (OutfitCache, ObsDataset) {
+        let (obs_dataset, _) = ObsDataset::from_mpc_80_col_files(paths);
+
+        let obs_dataset = obs_dataset
+            .with_error_model(ObsErrorModel::FCCT14)
+            .apply_batch_rms_correction(self.default_params.gap_max);
+
+        let cache = OutfitCache::build(&obs_dataset, &self.jpl_ephem, &self.ut1_provider)
+            .expect("Failed to build outfit cache");
+
+        (cache, obs_dataset)
+    }
+}
+
+fn assert_helio_position(cache: &OutfitCache, obs_dataset: &ObsDataset, trajectory_id: &str) {
+    let traj = obs_dataset
+        .materialize_trajectory(trajectory_id)
+        .unwrap()
+        .collect_into_vec();
+
+    let checks: &[(usize, [f64; 3])] = &[
+        (
+            0,
+            [0.996798968524259, -0.12232935537370689, -0.0530044254994447],
+        ),
+        (
+            traj.len() / 2,
+            [-0.2588304494454786, 0.8703635675926336, 0.3773300400916685],
+        ),
+        (
+            traj.len() - 1,
+            [-0.8383497659757538, 0.479843435538848, 0.20801659206288547],
+        ),
+    ];
+
+    for (idx, expected) in checks {
+        let obs = &traj[*idx];
+        let helio_pos = cache
+            .get_centric(obs.index())
+            .helio_position
+            .map(|x| x.into_inner());
+
+        assert_abs_diff_eq!(
+            helio_pos,
+            Vector3::from(*expected),
+            epsilon = POSITION_EPSILON
+        );
+    }
+}
+
+#[test]
+fn test_cache_consistency() {
+    let fixture = CacheFixture::new();
+
+    let dataset_combinations: &[&[&str]] = &[
+        &["tests/data/2015AB.obs"],
+        &["tests/data/8467.obs", "tests/data/2015AB.obs"],
+        &[
+            "tests/data/2015AB.obs",
+            "tests/data/8467.obs",
+            "tests/data/33803.obs",
+        ],
+    ];
+
+    for paths in dataset_combinations {
+        let (cache, obs_dataset) = fixture.build_cache(paths);
+        assert_helio_position(&cache, &obs_dataset, "K09R05F");
+    }
+}
diff --git a/tests/test_gauss_iod.rs b/tests/test_gauss_iod.rs
index c470136..4cd9885 100644
--- a/tests/test_gauss_iod.rs
+++ b/tests/test_gauss_iod.rs
@@ -9,13 +9,13 @@ use outfit::orbit_type::keplerian_element::KeplerianElements;
 use outfit::orbit_type::OrbitalElements;
 use outfit::JPLEphem;
 use photom::observation_dataset::ObsDataset;
+use photom::observer::error_model::ObsErrorModel;
 use rand::rngs::StdRng;
 use rand::SeedableRng;
 
 use crate::common::approx_equal;
 
 #[test]
-
 fn test_gauss_iod() {
     let test_max_relative = 1e-11;
     let test_epsilon = 1e-11;
@@ -23,10 +23,10 @@ fn test_gauss_iod() {
     let ut1_provider = Ut1Provider::download_from_jpl("latest_eop2.long")
         .expect("Download of the JPL short time scale UT1 data failed");
 
-    let jpl_file: EphemFileSource = "naif:DE440"
+    let jpl_file: EphemFileSource = "horizon:DE440"
         .try_into()
         .expect("Failed to parse JPL ephemeris source");
-    let jpl_ephem = JPLEphem::new(&jpl_file).expect("Failed to load JPL ephemeris from Naif");
+    let jpl_ephem = JPLEphem::new(&jpl_file).expect("Failed to load JPL ephemeris from Horizon");
 
     let (obs_dataset, errors) = ObsDataset::from_mpc_80_col_files(&[
         "tests/data/2015AB.obs",
@@ -51,6 +51,7 @@ fn test_gauss_iod() {
             &jpl_ephem,
             &ut1_provider,
             &default,
+            ObsErrorModel::FCCT14,
             &mut StdRng::seed_from_u64(42),
         )
         .unwrap();
@@ -59,61 +60,61 @@ fn test_gauss_iod() {
     let orbit = best_orbit.get_orbit();
 
     let expected_orbit = OrbitalElements::Keplerian(KeplerianElements {
-        reference_epoch: 57049.22904452732,
-        semi_major_axis: 1.8017634341924542,
-        eccentricity: 0.28360400982137396,
-        inclination: 0.20267485730439427,
-        ascending_node_longitude: 0.00810182022710516,
-        periapsis_argument: 1.2445523487100616,
-        mean_anomaly: 0.44069989140091426,
+        reference_epoch: 57049.2684537375,
+        semi_major_axis: 1.801740835743616,
+        eccentricity: 0.28356259478492557,
+        inclination: 0.2026828189979528,
+        ascending_node_longitude: 0.007951791820548622,
+        periapsis_argument: 1.2450647642587158,
+        mean_anomaly: 0.4408048786626789,
     });
 
     assert!(approx_equal(&expected_orbit, orbit, test_epsilon));
     assert_relative_eq!(
         best_rms,
-        47.67954270293223,
+        66.97479288637471,
         epsilon = test_epsilon,
         max_relative = test_max_relative
     );
 
     let expected_orbit = OrbitalElements::Keplerian(KeplerianElements {
-        reference_epoch: 60672.24113100201,
-        semi_major_axis: 3.189546977249391,
-        eccentricity: 0.05434034666134485,
-        inclination: 0.18343383575588465,
-        ascending_node_longitude: 0.03253594968161228,
-        periapsis_argument: 2.0197545218038355,
-        mean_anomaly: 4.85070383704545,
+        reference_epoch: 60672.2443617134,
+        semi_major_axis: 3.2199380906809876,
+        eccentricity: 0.0624192099888107,
+        inclination: 0.1829771029880289,
+        ascending_node_longitude: 0.030775930195064964,
+        periapsis_argument: 1.9053705720223801,
+        mean_anomaly: 4.980622835177979,
     });
 
-    let (best_orbit, best_rms) = full_orbit.remove(&"8467".into()).unwrap().unwrap();
+    let (best_orbit, best_rms) = full_orbit.remove(&8467_u32.into()).unwrap().unwrap();
     let orbit = best_orbit.get_orbit();
 
     assert!(approx_equal(&expected_orbit, orbit, test_epsilon));
     assert_relative_eq!(
         best_rms,
-        0.550927559734816,
+        0.5739558189489471,
         epsilon = test_epsilon,
         max_relative = test_max_relative
     );
 
     let expected_orbit = OrbitalElements::Keplerian(KeplerianElements {
-        reference_epoch: 60465.26778016307,
-        semi_major_axis: 2.192136202201971,
-        eccentricity: 0.2042936374305811,
-        inclination: 0.1189651192106584,
-        ascending_node_longitude: 3.091130251223283,
-        periapsis_argument: 2.4714439663661487,
-        mean_anomaly: 4.9466622638827324,
+        reference_epoch: 60465.26777915681,
+        semi_major_axis: 2.1874983804796972,
+        eccentricity: 0.20256414489486008,
+        inclination: 0.11906245183260411,
+        ascending_node_longitude: 3.0918063960305293,
+        periapsis_argument: 2.4793248309745692,
+        mean_anomaly: 4.934465465531324,
     });
 
-    let (best_orbit, best_rms) = full_orbit.remove(&"33803".into()).unwrap().unwrap();
+    let (best_orbit, best_rms) = full_orbit.remove(&33803_u32.into()).unwrap().unwrap();
     let orbit = best_orbit.get_orbit();
 
     assert!(approx_equal(&expected_orbit, orbit, test_epsilon));
     assert_relative_eq!(
         best_rms,
-        6.319395085728921,
+        18.963755528781288,
         epsilon = test_epsilon,
         max_relative = test_max_relative
     );

From 9b8319442c2ccc6d1026786f869815e547b98965 Mon Sep 17 00:00:00 2001
From: Roman 
Date: Tue, 19 May 2026 15:27:02 +0200
Subject: [PATCH 05/47] remove old benchs and examples, add new tests from
 parquet file to orbit

---
 Cargo.lock                             | 2057 +++++++++++++++++++-----
 Cargo.toml                             |   69 +-
 benches/gauss_prelim_orbit.rs          |  148 --
 benches/load_parquet.rs                |   54 -
 benches/outfit_gauss_iod.rs            |  122 --
 benches/solve_kepler_equation.rs       |  161 --
 examples/gauss_iod_once.rs             |   95 --
 examples/parquet_to_orbit.rs           |  659 --------
 src/initial_orbit_determination/mod.rs |   26 -
 src/outfit_errors.rs                   |    4 -
 tests/data/test_data_traj_str.parquet  |  Bin 0 -> 19876139 bytes
 tests/test_iod_from_polars.rs          |  144 ++
 tests/trajectories_from_parquet.rs     |   69 -
 tests/trajectories_from_vec.rs         |   68 -
 tests/vec_to_iod.rs                    |  281 ----
 15 files changed, 1848 insertions(+), 2109 deletions(-)
 delete mode 100644 benches/gauss_prelim_orbit.rs
 delete mode 100644 benches/load_parquet.rs
 delete mode 100644 benches/outfit_gauss_iod.rs
 delete mode 100644 benches/solve_kepler_equation.rs
 delete mode 100644 examples/gauss_iod_once.rs
 delete mode 100644 examples/parquet_to_orbit.rs
 create mode 100644 tests/data/test_data_traj_str.parquet
 create mode 100644 tests/test_iod_from_polars.rs
 delete mode 100644 tests/trajectories_from_parquet.rs
 delete mode 100644 tests/trajectories_from_vec.rs
 delete mode 100644 tests/vec_to_iod.rs

diff --git a/Cargo.lock b/Cargo.lock
index 781cb90..9ad6768 100644
--- a/Cargo.lock
+++ b/Cargo.lock
@@ -35,8 +35,6 @@ source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "5a15f179cd60c4584b8a8c596927aadc462e27f2ca70c04e0071964a73ba7a75"
 dependencies = [
  "cfg-if",
- "const-random",
- "getrandom 0.3.4",
  "once_cell",
  "version_check",
  "zerocopy",
@@ -51,6 +49,33 @@ dependencies = [
  "memchr",
 ]
 
+[[package]]
+name = "alloc-no-stdlib"
+version = "2.0.4"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "cc7bb162ec39d46ab1ca8c77bf72e890535becd1751bb45f64c597edb4c8c6b3"
+
+[[package]]
+name = "alloc-stdlib"
+version = "0.2.2"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "94fb8275041c72129eb51b7d0322c29b8387a0386127718b096429201a5d6ece"
+dependencies = [
+ "alloc-no-stdlib",
+]
+
+[[package]]
+name = "allocator-api2"
+version = "0.2.21"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "683d7910e743518b0e34f1186f92494becacb047c7b6bf616c96772180fef923"
+
+[[package]]
+name = "android-tzdata"
+version = "0.1.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "e999941b234f3131b00bc13c22d06e8c5ff726d1b6318ac7eb276997bbb4fef0"
+
 [[package]]
 name = "android_system_properties"
 version = "0.1.5"
@@ -88,110 +113,94 @@ dependencies = [
 ]
 
 [[package]]
-name = "arrayvec"
-version = "0.7.6"
+name = "ar_archive_writer"
+version = "0.5.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "7c02d123df017efcdfbd739ef81735b36c5ba83ec3c59c80a9d7ecc718f92e50"
+checksum = "7eb93bbb63b9c227414f6eb3a0adfddca591a8ce1e9b60661bb08969b87e340b"
+dependencies = [
+ "object",
+]
 
 [[package]]
-name = "arrow-array"
-version = "54.3.1"
+name = "argminmax"
+version = "0.6.3"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "a12fcdb3f1d03f69d3ec26ac67645a8fe3f878d77b5ebb0b15d64a116c212985"
+checksum = "70f13d10a41ac8d2ec79ee34178d61e6f47a29c2edfe7ef1721c7383b0359e65"
 dependencies = [
- "ahash",
- "arrow-buffer",
- "arrow-data",
- "arrow-schema",
- "chrono",
  "half",
- "hashbrown 0.15.5",
- "num",
+ "num-traits",
 ]
 
 [[package]]
-name = "arrow-buffer"
-version = "54.3.1"
+name = "array-init-cursor"
+version = "0.2.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "263f4801ff1839ef53ebd06f99a56cecd1dbaf314ec893d93168e2e860e0291c"
-dependencies = [
- "bytes",
- "half",
- "num",
-]
+checksum = "ed51fe0f224d1d4ea768be38c51f9f831dee9d05c163c11fba0b8c44387b1fc3"
 
 [[package]]
-name = "arrow-cast"
-version = "54.3.1"
+name = "arrayref"
+version = "0.3.9"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "ede6175fbc039dfc946a61c1b6d42fd682fcecf5ab5d148fbe7667705798cac9"
-dependencies = [
- "arrow-array",
- "arrow-buffer",
- "arrow-data",
- "arrow-schema",
- "arrow-select",
- "atoi",
- "base64",
- "chrono",
- "half",
- "lexical-core",
- "num",
- "ryu",
-]
+checksum = "76a2e8124351fda1ef8aaaa3bbd7ebbcb486bbcd4225aca0aa0d84bb2db8fecb"
+
+[[package]]
+name = "arrayvec"
+version = "0.7.6"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "7c02d123df017efcdfbd739ef81735b36c5ba83ec3c59c80a9d7ecc718f92e50"
 
 [[package]]
-name = "arrow-data"
-version = "54.3.1"
+name = "async-channel"
+version = "2.5.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "61cfdd7d99b4ff618f167e548b2411e5dd2c98c0ddebedd7df433d34c20a4429"
+checksum = "924ed96dd52d1b75e9c1a3e6275715fd320f5f9439fb5a4a11fa51f4221158d2"
 dependencies = [
- "arrow-buffer",
- "arrow-schema",
- "half",
- "num",
+ "concurrent-queue",
+ "event-listener-strategy",
+ "futures-core",
+ "pin-project-lite",
 ]
 
 [[package]]
-name = "arrow-ipc"
-version = "54.3.1"
+name = "async-stream"
+version = "0.3.6"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "62ff528658b521e33905334723b795ee56b393dbe9cf76c8b1f64b648c65a60c"
+checksum = "0b5a71a6f37880a80d1d7f19efd781e4b5de42c88f0722cc13bcb6cc2cfe8476"
 dependencies = [
- "arrow-array",
- "arrow-buffer",
- "arrow-data",
- "arrow-schema",
- "flatbuffers",
+ "async-stream-impl",
+ "futures-core",
+ "pin-project-lite",
 ]
 
 [[package]]
-name = "arrow-schema"
-version = "54.3.1"
+name = "async-stream-impl"
+version = "0.3.6"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "39cfaf5e440be44db5413b75b72c2a87c1f8f0627117d110264048f2969b99e9"
+checksum = "c7c24de15d275a1ecfd47a380fb4d5ec9bfe0933f309ed5e705b775596a3574d"
+dependencies = [
+ "proc-macro2",
+ "quote",
+ "syn",
+]
 
 [[package]]
-name = "arrow-select"
-version = "54.3.1"
+name = "async-trait"
+version = "0.1.89"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "69efcd706420e52cd44f5c4358d279801993846d1c2a8e52111853d61d55a619"
+checksum = "9035ad2d096bed7955a320ee7e2230574d28fd3c3a0f186cbea1ff3c7eed5dbb"
 dependencies = [
- "ahash",
- "arrow-array",
- "arrow-buffer",
- "arrow-data",
- "arrow-schema",
- "num",
+ "proc-macro2",
+ "quote",
+ "syn",
 ]
 
 [[package]]
-name = "atoi"
-version = "2.0.0"
+name = "atoi_simd"
+version = "0.17.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "f28d99ec8bfea296261ca1af174f24225171fea9664ba9003cbebee704810528"
+checksum = "8ad17c7c205c2c28b527b9845eeb91cf1b4d008b438f98ce0e628227a822758e"
 dependencies = [
- "num-traits",
+ "debug_unsafe",
 ]
 
 [[package]]
@@ -218,7 +227,7 @@ dependencies = [
  "miniz_oxide",
  "object",
  "rustc-demangle",
- "windows-link",
+ "windows-link 0.2.1",
 ]
 
 [[package]]
@@ -227,6 +236,26 @@ version = "0.22.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "72b3254f16251a8381aa12e40e3c4d2f0199f8c6508fbecb9d91f575e0fbb8c6"
 
+[[package]]
+name = "bincode"
+version = "2.0.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "36eaf5d7b090263e8150820482d5d93cd964a81e4019913c972f4edcc6edb740"
+dependencies = [
+ "bincode_derive",
+ "serde",
+ "unty",
+]
+
+[[package]]
+name = "bincode_derive"
+version = "2.0.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "bf95709a440f45e986983918d0e8a1f30a9b1df04918fc828670606804ac3c09"
+dependencies = [
+ "virtue",
+]
+
 [[package]]
 name = "bit-set"
 version = "0.8.0"
@@ -244,15 +273,62 @@ checksum = "5e764a1d40d510daf35e07be9eb06e75770908c27d411ee6c92109c9840eaaf7"
 
 [[package]]
 name = "bitflags"
-version = "1.3.2"
+version = "2.11.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "bef38d45163c2f1dde094a7dfd33ccf595c92905c8f8f4fdc18d06fb1037718a"
+checksum = "c4512299f36f043ab09a583e57bceb5a5aab7a73db1805848e8fef3c9e8c78b3"
+dependencies = [
+ "serde_core",
+]
 
 [[package]]
-name = "bitflags"
-version = "2.11.1"
+name = "blake3"
+version = "1.8.5"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "c4512299f36f043ab09a583e57bceb5a5aab7a73db1805848e8fef3c9e8c78b3"
+checksum = "0aa83c34e62843d924f905e0f5c866eb1dd6545fc4d719e803d9ba6030371fce"
+dependencies = [
+ "arrayref",
+ "arrayvec",
+ "cc",
+ "cfg-if",
+ "constant_time_eq",
+ "cpufeatures 0.3.0",
+]
+
+[[package]]
+name = "block-buffer"
+version = "0.10.4"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "3078c7629b62d3f0439517fa394996acacc5cbc91c5a20d8c658e77abd503a71"
+dependencies = [
+ "generic-array",
+]
+
+[[package]]
+name = "boxcar"
+version = "0.2.14"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "36f64beae40a84da1b4b26ff2761a5b895c12adc41dc25aaee1c4f2bbfe97a6e"
+
+[[package]]
+name = "brotli"
+version = "8.0.2"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "4bd8b9603c7aa97359dbd97ecf258968c95f3adddd6db2f7e7a5bef101c84560"
+dependencies = [
+ "alloc-no-stdlib",
+ "alloc-stdlib",
+ "brotli-decompressor",
+]
+
+[[package]]
+name = "brotli-decompressor"
+version = "5.0.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "874bb8112abecc98cbd6d81ea4fa7e94fb9449648c93cc89aa40c81c24d7de03"
+dependencies = [
+ "alloc-no-stdlib",
+ "alloc-stdlib",
+]
 
 [[package]]
 name = "bumpalo"
@@ -271,18 +347,29 @@ name = "bytemuck"
 version = "1.25.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "c8efb64bd706a16a1bdde310ae86b351e4d21550d98d056f22f8a7f7a2183fec"
+dependencies = [
+ "bytemuck_derive",
+]
 
 [[package]]
-name = "byteorder"
-version = "1.5.0"
+name = "bytemuck_derive"
+version = "1.10.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "1fd0f2584146f6f2ef48085050886acf353beff7305ebd1ae69500e27c67f64b"
+checksum = "f9abbd1bc6865053c427f7198e6af43bfdedc55ab791faed4fbd361d789575ff"
+dependencies = [
+ "proc-macro2",
+ "quote",
+ "syn",
+]
 
 [[package]]
 name = "bytes"
 version = "1.11.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "1e748733b7cbc798e1434b6ac524f0c1ff2ab456fe201501e6497c8417a4fc33"
+dependencies = [
+ "serde",
+]
 
 [[package]]
 name = "camino"
@@ -296,13 +383,24 @@ version = "0.3.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "37b2a672a2cb129a2e41c10b1224bb368f9f37a2b16b612598138befd7b37eb5"
 
+[[package]]
+name = "castaway"
+version = "0.2.4"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "dec551ab6e7578819132c713a93c022a05d60159dc86e7a7050223577484c55a"
+dependencies = [
+ "rustversion",
+]
+
 [[package]]
 name = "cc"
-version = "1.2.60"
+version = "1.2.62"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "43c5703da9466b66a946814e1adf53ea2c90f10063b86290cc9eb67ce3478a20"
+checksum = "a1dce859f0832a7d088c4f1119888ab94ef4b5d6795d1ce05afb7fe159d79f98"
 dependencies = [
  "find-msvc-tools",
+ "jobserver",
+ "libc",
  "shlex",
 ]
 
@@ -318,15 +416,38 @@ version = "0.2.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "613afe47fcd5fac7ccf1db93babcb082c5994d996f20b8b159f2ad1658eb5724"
 
+[[package]]
+name = "chacha20"
+version = "0.10.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "6f8d983286843e49675a4b7a2d174efe136dc93a18d69130dd18198a6c167601"
+dependencies = [
+ "cfg-if",
+ "cpufeatures 0.3.0",
+ "rand_core 0.10.1",
+]
+
 [[package]]
 name = "chrono"
-version = "0.4.44"
+version = "0.4.41"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "c673075a2e0e5f4a1dde27ce9dee1ea4558c7ffe648f576438a20ca1d2acc4b0"
+checksum = "c469d952047f47f91b68d1cba3f10d63c11d73e4636f24f08daf0278abf01c4d"
 dependencies = [
+ "android-tzdata",
  "iana-time-zone",
  "num-traits",
- "windows-link",
+ "serde",
+ "windows-link 0.1.3",
+]
+
+[[package]]
+name = "chrono-tz"
+version = "0.10.4"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "a6139a8597ed92cf816dfb33f5dd6cf0bb93a6adc938f11039f371bc5bcd26c3"
+dependencies = [
+ "chrono",
+ "phf",
 ]
 
 [[package]]
@@ -387,39 +508,49 @@ version = "7.2.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "958c5d6ecf1f214b4c2bbbbf6ab9523a864bd136dcf71a7e8904799acfe1ad47"
 dependencies = [
+ "crossterm",
  "unicode-segmentation",
  "unicode-width",
 ]
 
 [[package]]
-name = "console"
-version = "0.16.3"
+name = "compact_str"
+version = "0.9.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "d64e8af5551369d19cf50138de61f1c42074ab970f74e99be916646777f8fc87"
+checksum = "3fdb1325a1cece981e8a296ab8f0f9b63ae357bd0784a9faaf548cc7b480707a"
 dependencies = [
- "encode_unicode",
- "libc",
- "windows-sys 0.61.2",
+ "castaway",
+ "cfg-if",
+ "itoa",
+ "rustversion",
+ "ryu",
+ "serde",
+ "static_assertions",
 ]
 
 [[package]]
-name = "const-random"
-version = "0.1.18"
+name = "concurrent-queue"
+version = "2.5.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "87e00182fe74b066627d63b85fd550ac2998d4b0bd86bfed477a0ae4c7c71359"
+checksum = "4ca0197aee26d1ae37445ee532fefce43251d24cc7c166799f4d46817f1d3973"
 dependencies = [
- "const-random-macro",
+ "crossbeam-utils",
 ]
 
 [[package]]
-name = "const-random-macro"
-version = "0.1.16"
+name = "constant_time_eq"
+version = "0.4.2"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "3d52eff69cd5e647efe296129160853a42795992097e8af39800e1060caeea9b"
+
+[[package]]
+name = "core-foundation"
+version = "0.10.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "f9d839f2a20b0aee515dc581a6172f2321f96cab76c1a38a4c584a194955390e"
+checksum = "b2a6cd9ae233e7f62ba4e9353e81a88df7fc8a5987b8d445b4d90c879bd156f6"
 dependencies = [
- "getrandom 0.2.17",
- "once_cell",
- "tiny-keccak",
+ "core-foundation-sys",
+ "libc",
 ]
 
 [[package]]
@@ -428,6 +559,33 @@ version = "0.8.7"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "773648b94d0e5d620f64f280777445740e61fe701025087ec8b57f45c791888b"
 
+[[package]]
+name = "cpufeatures"
+version = "0.2.17"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "59ed5838eebb26a2bb2e58f6d5b5316989ae9d08bab10e0e6d103e656d1b0280"
+dependencies = [
+ "libc",
+]
+
+[[package]]
+name = "cpufeatures"
+version = "0.3.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "8b2a41393f66f16b0823bb79094d54ac5fbd34ab292ddafb9a0456ac9f87d201"
+dependencies = [
+ "libc",
+]
+
+[[package]]
+name = "crc32fast"
+version = "1.5.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "9481c1c90cbf2ac953f07c8d4a58aa3945c425b7185c9154d67a65e4230da511"
+dependencies = [
+ "cfg-if",
+]
+
 [[package]]
 name = "criterion"
 version = "0.5.1"
@@ -464,6 +622,15 @@ dependencies = [
  "itertools 0.10.5",
 ]
 
+[[package]]
+name = "crossbeam-channel"
+version = "0.5.15"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "82b8f8f868b36967f9606790d1903570de9ceaf870a7bf9fbbd3016d636a2cb2"
+dependencies = [
+ "crossbeam-utils",
+]
+
 [[package]]
 name = "crossbeam-deque"
 version = "0.8.6"
@@ -483,18 +650,76 @@ dependencies = [
  "crossbeam-utils",
 ]
 
+[[package]]
+name = "crossbeam-queue"
+version = "0.3.12"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "0f58bbc28f91df819d0aa2a2c00cd19754769c2fad90579b3592b1c9ba7a3115"
+dependencies = [
+ "crossbeam-utils",
+]
+
 [[package]]
 name = "crossbeam-utils"
 version = "0.8.21"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "d0a5c400df2834b80a4c3327b3aad3a4c4cd4de0629063962b03235697506a28"
 
+[[package]]
+name = "crossterm"
+version = "0.29.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "d8b9f2e4c67f833b660cdb0a3523065869fb35570177239812ed4c905aeff87b"
+dependencies = [
+ "bitflags",
+ "crossterm_winapi",
+ "document-features",
+ "parking_lot",
+ "rustix",
+ "winapi",
+]
+
+[[package]]
+name = "crossterm_winapi"
+version = "0.9.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "acdd7c62a3665c7f6830a51635d9ac9b23ed385797f70a83bb8bafe9c572ab2b"
+dependencies = [
+ "winapi",
+]
+
 [[package]]
 name = "crunchy"
 version = "0.2.4"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "460fbee9c2c2f33933d720630a6a0bac33ba7053db5344fac858d4b8952d77d5"
 
+[[package]]
+name = "crypto-common"
+version = "0.1.7"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "78c8292055d1c1df0cce5d180393dc8cce0abec0a7102adb6c7b1eef6016d60a"
+dependencies = [
+ "generic-array",
+ "typenum",
+]
+
+[[package]]
+name = "debug_unsafe"
+version = "0.1.4"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "7eed2c4702fa172d1ce21078faa7c5203e69f5394d48cc436d25928394a867a2"
+
+[[package]]
+name = "digest"
+version = "0.10.7"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "9ed9a281f7bc9b7576e61468ba615a66a5c8cfdff42420a70aa82701a3b1e292"
+dependencies = [
+ "block-buffer",
+ "crypto-common",
+]
+
 [[package]]
 name = "directories"
 version = "6.0.0"
@@ -528,16 +753,25 @@ dependencies = [
 ]
 
 [[package]]
-name = "either"
-version = "1.15.0"
+name = "document-features"
+version = "0.2.12"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "48c757948c5ede0e46177b7add2e67155f70e33c07fea8284df6576da70b3719"
+checksum = "d4b8a88685455ed29a21542a33abd9cb6510b6b129abadabdcef0f4c55bc8f61"
+dependencies = [
+ "litrs",
+]
 
 [[package]]
-name = "encode_unicode"
-version = "1.0.0"
+name = "dyn-clone"
+version = "1.0.20"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "34aa73646ffb006b8f5147f3dc182bd4bcb190227ce861fc4a4844bf8e3cb2c0"
+checksum = "d0881ea181b1df73ff77ffaaf9c7544ecc11e82fba9b5f27b262a3c73a332555"
+
+[[package]]
+name = "either"
+version = "1.15.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "48c757948c5ede0e46177b7add2e67155f70e33c07fea8284df6576da70b3719"
 
 [[package]]
 name = "equivalent"
@@ -556,41 +790,87 @@ dependencies = [
 ]
 
 [[package]]
-name = "fastrand"
-version = "2.4.1"
+name = "ethnum"
+version = "1.5.3"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "9f1f227452a390804cdb637b74a86990f2a7d7ba4b7d5693aac9b4dd6defd8d6"
+checksum = "40404c3f5f511ec4da6fe866ddf6a717c309fdbb69fbbad7b0f3edab8f2e835f"
 
 [[package]]
-name = "find-msvc-tools"
-version = "0.1.9"
+name = "event-listener"
+version = "5.4.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "5baebc0774151f905a1a2cc41989300b1e6fbb29aff0ceffa1064fdd3088d582"
+checksum = "e13b66accf52311f30a0db42147dadea9850cb48cd070028831ae5f5d4b856ab"
+dependencies = [
+ "concurrent-queue",
+ "parking",
+ "pin-project-lite",
+]
 
 [[package]]
-name = "flatbuffers"
-version = "24.12.23"
+name = "event-listener-strategy"
+version = "0.5.4"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "4f1baf0dbf96932ec9a3038d57900329c015b0bfb7b63d904f3bc27e2b02a096"
+checksum = "8be9f3dfaaffdae2972880079a491a1a8bb7cbed0b8dd7a347f668b4150a3b93"
 dependencies = [
- "bitflags 1.3.2",
- "rustc_version",
+ "event-listener",
+ "pin-project-lite",
 ]
 
 [[package]]
-name = "fnv"
-version = "1.0.7"
+name = "fallible-streaming-iterator"
+version = "0.1.9"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "3f9eec918d3f24069decb9af1554cad7c880e2da24a9afd88aca000531ab82c1"
+checksum = "7360491ce676a36bf9bb3c56c1aa791658183a54d2744120f27285738d90465a"
 
 [[package]]
-name = "foldhash"
-version = "0.1.5"
+name = "fast-float2"
+version = "0.2.3"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "d9c4f5dac5e15c24eb999c26181a6ca40b39fe946cbe4c263c7209467bc83af2"
+checksum = "f8eb564c5c7423d25c886fb561d1e4ee69f72354d16918afa32c08811f6b6a55"
 
 [[package]]
-name = "form_urlencoded"
+name = "fastrand"
+version = "2.4.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "9f1f227452a390804cdb637b74a86990f2a7d7ba4b7d5693aac9b4dd6defd8d6"
+
+[[package]]
+name = "find-msvc-tools"
+version = "0.1.9"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "5baebc0774151f905a1a2cc41989300b1e6fbb29aff0ceffa1064fdd3088d582"
+
+[[package]]
+name = "flate2"
+version = "1.1.9"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "843fba2746e448b37e26a819579957415c8cef339bf08564fe8b7ddbd959573c"
+dependencies = [
+ "crc32fast",
+ "miniz_oxide",
+ "zlib-rs",
+]
+
+[[package]]
+name = "fnv"
+version = "1.0.7"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "3f9eec918d3f24069decb9af1554cad7c880e2da24a9afd88aca000531ab82c1"
+
+[[package]]
+name = "foldhash"
+version = "0.1.5"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "d9c4f5dac5e15c24eb999c26181a6ca40b39fe946cbe4c263c7209467bc83af2"
+
+[[package]]
+name = "foldhash"
+version = "0.2.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "77ce24cb58228fbb8aa041425bb1050850ac19177686ea6e0f41a70416f56fdb"
+
+[[package]]
+name = "form_urlencoded"
 version = "1.2.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "cb4cb245038516f5f85277875cdaa4f7d2c9a0fa0468de06ed190163b1581fcf"
@@ -598,6 +878,31 @@ dependencies = [
  "percent-encoding",
 ]
 
+[[package]]
+name = "fs4"
+version = "0.13.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "8640e34b88f7652208ce9e88b1a37a2ae95227d84abec377ccd3c5cfeb141ed4"
+dependencies = [
+ "rustix",
+ "windows-sys 0.59.0",
+]
+
+[[package]]
+name = "futures"
+version = "0.3.32"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "8b147ee9d1f6d097cef9ce628cd2ee62288d963e16fb287bd9286455b241382d"
+dependencies = [
+ "futures-channel",
+ "futures-core",
+ "futures-executor",
+ "futures-io",
+ "futures-sink",
+ "futures-task",
+ "futures-util",
+]
+
 [[package]]
 name = "futures-channel"
 version = "0.3.32"
@@ -605,6 +910,7 @@ source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "07bbe89c50d7a535e539b8c17bc0b49bdb77747034daa8087407d655f3f7cc1d"
 dependencies = [
  "futures-core",
+ "futures-sink",
 ]
 
 [[package]]
@@ -613,6 +919,17 @@ version = "0.3.32"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "7e3450815272ef58cec6d564423f6e755e25379b217b0bc688e295ba24df6b1d"
 
+[[package]]
+name = "futures-executor"
+version = "0.3.32"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "baf29c38818342a3b26b5b923639e7b1f4a61fc5e76102d4b1981c6dc7a7579d"
+dependencies = [
+ "futures-core",
+ "futures-task",
+ "futures-util",
+]
+
 [[package]]
 name = "futures-io"
 version = "0.3.32"
@@ -648,6 +965,7 @@ version = "0.3.32"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "389ca41296e6190b48053de0321d02a77f32f8a5d2461dd38762c0593805c6d6"
 dependencies = [
+ "futures-channel",
  "futures-core",
  "futures-io",
  "futures-macro",
@@ -658,6 +976,16 @@ dependencies = [
  "slab",
 ]
 
+[[package]]
+name = "generic-array"
+version = "0.14.7"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "85649ca51fd72272d7821adaf274ad91c288277713d9c18820d8499a7ff69e9a"
+dependencies = [
+ "typenum",
+ "version_check",
+]
+
 [[package]]
 name = "getrandom"
 version = "0.2.17"
@@ -694,6 +1022,7 @@ dependencies = [
  "cfg-if",
  "libc",
  "r-efi 6.0.0",
+ "rand_core 0.10.1",
  "wasip2",
  "wasip3",
 ]
@@ -704,11 +1033,17 @@ version = "0.32.3"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "e629b9b98ef3dd8afe6ca2bd0f89306cec16d43d907889945bc5d6687f2f13c7"
 
+[[package]]
+name = "glob"
+version = "0.3.3"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "0cc23270f6e1808e30a928bdc84dea0b9b4136a8bc82338574f23baf47bbd280"
+
 [[package]]
 name = "h2"
-version = "0.4.13"
+version = "0.4.14"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "2f44da3a8150a6703ed5d34e164b875fd14c2cdab9af1252a9a1020bde2bdc54"
+checksum = "171fefbc92fe4a4de27e0698d6a5b392d6a0e333506bc49133760b3bcf948733"
 dependencies = [
  "atomic-waker",
  "bytes",
@@ -729,9 +1064,11 @@ version = "2.7.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "6ea2d84b969582b4b1864a92dc5d27cd2b77b622a8d79306834f1be5ba20d84b"
 dependencies = [
+ "bytemuck",
  "cfg-if",
  "crunchy",
  "num-traits",
+ "serde",
  "zerocopy",
 ]
 
@@ -741,14 +1078,30 @@ version = "0.15.5"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "9229cfe53dfd69f0609a49f65461bd93001ea1ef889cd5529dd176593f5338a1"
 dependencies = [
- "foldhash",
+ "allocator-api2",
+ "equivalent",
+ "foldhash 0.1.5",
+]
+
+[[package]]
+name = "hashbrown"
+version = "0.16.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "841d1cc9bed7f9236f321df977030373f4a4163ae1a7dbfe1a51a2c1a51d9100"
+dependencies = [
+ "allocator-api2",
+ "equivalent",
+ "foldhash 0.2.0",
+ "rayon",
+ "serde",
+ "serde_core",
 ]
 
 [[package]]
 name = "hashbrown"
-version = "0.17.0"
+version = "0.17.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "4f467dd6dccf739c208452f8014c75c18bb8301b050ad1cfb27153803edb0f51"
+checksum = "ed5909b6e89a2db4456e54cd5f673791d7eca6732202bbf2a9cc504fe2f9b84a"
 
 [[package]]
 name = "heck"
@@ -762,11 +1115,17 @@ version = "0.5.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "fc0fef456e4baa96da950455cd02c081ca953b141298e41db3fc7e36b1da849c"
 
+[[package]]
+name = "hex"
+version = "0.4.3"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "7f24254aa9a54b5c858eaee2f5bccdb46aaf0e486a595ed5fd8f86ba55232a70"
+
 [[package]]
 name = "hifitime"
-version = "4.2.6"
+version = "4.3.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "22f1dfc1be6cd1c3a44704db0a8800aa53ebb07a9509535a0261cd387eedee7c"
+checksum = "a978b79fb40cea4c6592890ffe0021dfea5c51a107fbac565abae82fd24a15af"
 dependencies = [
  "js-sys",
  "lexical-core",
@@ -781,6 +1140,15 @@ dependencies = [
  "web-time",
 ]
 
+[[package]]
+name = "home"
+version = "0.5.12"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "cc627f471c528ff0c4a49e1d5e60450c8f6461dd6d10ba9dcd3a61d3dff7728d"
+dependencies = [
+ "windows-sys 0.61.2",
+]
+
 [[package]]
 name = "http"
 version = "1.4.0"
@@ -820,6 +1188,12 @@ version = "1.10.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "6dbf3de79e51f3d586ab4cb9d5c3e2c14aa28ed23d180cf89b4df0454a69cc87"
 
+[[package]]
+name = "humantime"
+version = "2.3.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "135b12329e5e3ce057a9f972339ea52bc954fe1e9358ef27f95e89716fbc5424"
+
 [[package]]
 name = "husky-rs"
 version = "0.1.5"
@@ -857,6 +1231,7 @@ dependencies = [
  "hyper",
  "hyper-util",
  "rustls",
+ "rustls-native-certs",
  "tokio",
  "tokio-rustls",
  "tower-service",
@@ -1011,9 +1386,9 @@ dependencies = [
 
 [[package]]
 name = "idna_adapter"
-version = "1.2.1"
+version = "1.2.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "3acae9609540aa318d1bc588455225fb2085b9ed0c4f6bd0d9d5bcd86f1a0344"
+checksum = "cb68373c0d6620ef8105e855e7745e18b0d00d3bdb07fb532e434244cdb9a714"
 dependencies = [
  "icu_normalizer",
  "icu_properties",
@@ -1026,44 +1401,17 @@ source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "d466e9454f08e4a911e14806c24e16fba1b4c121d1ea474396f396069cf949d9"
 dependencies = [
  "equivalent",
- "hashbrown 0.17.0",
+ "hashbrown 0.17.1",
  "serde",
  "serde_core",
 ]
 
-[[package]]
-name = "indicatif"
-version = "0.18.4"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "25470f23803092da7d239834776d653104d551bc4d7eacaf31e6837854b8e9eb"
-dependencies = [
- "console",
- "portable-atomic",
- "unit-prefix",
-]
-
-[[package]]
-name = "integer-encoding"
-version = "3.0.4"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "8bb03732005da905c88227371639bf1ad885cc712789c011c31c5fb3ab3ccf02"
-
 [[package]]
 name = "ipnet"
 version = "2.12.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "d98f6fed1fde3f8c21bc40a1abb88dd75e67924f9cffc3ef95607bad8017f8e2"
 
-[[package]]
-name = "iri-string"
-version = "0.7.12"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "25e659a4bb38e810ebc252e53b5814ff908a8c58c2a9ce2fae1bbec24cbf4e20"
-dependencies = [
- "memchr",
- "serde",
-]
-
 [[package]]
 name = "is-terminal"
 version = "0.4.17"
@@ -1099,11 +1447,21 @@ version = "1.0.18"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "8f42a60cbdf9a97f5d2305f08a87dc4e09308d1276d28c869c684d7777685682"
 
+[[package]]
+name = "jobserver"
+version = "0.1.34"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "9afb3de4395d6b3e67a780b6de64b51c978ecf11cb9a462c66be7d4ca9039d33"
+dependencies = [
+ "getrandom 0.3.4",
+ "libc",
+]
+
 [[package]]
 name = "js-sys"
-version = "0.3.95"
+version = "0.3.98"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "2964e92d1d9dc3364cae4d718d93f227e3abb088e747d92e0395bfdedf1c12ca"
+checksum = "67df7112613f8bfd9150013a0314e196f4800d3201ae742489d999db2f979f08"
 dependencies = [
  "cfg-if",
  "futures-util",
@@ -1126,8 +1484,6 @@ dependencies = [
  "lexical-parse-float",
  "lexical-parse-integer",
  "lexical-util",
- "lexical-write-float",
- "lexical-write-integer",
 ]
 
 [[package]]
@@ -1155,25 +1511,6 @@ version = "1.0.7"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "2604dd126bb14f13fb5d1bd6a66155079cb9fa655b37f875b3a742c705dbed17"
 
-[[package]]
-name = "lexical-write-float"
-version = "1.0.6"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "50c438c87c013188d415fbabbb1dceb44249ab81664efbd31b14ae55dabb6361"
-dependencies = [
- "lexical-util",
- "lexical-write-integer",
-]
-
-[[package]]
-name = "lexical-write-integer"
-version = "1.0.6"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "409851a618475d2d5796377cad353802345cba92c867d9fbcde9cf4eac4e14df"
-dependencies = [
- "lexical-util",
-]
-
 [[package]]
 name = "libc"
 version = "0.2.186"
@@ -1207,6 +1544,21 @@ version = "0.8.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "92daf443525c4cce67b150400bc2316076100ce0b3686209eb8cf3c31612e6f0"
 
+[[package]]
+name = "litrs"
+version = "1.0.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "11d3d7f243d5c5a8b9bb5d6dd2b1602c0cb0b9db1621bafc7ed66e35ff9fe092"
+
+[[package]]
+name = "lock_api"
+version = "0.4.14"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "224399e74b87b5f3557511d98dff8b14089b3dadafcab6bb93eab67d3aace965"
+dependencies = [
+ "scopeguard",
+]
+
 [[package]]
 name = "log"
 version = "0.4.29"
@@ -1219,6 +1571,25 @@ version = "0.1.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "112b39cec0b298b6c1999fee3e31427f74f676e4cb9879ed1a121b43661a4154"
 
+[[package]]
+name = "lz4"
+version = "1.28.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "a20b523e860d03443e98350ceaac5e71c6ba89aea7d960769ec3ce37f4de5af4"
+dependencies = [
+ "lz4-sys",
+]
+
+[[package]]
+name = "lz4-sys"
+version = "1.11.1+lz4-1.10.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "6bd8c0d6c6ed0cd30b3652886bb8711dc4bb01d637a68105a3d5158039b418e6"
+dependencies = [
+ "cc",
+ "libc",
+]
+
 [[package]]
 name = "matrixmultiply"
 version = "0.3.10"
@@ -1235,6 +1606,15 @@ version = "2.8.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "f8ca58f447f06ed17d5fc4043ce1b10dd205e060fb3ce5b979b8ed8e59ff3f79"
 
+[[package]]
+name = "memmap2"
+version = "0.9.10"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "714098028fe011992e1c3962653c96b2d578c4b4bce9036e15ff220319b1e0e3"
+dependencies = [
+ "libc",
+]
+
 [[package]]
 name = "miniz_oxide"
 version = "0.8.9"
@@ -1242,6 +1622,7 @@ source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "1fa76a2c86f704bdb222d66965fb3d63269ce38518b83cb0575fca855ebb6316"
 dependencies = [
  "adler2",
+ "simd-adler32",
 ]
 
 [[package]]
@@ -1292,17 +1673,12 @@ dependencies = [
 ]
 
 [[package]]
-name = "num"
-version = "0.4.3"
+name = "now"
+version = "0.1.3"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "35bd024e8b2ff75562e5f34e7f4905839deb4b22955ef5e73d2fea1b9813cb23"
+checksum = "6d89e9874397a1f0a52fc1f197a8effd9735223cb2390e9dcc83ac6cd02923d0"
 dependencies = [
- "num-bigint",
- "num-complex",
- "num-integer",
- "num-iter",
- "num-rational",
- "num-traits",
+ "chrono",
 ]
 
 [[package]]
@@ -1325,22 +1701,22 @@ dependencies = [
 ]
 
 [[package]]
-name = "num-integer"
-version = "0.1.46"
+name = "num-derive"
+version = "0.4.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "7969661fd2958a5cb096e56c8e1ad0444ac2bbcd0061bd28660485a44879858f"
+checksum = "ed3955f1a9c7c0c15e092f9c887db08b1fc683305fdf6eb6684f22555355e202"
 dependencies = [
- "num-traits",
+ "proc-macro2",
+ "quote",
+ "syn",
 ]
 
 [[package]]
-name = "num-iter"
-version = "0.1.45"
+name = "num-integer"
+version = "0.1.46"
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-checksum = "1429034a0490724d0075ebb2bc9e875d6503c3cf69e235a8941aa757d83ef5bf"
+checksum = "7969661fd2958a5cb096e56c8e1ad0444ac2bbcd0061bd28660485a44879858f"
 dependencies = [
- "autocfg",
- "num-integer",
  "num-traits",
 ]
 
@@ -1374,6 +1750,43 @@ dependencies = [
  "memchr",
 ]
 
+[[package]]
+name = "object_store"
+version = "0.13.2"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "622acbc9100d3c10e2ee15804b0caa40e55c933d5aa53814cd520805b7958a49"
+dependencies = [
+ "async-trait",
+ "base64",
+ "bytes",
+ "chrono",
+ "form_urlencoded",
+ "futures-channel",
+ "futures-core",
+ "futures-util",
+ "http",
+ "http-body-util",
+ "humantime",
+ "hyper",
+ "itertools 0.14.0",
+ "parking_lot",
+ "percent-encoding",
+ "quick-xml",
+ "rand 0.10.1",
+ "reqwest",
+ "ring",
+ "serde",
+ "serde_json",
+ "serde_urlencoded",
+ "thiserror",
+ "tokio",
+ "tracing",
+ "url",
+ "walkdir",
+ "wasm-bindgen-futures",
+ "web-time",
+]
+
 [[package]]
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@@ -1387,19 +1800,16 @@ source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "d6790f58c7ff633d8771f42965289203411a5e5c68388703c06e14f24770b41e"
 
 [[package]]
-name = "option-ext"
-version = "0.2.0"
+name = "openssl-probe"
+version = "0.2.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "04744f49eae99ab78e0d5c0b603ab218f515ea8cfe5a456d7629ad883a3b6e7d"
+checksum = "7c87def4c32ab89d880effc9e097653c8da5d6ef28e6b539d313baaacfbafcbe"
 
 [[package]]
-name = "ordered-float"
-version = "2.10.1"
+name = "option-ext"
+version = "0.2.0"
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-checksum = "68f19d67e5a2795c94e73e0bb1cc1a7edeb2e28efd39e2e1c9b7a40c1108b11c"
-dependencies = [
- "num-traits",
-]
+checksum = "04744f49eae99ab78e0d5c0b603ab218f515ea8cfe5a456d7629ad883a3b6e7d"
 
 [[package]]
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@@ -1419,29 +1829,21 @@ dependencies = [
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  "ahash",
  "approx",
- "arrow-array",
  "camino",
- "comfy-table",
  "criterion",
  "directories",
  "hifitime",
  "husky-rs",
- "indicatif",
- "itertools 0.14.0",
  "nalgebra",
  "nom",
- "once_cell",
- "ordered-float 5.3.0",
- "parquet",
+ "ordered-float",
  "photom",
+ "polars",
  "proptest",
- "quick-xml 0.37.5",
  "rand 0.9.4",
  "rand_distr",
- "rayon",
  "reqwest",
  "roots",
- "serde",
  "smallvec",
  "thiserror",
  "tokio",
@@ -1461,45 +1863,64 @@ dependencies = [
 ]
 
 [[package]]
-name = "parquet"
-version = "54.3.1"
+name = "parking"
+version = "2.2.1"
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-checksum = "bfb15796ac6f56b429fd99e33ba133783ad75b27c36b4b5ce06f1f82cc97754e"
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- "arrow-array",
- "arrow-buffer",
- "arrow-cast",
- "arrow-data",
- "arrow-ipc",
- "arrow-schema",
- "arrow-select",
- "base64",
- "bytes",
- "chrono",
- "half",
- "hashbrown 0.15.5",
- "num",
- "num-bigint",
- "paste",
- "seq-macro",
- "snap",
- "thrift",
- "twox-hash",
-]
+checksum = "f38d5652c16fde515bb1ecef450ab0f6a219d619a7274976324d5e377f7dceba"
 
 [[package]]
-name = "paste"
-version = "1.0.15"
+name = "parking_lot"
+version = "0.12.5"
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-checksum = "57c0d7b74b563b49d38dae00a0c37d4d6de9b432382b2892f0574ddcae73fd0a"
+checksum = "93857453250e3077bd71ff98b6a65ea6621a19bb0f559a85248955ac12c45a1a"
+dependencies = [
+ "lock_api",
+ "parking_lot_core",
+]
 
 [[package]]
-name = "percent-encoding"
-version = "2.3.2"
+name = "parking_lot_core"
+version = "0.9.12"
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+checksum = "2621685985a2ebf1c516881c026032ac7deafcda1a2c9b7850dc81e3dfcb64c1"
+dependencies = [
+ "cfg-if",
+ "libc",
+ "redox_syscall",
+ "smallvec",
+ "windows-link 0.2.1",
+]
+
+[[package]]
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+version = "1.0.15"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "57c0d7b74b563b49d38dae00a0c37d4d6de9b432382b2892f0574ddcae73fd0a"
+
+[[package]]
+name = "percent-encoding"
+version = "2.3.2"
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 checksum = "9b4f627cb1b25917193a259e49bdad08f671f8d9708acfd5fe0a8c1455d87220"
 
+[[package]]
+name = "phf"
+version = "0.12.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "913273894cec178f401a31ec4b656318d95473527be05c0752cc41cdc32be8b7"
+dependencies = [
+ "phf_shared",
+]
+
+[[package]]
+name = "phf_shared"
+version = "0.12.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "06005508882fb681fd97892ecff4b7fd0fee13ef1aa569f8695dae7ab9099981"
+dependencies = [
+ "siphasher",
+]
+
 [[package]]
 name = "photom"
 version = "0.1.0"
@@ -1510,8 +1931,9 @@ dependencies = [
  "hifitime",
  "itertools 0.14.0",
  "nom",
- "ordered-float 5.3.0",
- "quick-xml 0.39.2",
+ "ordered-float",
+ "polars",
+ "quick-xml",
  "serde",
  "thiserror",
  "ureq",
@@ -1523,6 +1945,22 @@ version = "0.2.17"
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 checksum = "a89322df9ebe1c1578d689c92318e070967d1042b512afbe49518723f4e6d5cd"
 
+[[package]]
+name = "pkg-config"
+version = "0.3.33"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "19f132c84eca552bf34cab8ec81f1c1dcc229b811638f9d283dceabe58c5569e"
+
+[[package]]
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+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "3daf8e3d4b712abe1d690838f6e29fb76b76ea19589c4afa39ec30e12f62af71"
+dependencies = [
+ "array-init-cursor",
+ "hashbrown 0.15.5",
+]
+
 [[package]]
 name = "plotters"
 version = "0.3.7"
@@ -1552,10 +1990,555 @@ dependencies = [
 ]
 
 [[package]]
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-version = "1.13.1"
+name = "polars"
+version = "0.53.0"
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+ "getrandom 0.3.4",
+ "polars-arrow",
+ "polars-buffer",
+ "polars-compute",
+ "polars-core",
+ "polars-error",
+ "polars-io",
+ "polars-lazy",
+ "polars-ops",
+ "polars-parquet",
+ "polars-sql",
+ "polars-time",
+ "polars-utils",
+ "version_check",
+]
+
+[[package]]
+name = "polars-arrow"
+version = "0.53.0"
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+ "bitflags",
+ "bytemuck",
+ "bytes",
+ "chrono",
+ "chrono-tz",
+ "dyn-clone",
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+ "lz4",
+ "num-traits",
+ "polars-arrow-format",
+ "polars-buffer",
+ "polars-error",
+ "polars-schema",
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+checksum = "f7930d5ae1d006179e65f01af57c859307b5875a4cc078dc75257250b9ae5162"
+dependencies = [
+ "bitflags",
+ "blake3",
+ "bytemuck",
+ "bytes",
+ "chrono",
+ "chrono-tz",
+ "either",
+ "futures",
+ "hashbrown 0.16.1",
+ "memmap2",
+ "num-traits",
+ "percent-encoding",
+ "polars-arrow",
+ "polars-buffer",
+ "polars-compute",
+ "polars-core",
+ "polars-error",
+ "polars-io",
+ "polars-ops",
+ "polars-parquet",
+ "polars-time",
+ "polars-utils",
+ "rayon",
+ "recursive",
+ "regex",
+ "sha2",
+ "slotmap",
+ "strum_macros",
+ "tokio",
+ "version_check",
+]
+
+[[package]]
+name = "polars-row"
+version = "0.53.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "d29ea1a4554fe06442db1d6229235cd358e8eacba96aed8718f612caf3e3a646"
+dependencies = [
+ "bitflags",
+ "bytemuck",
+ "polars-arrow",
+ "polars-buffer",
+ "polars-compute",
+ "polars-dtype",
+ "polars-error",
+ "polars-utils",
+]
+
+[[package]]
+name = "polars-schema"
+version = "0.53.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "d688e73f9156f93cb29350be144c8f1e84c1bc705f00ee7f15eb9706a7971273"
+dependencies = [
+ "indexmap",
+ "polars-error",
+ "polars-utils",
+ "serde",
+ "version_check",
+]
+
+[[package]]
+name = "polars-sql"
+version = "0.53.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "100415f86069d7e9fbf54737148fc161a7c7316a6a7d375fb6cfc7fc64f570ae"
+dependencies = [
+ "bitflags",
+ "hex",
+ "polars-core",
+ "polars-error",
+ "polars-lazy",
+ "polars-ops",
+ "polars-plan",
+ "polars-time",
+ "polars-utils",
+ "regex",
+ "serde",
+ "sqlparser",
+]
+
+[[package]]
+name = "polars-stream"
+version = "0.53.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "65a0c054bdf16efd16bbc587e8d5418ae28464d61afd735513579cd3c338fa70"
+dependencies = [
+ "async-channel",
+ "async-trait",
+ "atomic-waker",
+ "bitflags",
+ "bytes",
+ "chrono-tz",
+ "crossbeam-channel",
+ "crossbeam-deque",
+ "crossbeam-queue",
+ "crossbeam-utils",
+ "futures",
+ "memchr",
+ "memmap2",
+ "num-traits",
+ "parking_lot",
+ "percent-encoding",
+ "pin-project-lite",
+ "polars-arrow",
+ "polars-buffer",
+ "polars-compute",
+ "polars-core",
+ "polars-error",
+ "polars-expr",
+ "polars-io",
+ "polars-mem-engine",
+ "polars-ops",
+ "polars-parquet",
+ "polars-plan",
+ "polars-time",
+ "polars-utils",
+ "rand 0.9.4",
+ "rayon",
+ "recursive",
+ "slotmap",
+ "tokio",
+ "version_check",
+]
+
+[[package]]
+name = "polars-time"
+version = "0.53.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "72e80404e1e418c997230e3b2972c3be331f45df8bdd3150fe3bef562c7a332f"
+dependencies = [
+ "atoi_simd",
+ "bytemuck",
+ "chrono",
+ "chrono-tz",
+ "now",
+ "num-traits",
+ "polars-arrow",
+ "polars-compute",
+ "polars-core",
+ "polars-error",
+ "polars-ops",
+ "polars-utils",
+ "rayon",
+ "regex",
+ "strum_macros",
+]
+
+[[package]]
+name = "polars-utils"
+version = "0.53.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "c97cabf53eb8fbf6050cde3fef8f596c51cc25fd7d55fbde108d815ee6674abf"
+dependencies = [
+ "argminmax",
+ "bincode",
+ "bytemuck",
+ "bytes",
+ "compact_str",
+ "either",
+ "flate2",
+ "foldhash 0.2.0",
+ "half",
+ "hashbrown 0.16.1",
+ "indexmap",
+ "libc",
+ "memmap2",
+ "num-derive",
+ "num-traits",
+ "polars-error",
+ "rand 0.9.4",
+ "raw-cpuid",
+ "rayon",
+ "regex",
+ "rmp-serde",
+ "serde",
+ "serde_json",
+ "serde_stacker",
+ "slotmap",
+ "stacker",
+ "uuid",
+ "version_check",
+]
 
 [[package]]
 name = "potential_utf"
@@ -1624,7 +2607,7 @@ checksum = "4b45fcc2344c680f5025fe57779faef368840d0bd1f42f216291f0dc4ace4744"
 dependencies = [
  "bit-set",
  "bit-vec",
- "bitflags 2.11.1",
+ "bitflags",
  "num-traits",
  "rand 0.9.4",
  "rand_chacha",
@@ -1636,26 +2619,26 @@ dependencies = [
 ]
 
 [[package]]
-name = "quick-error"
-version = "1.2.3"
+name = "psm"
+version = "0.1.31"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "a1d01941d82fa2ab50be1e79e6714289dd7cde78eba4c074bc5a4374f650dfe0"
+checksum = "645dbe486e346d9b5de3ef16ede18c26e6c70ad97418f4874b8b1889d6e761ea"
+dependencies = [
+ "ar_archive_writer",
+ "cc",
+]
 
 [[package]]
-name = "quick-xml"
-version = "0.37.5"
+name = "quick-error"
+version = "1.2.3"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "331e97a1af0bf59823e6eadffe373d7b27f485be8748f71471c662c1f269b7fb"
-dependencies = [
- "memchr",
- "serde",
-]
+checksum = "a1d01941d82fa2ab50be1e79e6714289dd7cde78eba4c074bc5a4374f650dfe0"
 
 [[package]]
 name = "quick-xml"
-version = "0.39.2"
+version = "0.39.4"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "958f21e8e7ceb5a1aa7fa87fab28e7c75976e0bfe7e23ff069e0a260f894067d"
+checksum = "cdcc8dd4e2f670d309a5f0e83fe36dfdc05af317008fea29144da1a2ac858e5e"
 dependencies = [
  "memchr",
  "serde",
@@ -1757,6 +2740,17 @@ dependencies = [
  "rand_core 0.9.5",
 ]
 
+[[package]]
+name = "rand"
+version = "0.10.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "d2e8e8bcc7961af1fdac401278c6a831614941f6164ee3bf4ce61b7edb162207"
+dependencies = [
+ "chacha20",
+ "getrandom 0.4.2",
+ "rand_core 0.10.1",
+]
+
 [[package]]
 name = "rand_chacha"
 version = "0.9.0"
@@ -1785,6 +2779,12 @@ dependencies = [
  "getrandom 0.3.4",
 ]
 
+[[package]]
+name = "rand_core"
+version = "0.10.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "63b8176103e19a2643978565ca18b50549f6101881c443590420e4dc998a3c69"
+
 [[package]]
 name = "rand_distr"
 version = "0.5.1"
@@ -1804,6 +2804,15 @@ dependencies = [
  "rand_core 0.9.5",
 ]
 
+[[package]]
+name = "raw-cpuid"
+version = "11.6.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "498cd0dc59d73224351ee52a95fee0f1a617a2eae0e7d9d720cc622c73a54186"
+dependencies = [
+ "bitflags",
+]
+
 [[package]]
 name = "rawpointer"
 version = "0.2.1"
@@ -1830,6 +2839,35 @@ dependencies = [
  "crossbeam-utils",
 ]
 
+[[package]]
+name = "recursive"
+version = "0.1.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "0786a43debb760f491b1bc0269fe5e84155353c67482b9e60d0cfb596054b43e"
+dependencies = [
+ "recursive-proc-macro-impl",
+ "stacker",
+]
+
+[[package]]
+name = "recursive-proc-macro-impl"
+version = "0.1.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "76009fbe0614077fc1a2ce255e3a1881a2e3a3527097d5dc6d8212c585e7e38b"
+dependencies = [
+ "quote",
+ "syn",
+]
+
+[[package]]
+name = "redox_syscall"
+version = "0.5.18"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "ed2bf2547551a7053d6fdfafda3f938979645c44812fbfcda098faae3f1a362d"
+dependencies = [
+ "bitflags",
+]
+
 [[package]]
 name = "redox_users"
 version = "0.5.2"
@@ -1893,6 +2931,7 @@ dependencies = [
  "pin-project-lite",
  "quinn",
  "rustls",
+ "rustls-native-certs",
  "rustls-pki-types",
  "serde",
  "serde_json",
@@ -1916,14 +2955,33 @@ dependencies = [
 name = "ring"
 version = "0.17.14"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "a4689e6c2294d81e88dc6261c768b63bc4fcdb852be6d1352498b114f61383b7"
+checksum = "a4689e6c2294d81e88dc6261c768b63bc4fcdb852be6d1352498b114f61383b7"
+dependencies = [
+ "cc",
+ "cfg-if",
+ "getrandom 0.2.17",
+ "libc",
+ "untrusted",
+ "windows-sys 0.52.0",
+]
+
+[[package]]
+name = "rmp"
+version = "0.8.15"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "4ba8be72d372b2c9b35542551678538b562e7cf86c3315773cae48dfbfe7790c"
+dependencies = [
+ "num-traits",
+]
+
+[[package]]
+name = "rmp-serde"
+version = "1.3.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "72f81bee8c8ef9b577d1681a70ebbc962c232461e397b22c208c43c04b67a155"
 dependencies = [
- "cc",
- "cfg-if",
- "getrandom 0.2.17",
- "libc",
- "untrusted",
- "windows-sys 0.52.0",
+ "rmp",
+ "serde",
 ]
 
 [[package]]
@@ -1944,22 +3002,13 @@ version = "2.1.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "94300abf3f1ae2e2b8ffb7b58043de3d399c73fa6f4b73826402a5c457614dbe"
 
-[[package]]
-name = "rustc_version"
-version = "0.4.1"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "cfcb3a22ef46e85b45de6ee7e79d063319ebb6594faafcf1c225ea92ab6e9b92"
-dependencies = [
- "semver",
-]
-
 [[package]]
 name = "rustix"
 version = "1.1.4"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "b6fe4565b9518b83ef4f91bb47ce29620ca828bd32cb7e408f0062e9930ba190"
 dependencies = [
- "bitflags 2.11.1",
+ "bitflags",
  "errno",
  "libc",
  "linux-raw-sys",
@@ -1968,9 +3017,9 @@ dependencies = [
 
 [[package]]
 name = "rustls"
-version = "0.23.39"
+version = "0.23.40"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "7c2c118cb077cca2822033836dfb1b975355dfb784b5e8da48f7b6c5db74e60e"
+checksum = "ef86cd5876211988985292b91c96a8f2d298df24e75989a43a3c73f2d4d8168b"
 dependencies = [
  "log",
  "once_cell",
@@ -1981,11 +3030,23 @@ dependencies = [
  "zeroize",
 ]
 
+[[package]]
+name = "rustls-native-certs"
+version = "0.8.3"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "612460d5f7bea540c490b2b6395d8e34a953e52b491accd6c86c8164c5932a63"
+dependencies = [
+ "openssl-probe",
+ "rustls-pki-types",
+ "schannel",
+ "security-framework",
+]
+
 [[package]]
 name = "rustls-pki-types"
-version = "1.14.0"
+version = "1.14.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "be040f8b0a225e40375822a563fa9524378b9d63112f53e19ffff34df5d33fdd"
+checksum = "30a7197ae7eb376e574fe940d068c30fe0462554a3ddbe4eca7838e049c937a9"
 dependencies = [
  "web-time",
  "zeroize",
@@ -2045,16 +3106,48 @@ dependencies = [
 ]
 
 [[package]]
-name = "semver"
-version = "1.0.28"
+name = "schannel"
+version = "0.1.29"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "8a7852d02fc848982e0c167ef163aaff9cd91dc640ba85e263cb1ce46fae51cd"
+checksum = "91c1b7e4904c873ef0710c1f407dde2e6287de2bebc1bbbf7d430bb7cbffd939"
+dependencies = [
+ "windows-sys 0.61.2",
+]
 
 [[package]]
-name = "seq-macro"
-version = "0.3.6"
+name = "scopeguard"
+version = "1.2.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "94143f37725109f92c262ed2cf5e59bce7498c01bcc1502d7b9afe439a4e9f49"
+
+[[package]]
+name = "security-framework"
+version = "3.7.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "b7f4bc775c73d9a02cde8bf7b2ec4c9d12743edf609006c7facc23998404cd1d"
+dependencies = [
+ "bitflags",
+ "core-foundation",
+ "core-foundation-sys",
+ "libc",
+ "security-framework-sys",
+]
+
+[[package]]
+name = "security-framework-sys"
+version = "2.17.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "6ce2691df843ecc5d231c0b14ece2acc3efb62c0a398c7e1d875f3983ce020e3"
+dependencies = [
+ "core-foundation-sys",
+ "libc",
+]
+
+[[package]]
+name = "semver"
+version = "1.0.28"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "1bc711410fbe7399f390ca1c3b60ad0f53f80e95c5eb935e52268a0e2cd49acc"
+checksum = "8a7852d02fc848982e0c167ef163aaff9cd91dc640ba85e263cb1ce46fae51cd"
 
 [[package]]
 name = "serde"
@@ -2099,6 +3192,17 @@ dependencies = [
  "zmij",
 ]
 
+[[package]]
+name = "serde_stacker"
+version = "0.1.14"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "d4936375d50c4be7eff22293a9344f8e46f323ed2b3c243e52f89138d9bb0f4a"
+dependencies = [
+ "serde",
+ "serde_core",
+ "stacker",
+]
+
 [[package]]
 name = "serde_urlencoded"
 version = "0.7.1"
@@ -2111,12 +3215,43 @@ dependencies = [
  "serde",
 ]
 
+[[package]]
+name = "sha2"
+version = "0.10.9"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "a7507d819769d01a365ab707794a4084392c824f54a7a6a7862f8c3d0892b283"
+dependencies = [
+ "cfg-if",
+ "cpufeatures 0.2.17",
+ "digest",
+]
+
 [[package]]
 name = "shlex"
 version = "1.3.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "0fda2ff0d084019ba4d7c6f371c95d8fd75ce3524c3cb8fb653a3023f6323e64"
 
+[[package]]
+name = "signal-hook"
+version = "0.4.4"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "b2a0c28ca5908dbdbcd52e6fdaa00358ab88637f8ab33e1f188dd510eb44b53d"
+dependencies = [
+ "libc",
+ "signal-hook-registry",
+]
+
+[[package]]
+name = "signal-hook-registry"
+version = "1.4.8"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "c4db69cba1110affc0e9f7bcd48bbf87b3f4fc7c61fc9155afd4c469eb3d6c1b"
+dependencies = [
+ "errno",
+ "libc",
+]
+
 [[package]]
 name = "simba"
 version = "0.9.1"
@@ -2130,12 +3265,39 @@ dependencies = [
  "wide",
 ]
 
+[[package]]
+name = "simd-adler32"
+version = "0.3.9"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "703d5c7ef118737c72f1af64ad2f6f8c5e1921f818cdcb97b8fe6fc69bf66214"
+
+[[package]]
+name = "simdutf8"
+version = "0.1.5"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "e3a9fe34e3e7a50316060351f37187a3f546bce95496156754b601a5fa71b76e"
+
+[[package]]
+name = "siphasher"
+version = "1.0.3"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "8ee5873ec9cce0195efcb7a4e9507a04cd49aec9c83d0389df45b1ef7ba2e649"
+
 [[package]]
 name = "slab"
 version = "0.4.12"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "0c790de23124f9ab44544d7ac05d60440adc586479ce501c1d6d7da3cd8c9cf5"
 
+[[package]]
+name = "slotmap"
+version = "1.1.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "bdd58c3c93c3d278ca835519292445cb4b0d4dc59ccfdf7ceadaab3f8aeb4038"
+dependencies = [
+ "version_check",
+]
+
 [[package]]
 name = "smallvec"
 version = "1.15.1"
@@ -2180,18 +3342,86 @@ dependencies = [
  "windows-sys 0.61.2",
 ]
 
+[[package]]
+name = "sqlparser"
+version = "0.60.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "505aa16b045c4c1375bf5f125cce3813d0176325bfe9ffc4a903f423de7774ff"
+dependencies = [
+ "log",
+ "recursive",
+ "sqlparser_derive",
+]
+
+[[package]]
+name = "sqlparser_derive"
+version = "0.4.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "028e551d5e270b31b9f3ea271778d9d827148d4287a5d96167b6bb9787f5cc38"
+dependencies = [
+ "proc-macro2",
+ "quote",
+ "syn",
+]
+
 [[package]]
 name = "stable_deref_trait"
 version = "1.2.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "6ce2be8dc25455e1f91df71bfa12ad37d7af1092ae736f3a6cd0e37bc7810596"
 
+[[package]]
+name = "stacker"
+version = "0.1.24"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "640c8cdd92b6b12f5bcb1803ca3bbf5ab96e5e6b6b96b9ab77dabe9e880b3190"
+dependencies = [
+ "cc",
+ "cfg-if",
+ "libc",
+ "psm",
+ "windows-sys 0.61.2",
+]
+
 [[package]]
 name = "static_assertions"
 version = "1.1.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "a2eb9349b6444b326872e140eb1cf5e7c522154d69e7a0ffb0fb81c06b37543f"
 
+[[package]]
+name = "streaming-decompression"
+version = "0.1.2"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "bf6cc3b19bfb128a8ad11026086e31d3ce9ad23f8ea37354b31383a187c44cf3"
+dependencies = [
+ "fallible-streaming-iterator",
+]
+
+[[package]]
+name = "streaming-iterator"
+version = "0.1.9"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "2b2231b7c3057d5e4ad0156fb3dc807d900806020c5ffa3ee6ff2c8c76fb8520"
+
+[[package]]
+name = "strength_reduce"
+version = "0.2.4"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "fe895eb47f22e2ddd4dabc02bce419d2e643c8e3b585c78158b349195bc24d82"
+
+[[package]]
+name = "strum_macros"
+version = "0.27.2"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "7695ce3845ea4b33927c055a39dc438a45b059f7c1b3d91d38d10355fb8cbca7"
+dependencies = [
+ "heck",
+ "proc-macro2",
+ "quote",
+ "syn",
+]
+
 [[package]]
 name = "subtle"
 version = "2.6.1"
@@ -2295,26 +3525,6 @@ dependencies = [
  "syn",
 ]
 
-[[package]]
-name = "thrift"
-version = "0.17.0"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "7e54bc85fc7faa8bc175c4bab5b92ba8d9a3ce893d0e9f42cc455c8ab16a9e09"
-dependencies = [
- "byteorder",
- "integer-encoding",
- "ordered-float 2.10.1",
-]
-
-[[package]]
-name = "tiny-keccak"
-version = "2.0.2"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "2c9d3793400a45f954c52e73d068316d76b6f4e36977e3fcebb13a2721e80237"
-dependencies = [
- "crunchy",
-]
-
 [[package]]
 name = "tinystr"
 version = "0.8.3"
@@ -2352,18 +3562,30 @@ checksum = "1f3ccbac311fea05f86f61904b462b55fb3df8837a366dfc601a0161d0532f20"
 
 [[package]]
 name = "tokio"
-version = "1.52.1"
+version = "1.52.3"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "b67dee974fe86fd92cc45b7a95fdd2f99a36a6d7b0d431a231178d3d670bbcc6"
+checksum = "8fc7f01b389ac15039e4dc9531aa973a135d7a4135281b12d7c1bc79fd57fffe"
 dependencies = [
  "bytes",
  "libc",
  "mio",
  "pin-project-lite",
  "socket2",
+ "tokio-macros",
  "windows-sys 0.61.2",
 ]
 
+[[package]]
+name = "tokio-macros"
+version = "2.7.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "385a6cb71ab9ab790c5fe8d67f1645e6c450a7ce006a33de03daa956cf70a496"
+dependencies = [
+ "proc-macro2",
+ "quote",
+ "syn",
+]
+
 [[package]]
 name = "tokio-rustls"
 version = "0.26.4"
@@ -2415,20 +3637,20 @@ dependencies = [
 
 [[package]]
 name = "tower-http"
-version = "0.6.8"
+version = "0.6.11"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "d4e6559d53cc268e5031cd8429d05415bc4cb4aefc4aa5d6cc35fbf5b924a1f8"
+checksum = "4cfcf7e2740e6fc6d4d688b4ef00650406bb94adf4731e43c096c3a19fe40840"
 dependencies = [
- "bitflags 2.11.1",
+ "bitflags",
  "bytes",
  "futures-util",
  "http",
  "http-body",
- "iri-string",
  "pin-project-lite",
  "tower",
  "tower-layer",
  "tower-service",
+ "url",
 ]
 
 [[package]]
@@ -2450,9 +3672,21 @@ source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "63e71662fa4b2a2c3a26f570f037eb95bb1f85397f3cd8076caed2f026a6d100"
 dependencies = [
  "pin-project-lite",
+ "tracing-attributes",
  "tracing-core",
 ]
 
+[[package]]
+name = "tracing-attributes"
+version = "0.1.31"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "7490cfa5ec963746568740651ac6781f701c9c5ea257c58e057f3ba8cf69e8da"
+dependencies = [
+ "proc-macro2",
+ "quote",
+ "syn",
+]
+
 [[package]]
 name = "tracing-core"
 version = "0.1.36"
@@ -2468,16 +3702,6 @@ version = "0.2.5"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "e421abadd41a4225275504ea4d6566923418b7f05506fbc9c0fe86ba7396114b"
 
-[[package]]
-name = "twox-hash"
-version = "1.6.3"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "97fee6b57c6a41524a810daee9286c02d7752c4253064d0b05472833a438f675"
-dependencies = [
- "cfg-if",
- "static_assertions",
-]
-
 [[package]]
 name = "typenum"
 version = "1.20.0"
@@ -2496,6 +3720,24 @@ version = "1.0.24"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "e6e4313cd5fcd3dad5cafa179702e2b244f760991f45397d14d4ebf38247da75"
 
+[[package]]
+name = "unicode-normalization"
+version = "0.1.25"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "5fd4f6878c9cb28d874b009da9e8d183b5abc80117c40bbd187a1fde336be6e8"
+dependencies = [
+ "tinyvec",
+]
+
+[[package]]
+name = "unicode-reverse"
+version = "1.0.9"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "4b6f4888ebc23094adfb574fdca9fdc891826287a6397d2cd28802ffd6f20c76"
+dependencies = [
+ "unicode-segmentation",
+]
+
 [[package]]
 name = "unicode-segmentation"
 version = "1.13.2"
@@ -2514,18 +3756,18 @@ version = "0.2.6"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "ebc1c04c71510c7f702b52b7c350734c9ff1295c464a03335b00bb84fc54f853"
 
-[[package]]
-name = "unit-prefix"
-version = "0.5.2"
-source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "81e544489bf3d8ef66c953931f56617f423cd4b5494be343d9b9d3dda037b9a3"
-
 [[package]]
 name = "untrusted"
 version = "0.9.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "8ecb6da28b8a351d773b68d5825ac39017e680750f980f3a1a85cd8dd28a47c1"
 
+[[package]]
+name = "unty"
+version = "0.0.4"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "6d49784317cd0d1ee7ec5c716dd598ec5b4483ea832a2dced265471cc0f690ae"
+
 [[package]]
 name = "ureq"
 version = "3.3.0"
@@ -2578,12 +3820,30 @@ version = "1.0.4"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "b6c140620e7ffbb22c2dee59cafe6084a59b5ffc27a8859a5f0d494b5d52b6be"
 
+[[package]]
+name = "uuid"
+version = "1.23.1"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "ddd74a9687298c6858e9b88ec8935ec45d22e8fd5e6394fa1bd4e99a87789c76"
+dependencies = [
+ "getrandom 0.4.2",
+ "js-sys",
+ "serde_core",
+ "wasm-bindgen",
+]
+
 [[package]]
 name = "version_check"
 version = "0.9.5"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "0b928f33d975fc6ad9f86c8f283853ad26bdd5b10b7f1542aa2fa15e2289105a"
 
+[[package]]
+name = "virtue"
+version = "0.0.18"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "051eb1abcf10076295e815102942cc58f9d5e3b4560e46e53c21e8ff6f3af7b1"
+
 [[package]]
 name = "wait-timeout"
 version = "0.2.1"
@@ -2638,9 +3898,9 @@ dependencies = [
 
 [[package]]
 name = "wasm-bindgen"
-version = "0.2.118"
+version = "0.2.121"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "0bf938a0bacb0469e83c1e148908bd7d5a6010354cf4fb73279b7447422e3a89"
+checksum = "49ace1d07c165b0864824eee619580c4689389afa9dc9ed3a4c75040d82e6790"
 dependencies = [
  "cfg-if",
  "once_cell",
@@ -2651,9 +3911,9 @@ dependencies = [
 
 [[package]]
 name = "wasm-bindgen-futures"
-version = "0.4.68"
+version = "0.4.71"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "f371d383f2fb139252e0bfac3b81b265689bf45b6874af544ffa4c975ac1ebf8"
+checksum = "96492d0d3ffba25305a7dc88720d250b1401d7edca02cc3bcd50633b424673b8"
 dependencies = [
  "js-sys",
  "wasm-bindgen",
@@ -2661,9 +3921,9 @@ dependencies = [
 
 [[package]]
 name = "wasm-bindgen-macro"
-version = "0.2.118"
+version = "0.2.121"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "eeff24f84126c0ec2db7a449f0c2ec963c6a49efe0698c4242929da037ca28ed"
+checksum = "8e68e6f4afd367a562002c05637acb8578ff2dea1943df76afb9e83d177c8578"
 dependencies = [
  "quote",
  "wasm-bindgen-macro-support",
@@ -2671,9 +3931,9 @@ dependencies = [
 
 [[package]]
 name = "wasm-bindgen-macro-support"
-version = "0.2.118"
+version = "0.2.121"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "9d08065faf983b2b80a79fd87d8254c409281cf7de75fc4b773019824196c904"
+checksum = "d95a9ec35c64b2a7cb35d3fead40c4238d0940c86d107136999567a4703259f2"
 dependencies = [
  "bumpalo",
  "proc-macro2",
@@ -2684,9 +3944,9 @@ dependencies = [
 
 [[package]]
 name = "wasm-bindgen-shared"
-version = "0.2.118"
+version = "0.2.121"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "5fd04d9e306f1907bd13c6361b5c6bfc7b3b3c095ed3f8a9246390f8dbdee129"
+checksum = "c4e0100b01e9f0d03189a92b96772a1fb998639d981193d7dbab487302513441"
 dependencies = [
  "unicode-ident",
 ]
@@ -2732,7 +3992,7 @@ version = "0.244.0"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "47b807c72e1bac69382b3a6fb3dbe8ea4c0ed87ff5629b8685ae6b9a611028fe"
 dependencies = [
- "bitflags 2.11.1",
+ "bitflags",
  "hashbrown 0.15.5",
  "indexmap",
  "semver",
@@ -2740,9 +4000,9 @@ dependencies = [
 
 [[package]]
 name = "web-sys"
-version = "0.3.95"
+version = "0.3.98"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "4f2dfbb17949fa2088e5d39408c48368947b86f7834484e87b73de55bc14d97d"
+checksum = "4b572dff8bcf38bad0fa19729c89bb5748b2b9b1d8be70cf90df697e3a8f32aa"
 dependencies = [
  "js-sys",
  "wasm-bindgen",
@@ -2777,6 +4037,22 @@ dependencies = [
  "safe_arch",
 ]
 
+[[package]]
+name = "winapi"
+version = "0.3.9"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "5c839a674fcd7a98952e593242ea400abe93992746761e38641405d28b00f419"
+dependencies = [
+ "winapi-i686-pc-windows-gnu",
+ "winapi-x86_64-pc-windows-gnu",
+]
+
+[[package]]
+name = "winapi-i686-pc-windows-gnu"
+version = "0.4.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "ac3b87c63620426dd9b991e5ce0329eff545bccbbb34f3be09ff6fb6ab51b7b6"
+
 [[package]]
 name = "winapi-util"
 version = "0.1.11"
@@ -2786,6 +4062,12 @@ dependencies = [
  "windows-sys 0.61.2",
 ]
 
+[[package]]
+name = "winapi-x86_64-pc-windows-gnu"
+version = "0.4.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "712e227841d057c1ee1cd2fb22fa7e5a5461ae8e48fa2ca79ec42cfc1931183f"
+
 [[package]]
 name = "windows-core"
 version = "0.62.2"
@@ -2794,7 +4076,7 @@ checksum = "b8e83a14d34d0623b51dce9581199302a221863196a1dde71a7663a4c2be9deb"
 dependencies = [
  "windows-implement",
  "windows-interface",
- "windows-link",
+ "windows-link 0.2.1",
  "windows-result",
  "windows-strings",
 ]
@@ -2821,6 +4103,12 @@ dependencies = [
  "syn",
 ]
 
+[[package]]
+name = "windows-link"
+version = "0.1.3"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "5e6ad25900d524eaabdbbb96d20b4311e1e7ae1699af4fb28c17ae66c80d798a"
+
 [[package]]
 name = "windows-link"
 version = "0.2.1"
@@ -2833,7 +4121,7 @@ version = "0.4.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "7781fa89eaf60850ac3d2da7af8e5242a5ea78d1a11c49bf2910bb5a73853eb5"
 dependencies = [
- "windows-link",
+ "windows-link 0.2.1",
 ]
 
 [[package]]
@@ -2842,7 +4130,7 @@ version = "0.5.1"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "7837d08f69c77cf6b07689544538e017c1bfcf57e34b4c0ff58e6c2cd3b37091"
 dependencies = [
- "windows-link",
+ "windows-link 0.2.1",
 ]
 
 [[package]]
@@ -2854,6 +4142,15 @@ dependencies = [
  "windows-targets 0.52.6",
 ]
 
+[[package]]
+name = "windows-sys"
+version = "0.59.0"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "1e38bc4d79ed67fd075bcc251a1c39b32a1776bbe92e5bef1f0bf1f8c531853b"
+dependencies = [
+ "windows-targets 0.52.6",
+]
+
 [[package]]
 name = "windows-sys"
 version = "0.60.2"
@@ -2869,7 +4166,7 @@ version = "0.61.2"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "ae137229bcbd6cdf0f7b80a31df61766145077ddf49416a728b02cb3921ff3fc"
 dependencies = [
- "windows-link",
+ "windows-link 0.2.1",
 ]
 
 [[package]]
@@ -2894,7 +4191,7 @@ version = "0.53.5"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "4945f9f551b88e0d65f3db0bc25c33b8acea4d9e41163edf90dcd0b19f9069f3"
 dependencies = [
- "windows-link",
+ "windows-link 0.2.1",
  "windows_aarch64_gnullvm 0.53.1",
  "windows_aarch64_msvc 0.53.1",
  "windows_i686_gnu 0.53.1",
@@ -3065,7 +4362,7 @@ source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "9d66ea20e9553b30172b5e831994e35fbde2d165325bec84fc43dbf6f4eb9cb2"
 dependencies = [
  "anyhow",
- "bitflags 2.11.1",
+ "bitflags",
  "indexmap",
  "log",
  "serde",
@@ -3101,6 +4398,12 @@ version = "0.6.3"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "1ffae5123b2d3fc086436f8834ae3ab053a283cfac8fe0a0b8eaae044768a4c4"
 
+[[package]]
+name = "xxhash-rust"
+version = "0.8.15"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "fdd20c5420375476fbd4394763288da7eb0cc0b8c11deed431a91562af7335d3"
+
 [[package]]
 name = "yoke"
 version = "0.8.2"
@@ -3146,9 +4449,9 @@ dependencies = [
 
 [[package]]
 name = "zerofrom"
-version = "0.1.7"
+version = "0.1.8"
 source = "registry+https://github.com/rust-lang/crates.io-index"
-checksum = "69faa1f2a1ea75661980b013019ed6687ed0e83d069bc1114e2cc74c6c04c4df"
+checksum = "0ec05a11813ea801ff6d75110ad09cd0824ddba17dfe17128ea0d5f68e6c5272"
 dependencies = [
  "zerofrom-derive",
 ]
@@ -3204,8 +4507,42 @@ dependencies = [
  "syn",
 ]
 
+[[package]]
+name = "zlib-rs"
+version = "0.6.3"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "3be3d40e40a133f9c916ee3f9f4fa2d9d63435b5fbe1bfc6d9dae0aa0ada1513"
+
 [[package]]
 name = "zmij"
 version = "1.0.21"
 source = "registry+https://github.com/rust-lang/crates.io-index"
 checksum = "b8848ee67ecc8aedbaf3e4122217aff892639231befc6a1b58d29fff4c2cabaa"
+
+[[package]]
+name = "zstd"
+version = "0.13.3"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "e91ee311a569c327171651566e07972200e76fcfe2242a4fa446149a3881c08a"
+dependencies = [
+ "zstd-safe",
+]
+
+[[package]]
+name = "zstd-safe"
+version = "7.2.4"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "8f49c4d5f0abb602a93fb8736af2a4f4dd9512e36f7f570d66e65ff867ed3b9d"
+dependencies = [
+ "zstd-sys",
+]
+
+[[package]]
+name = "zstd-sys"
+version = "2.0.16+zstd.1.5.7"
+source = "registry+https://github.com/rust-lang/crates.io-index"
+checksum = "91e19ebc2adc8f83e43039e79776e3fda8ca919132d68a1fed6a5faca2683748"
+dependencies = [
+ "cc",
+ "pkg-config",
+]
diff --git a/Cargo.toml b/Cargo.toml
index 8d94981..a647e61 100644
--- a/Cargo.toml
+++ b/Cargo.toml
@@ -25,36 +25,23 @@ photom = { version = "0.1.0", path = "../photom" }
 
 aberth = { version = "0.4.1", default-features = false }
 ahash = { version = "0.8.11", default-features = false }
-arrow-array = { version = "54.3.1", default-features = false }
 camino = { version = "1.1.9", default-features = false }
 directories = "6.0.0"
 hifitime = { version = "4.2.0", default-features = false, features = [
     "ut1",
     "std",
 ] }
-itertools = { version = "0.14.0", default-features = false, features = [
-    "use_std",
-] }
 nalgebra = { version = "0.33.2" }
 ordered-float = { version = "5.0.0", default-features = false }
-parquet = { version = "54.2.1", default-features = false, features = [
-    "arrow",
-    "snap",
-] }
-quick-xml = { version = "0.37.3", features = [
-    "serialize",
-], default-features = false }
-serde = { version = "1.0", features = ["derive"], default-features = false }
 smallvec = { version = "1.14.0", default-features = false }
 thiserror = { version = "2.0.12", default-features = false }
 ureq = { version = "3.0.10", default-features = false, features = ["rustls"] }
 nom = { version = "8.0.0" }
-once_cell = { version = "1.21.3", default-features = false }
 roots = { version = "0.0.8", default-features = false }
 rand = { version = "0.9.2", default-features = false, features = [
     "std_rng",
     "os_rng",
-    "small_rng"
+    "small_rng",
 ] }
 rand_distr = { version = "0.5.1", default-features = false }
 
@@ -70,9 +57,6 @@ tokio = { version = "1.44.1", default-features = false, features = [
     "io-util",
 ] }
 tokio-stream = { version = "0.1.17", default-features = false }
-indicatif = { version = "0.18", optional = true, default-features = false }
-rayon = { version = "1.11.0", optional = true, default-features = false }
-comfy-table = { version = "7.1.4", default-features = false }
 
 [dev-dependencies]
 approx = { version = "0.5.1", default-features = false }
@@ -80,51 +64,12 @@ criterion = { version = "0.5.1", features = ["html_reports"] }
 husky-rs = "0.1.5"
 proptest = "1.7.0"
 
-photom = { version = "0.1.0", path = "../photom", features = ["mpc_80_col", "ades"] }
-
-[features]
-progress = ["dep:indicatif"]
-parallel = ["dep:rayon"]
-
-[[test]]
-name = "test_large_parquet"
-path = "tests/trajectories_from_parquet.rs"
-required-features = ["jpl-download"]
-
-[[test]]
-name = "test_trajectories_from_vec"
-path = "tests/trajectories_from_vec.rs"
-required-features = ["jpl-download"]
-
-[[example]]
-name = "gauss_iod_once"
-path = "examples/gauss_iod_once.rs"
-required-features = ["jpl-download"]
-
-[[example]]
-name = "parquet_to_orbit"
-path = "examples/parquet_to_orbit.rs"
-required-features = ["jpl-download"]
-
-[[bench]]
-name = "load_parquet"
-harness = false
-required-features = ["jpl-download"]
-
-[[bench]]
-name = "outfit_gauss_iod"
-harness = false
-required-features = ["jpl-download"]
-
-[[bench]]
-name = "solve_kepler_equation"
-harness = false
-required-features = ["jpl-download"]
-
-[[bench]]
-name = "gauss_prelim_orbit"
-harness = false
-required-features = ["jpl-download"]
+photom = { version = "0.1.0", path = "../photom", features = [
+    "mpc_80_col",
+    "ades",
+    "polars",
+] }
+polars = { version = "0.53.0", features = ["is_in"] }
 
 [profile.bench]
 opt-level = 3
diff --git a/benches/gauss_prelim_orbit.rs b/benches/gauss_prelim_orbit.rs
deleted file mode 100644
index 7621ca1..0000000
--- a/benches/gauss_prelim_orbit.rs
+++ /dev/null
@@ -1,148 +0,0 @@
-//! Benchmarks for GaussObs::prelim_orbit (single-threaded)
-//!
-//! Exemples d'exécution :
-//!   cargo bench --bench gauss_prelim_orbit --features jpl-download
-//!   cargo bench gauss_prelim_orbit -- gauss_prelim_orbit/single_call
-//!   cargo bench gauss_prelim_orbit -- gauss_prelim_orbit/batch_100
-//!   cargo bench gauss_prelim_orbit -- gauss_prelim_orbit/noisy_batch_100
-//!
-//! Astuce : vous pouvez aussi lancer en ligne de commande avec
-//!   RAYON_NUM_THREADS=1 cargo bench --bench gauss_prelim_orbit
-
-#![cfg_attr(not(feature = "jpl-download"), allow(dead_code))]
-
-use criterion::{black_box, criterion_group, criterion_main, BatchSize, Criterion};
-use nalgebra::{Matrix3, Vector3};
-
-use outfit::initial_orbit_determination::gauss::GaussObs;
-use outfit::initial_orbit_determination::gauss_result::GaussResult;
-use outfit::initial_orbit_determination::IODParams;
-use outfit::outfit::Outfit;
-use outfit::outfit_errors::OutfitError;
-use rand::SeedableRng;
-
-/// Build global Outfit state (ephemerides, frames, etc.)
-/// Note: keep this outside the hot loops.
-fn build_state() -> Result {
-    // English in-code comments per user preference:
-    // Using FCCT14 as in production; adjust if you want to compare error models.
-    use outfit::error_models::ErrorModel;
-    Outfit::new("horizon:DE440", ErrorModel::FCCT14)
-}
-
-/// Deterministic GaussObs fixture (angles in radians, times in MJD TT)
-fn make_fixture_gaussobs() -> GaussObs {
-    let idx_obs = Vector3::new(0, 1, 2);
-    let ra = Vector3::new(1.6894680985108945, 1.6898614520910629, 1.7526450904422723);
-    let dec = Vector3::new(
-        1.0825984522657437,
-        0.943_679_018_934_623_1,
-        0.827_517_321_571_201_4,
-    );
-    let time = Vector3::new(
-        57_028.454_047_592_59,
-        57_049.231_857_592_59,
-        57_063.959_487_592_59,
-    );
-
-    let observer_helio_position = Matrix3::new(
-        -0.264_135_633_607_079,
-        -0.588_973_552_650_573_5,
-        -0.774_192_148_350_372,
-        0.869_046_620_910_086,
-        0.724_011_718_791_646,
-        0.561_510_219_548_918_2,
-        0.376_746_685_666_572_5,
-        0.313_873_420_677_094,
-        0.243_444_791_401_658_5,
-    );
-
-    GaussObs::with_observer_position(idx_obs, ra, dec, time, observer_helio_position)
-}
-
-/// Force Rayon (if used by downstream code) to a single worker thread.
-/// Must be called before any Rayon pool is created by dependencies.
-fn force_single_thread_pool() {
-    // Pure env-var approach: works even if we don't depend on rayon directly.
-    // Must be set very early, before any rayon usage.
-    std::env::set_var("RAYON_NUM_THREADS", "1");
-
-    // If you prefer hard enforcement and have rayon as a dev-dependency,
-    // you could uncomment this block (but it's optional):
-    //
-    // #[cfg(any())]
-    // {
-    //     let _ = rayon::ThreadPoolBuilder::new()
-    //         .num_threads(1)
-    //         .build_global();
-    //     // Ignore the error if the global pool was already built.
-    // }
-}
-
-fn bench_prelim_orbit(c: &mut Criterion) {
-    // Ensure single-threaded execution before anything else touches Rayon.
-    force_single_thread_pool();
-
-    let mut group = c.benchmark_group("gauss_prelim_orbit");
-
-    // Build global state once (outside hot loops).
-    let state = build_state().expect("Outfit state");
-
-    // Deterministic fixture.
-    let gauss = make_fixture_gaussobs();
-
-    // 1) Single call
-    group.bench_function("single_call", |b| {
-        b.iter(|| {
-            let res = gauss.prelim_orbit(black_box(&state), &IODParams::default());
-            match res {
-                Ok(GaussResult::PrelimOrbit(_)) | Ok(GaussResult::CorrectedOrbit(_)) => {}
-                Err(e) => panic!("prelim_orbit failed: {e:?}"),
-            }
-        })
-    });
-
-    // 2) Batch 100: reuse same input, measure algorithmic cost only
-    group.bench_function("batch_100", |b| {
-        b.iter_batched(
-            || gauss.clone(),
-            |g| {
-                for _ in 0..100 {
-                    let res = g.prelim_orbit(&state, &IODParams::default());
-                    black_box(&res);
-                }
-            },
-            BatchSize::SmallInput,
-        )
-    });
-
-    // 3) Noisy: generate one noisy realization then run prelim_orbit
-    group.bench_function("noisy_single_call", |b| {
-        b.iter_batched(
-            || gauss.clone(),
-            |g| {
-                // 0.3" ≈ 1.454e-6 rad; use your production noise scale if different.
-                let sigma_rad = 1.5e-6_f64;
-                let mut rng = rand::rngs::StdRng::seed_from_u64(42);
-                let noisy = g.generate_noisy_realizations(
-                    &(Vector3::zeros().add_scalar(1.0) * sigma_rad),
-                    &(Vector3::zeros().add_scalar(1.0) * sigma_rad),
-                    100,
-                    1.0,
-                    &mut rng,
-                );
-
-                for gg in noisy {
-                    let res = gg.prelim_orbit(&state, &IODParams::default());
-                    black_box(&res);
-                }
-            },
-            BatchSize::SmallInput,
-        )
-    });
-
-    group.finish();
-}
-
-criterion_group!(gauss_benches, bench_prelim_orbit);
-criterion_main!(gauss_benches);
diff --git a/benches/load_parquet.rs b/benches/load_parquet.rs
deleted file mode 100644
index c3580d1..0000000
--- a/benches/load_parquet.rs
+++ /dev/null
@@ -1,54 +0,0 @@
-use camino::Utf8Path;
-use criterion::Throughput;
-use criterion::{criterion_group, criterion_main, BenchmarkId, Criterion};
-use outfit::error_models::ErrorModel;
-use outfit::outfit::Outfit;
-use outfit::trajectories::trajectory_file::TrajectoryFile;
-use outfit::TrajectorySet;
-
-fn bench_load_parquet(c: &mut Criterion) {
-    let mut outfit = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
-    let path = Utf8Path::new("tests/data/test_from_fink.parquet");
-    let ztf_observer = outfit.get_observer_from_mpc_code(&"I41".into());
-
-    let mut batch_group = c.benchmark_group("batch_sizes");
-
-    for batch_size in [
-        Some(2),
-        Some(4),
-        Some(8),
-        Some(16),
-        Some(32),
-        Some(64),
-        Some(128),
-        Some(256),
-        Some(512),
-        Some(1024),
-        Some(2048),
-        Some(4096),
-        Some(65536),
-    ]
-    .iter()
-    {
-        batch_group.throughput(Throughput::Elements(1));
-        batch_group.bench_with_input(
-            BenchmarkId::from_parameter(format!("{batch_size:?}")),
-            batch_size,
-            |b, batch_size| {
-                b.iter(|| {
-                    let _ = TrajectorySet::new_from_parquet(
-                        &mut outfit,
-                        path,
-                        ztf_observer.clone(),
-                        0.5,
-                        0.5,
-                        *batch_size,
-                    );
-                })
-            },
-        );
-    }
-}
-
-criterion_group!(benches, bench_load_parquet);
-criterion_main!(benches);
diff --git a/benches/outfit_gauss_iod.rs b/benches/outfit_gauss_iod.rs
deleted file mode 100644
index d9acdc2..0000000
--- a/benches/outfit_gauss_iod.rs
+++ /dev/null
@@ -1,122 +0,0 @@
-// benches/outfit_gauss_iod.rs
-
-#[cfg(feature = "jpl-download")]
-mod benches_impl {
-    use std::cell::RefCell;
-
-    use camino::Utf8Path;
-    use criterion::{black_box, BatchSize, Criterion};
-    use outfit::constants::ObjectNumber;
-    use outfit::error_models::ErrorModel;
-    use outfit::initial_orbit_determination::gauss_result::GaussResult;
-    use outfit::initial_orbit_determination::IODParams;
-    use outfit::observations::observations_ext::ObservationIOD;
-    use outfit::outfit::Outfit;
-    use outfit::outfit_errors::OutfitError;
-    use outfit::trajectories::trajectory_file::TrajectoryFile;
-    use outfit::TrajectorySet;
-    use rand::rngs::StdRng;
-    use rand::SeedableRng;
-
-    /// Run Gauss IOD on a single trajectory and return the best orbit + RMS.
-    fn run_iod(
-        env_state: &mut Outfit,
-        traj_set: &mut TrajectorySet,
-        traj_number: &ObjectNumber,
-    ) -> Result<(GaussResult, f64), OutfitError> {
-        let obs = traj_set.get_mut(traj_number).expect("trajectory not found");
-        let mut rng = StdRng::seed_from_u64(42);
-
-        let params = IODParams::builder()
-            .n_noise_realizations(10)
-            .noise_scale(1.1)
-            .max_obs_for_triplets(obs.len())
-            .max_triplets(30)
-            .build()?;
-
-        obs.estimate_best_orbit(env_state, &ErrorModel::FCCT14, &mut rng, ¶ms)
-    }
-
-    /// Prepare environment with DE440 and 3 trajectories.
-    fn prepare_env() -> (Outfit, TrajectorySet, [ObjectNumber; 3]) {
-        let mut env = Outfit::new("horizon:DE440", ErrorModel::FCCT14).expect("Outfit init");
-
-        let mut set =
-            TrajectorySet::new_from_80col(&mut env, Utf8Path::new("tests/data/2015AB.obs"));
-        set.add_from_80col(&mut env, Utf8Path::new("tests/data/8467.obs"));
-        set.add_from_80col(&mut env, Utf8Path::new("tests/data/33803.obs"));
-
-        let ids = [
-            ObjectNumber::String("K09R05F".into()),
-            ObjectNumber::String("8467".into()),
-            ObjectNumber::String("33803".into()),
-        ];
-
-        (env, set, ids)
-    }
-
-    /// End-to-end benchmark.
-    pub fn bench_gauss_iod_e2e(c: &mut Criterion) {
-        c.bench_function("gauss_iod_e2e_all", |b| {
-            b.iter_batched(
-                prepare_env,
-                |(mut env, mut set, ids)| {
-                    for id in &ids {
-                        let res = run_iod(&mut env, &mut set, id).expect("IOD");
-                        black_box(res);
-                    }
-                },
-                BatchSize::SmallInput,
-            )
-        });
-    }
-
-    /// Core benchmark.
-    pub fn bench_gauss_iod_core(c: &mut Criterion) {
-        let (env0, _set_once, _ids) = prepare_env();
-        let env = RefCell::new(env0);
-        let target = ObjectNumber::String("K09R05F".into());
-        let obs_path = Utf8Path::new("tests/data/2015AB.obs");
-
-        c.bench_function("gauss_iod_core_single_refcell", |b| {
-            b.iter_batched(
-                || {
-                    let mut env_borrow = env.borrow_mut();
-                    TrajectorySet::new_from_80col(&mut env_borrow, obs_path)
-                },
-                |mut set| {
-                    let mut env_borrow = env.borrow_mut();
-                    let res = run_iod(&mut env_borrow, &mut set, &target).expect("IOD");
-                    black_box(res);
-                },
-                BatchSize::SmallInput,
-            )
-        });
-    }
-}
-
-#[cfg(feature = "jpl-download")]
-use criterion::{criterion_group, criterion_main, Criterion};
-
-#[cfg(feature = "jpl-download")]
-criterion_group!(
-    name = benches;
-    config = Criterion::default()
-        .sample_size(30)
-        .warm_up_time(std::time::Duration::from_secs(5))
-        .measurement_time(std::time::Duration::from_secs(25))
-        .with_plots();
-    targets = benches_impl::bench_gauss_iod_e2e, benches_impl::bench_gauss_iod_core
-);
-
-#[cfg(feature = "jpl-download")]
-criterion_main!(benches);
-
-// Fallback quand la feature est absente : fournit une main au crate.
-#[cfg(not(feature = "jpl-download"))]
-fn main() {
-    eprintln!(
-        "This benchmark requires the `jpl-download` feature. \
-         Run with: `cargo bench --features jpl-download`"
-    );
-}
diff --git a/benches/solve_kepler_equation.rs b/benches/solve_kepler_equation.rs
deleted file mode 100644
index e6a1af5..0000000
--- a/benches/solve_kepler_equation.rs
+++ /dev/null
@@ -1,161 +0,0 @@
-use criterion::{black_box, criterion_group, criterion_main, BatchSize, Criterion};
-use rand::rngs::StdRng;
-use rand::{Rng, SeedableRng};
-
-use outfit::orbit_type::equinoctial_element::EquinoctialElements;
-
-/// Uniform random in [0, 2π)
-#[inline]
-fn rand_angle(rng: &mut StdRng) -> f64 {
-    let two_pi = std::f64::consts::TAU;
-    rng.random::() * two_pi
-}
-
-/// Build equinoctial elements with only h,k,λ set (others neutral).
-#[inline]
-fn make_equinoctial(h: f64, k: f64, lambda: f64) -> EquinoctialElements {
-    EquinoctialElements {
-        reference_epoch: 59000.0,
-        semi_major_axis: 1.0, // not used here
-        eccentricity_sin_lon: h,
-        eccentricity_cos_lon: k,
-        tan_half_incl_sin_node: 0.0,
-        tan_half_incl_cos_node: 0.0,
-        mean_longitude: lambda,
-    }
-}
-
-/// Adjust λ so that λ >= ϖ, mimicking the production path in solve_two_body_problem.
-#[inline]
-fn align_lambda_with_periapsis(lambda: f64, w: f64) -> f64 {
-    let mut lam = lambda.rem_euclid(std::f64::consts::TAU);
-    let w_mod = w.rem_euclid(std::f64::consts::TAU);
-    if lam < w_mod {
-        lam += std::f64::consts::TAU;
-    }
-    lam
-}
-
-/// Typical regime: e ∈ [0.0, 0.7]
-fn bench_typical(c: &mut Criterion) {
-    let mut rng = StdRng::seed_from_u64(0xDEADBEEF);
-    let samples = 10_000usize;
-
-    c.bench_function("solve_kepler_equation/typical_e<=0.7", |b| {
-        b.iter_batched(
-            || {
-                // Pre-generate inputs to avoid RNG cost in the timed section
-                (0..samples)
-                    .map(|_| {
-                        let e = rng.random_range(0.0..=0.7);
-                        let w = rand_angle(&mut rng);
-                        let lambda = align_lambda_with_periapsis(rand_angle(&mut rng), w);
-                        let h = e * w.sin();
-                        let k = e * w.cos();
-                        (h, k, lambda, w)
-                    })
-                    .collect::>()
-            },
-            |cases| {
-                // Benchmark only the solver calls
-                for (h, k, lambda, w) in cases {
-                    let equ = make_equinoctial(h, k, lambda);
-                    let f = equ
-                        .solve_kepler_equation(black_box(lambda), black_box(w))
-                        .unwrap();
-                    black_box(f);
-                }
-            },
-            BatchSize::LargeInput,
-        )
-    });
-}
-
-/// High-eccentricity (still elliptic): e ∈ [0.7, 0.9]
-fn bench_high_e(c: &mut Criterion) {
-    let mut rng = StdRng::seed_from_u64(0xBADF00D);
-    let samples = 10_000usize;
-
-    c.bench_function("solve_kepler_equation/high_e_0.7..0.9", |b| {
-        b.iter_batched(
-            || {
-                (0..samples)
-                    .map(|_| {
-                        let e = rng.random_range(0.7..0.9);
-                        let w = rand_angle(&mut rng);
-                        let lambda = align_lambda_with_periapsis(rand_angle(&mut rng), w);
-                        let h = e * w.sin();
-                        let k = e * w.cos();
-                        (h, k, lambda, w)
-                    })
-                    .collect::>()
-            },
-            |cases| {
-                for (h, k, lambda, w) in cases {
-                    let equ = make_equinoctial(h, k, lambda);
-                    let _ = equ.solve_kepler_equation(black_box(lambda), black_box(w));
-                }
-            },
-            BatchSize::LargeInput,
-        )
-    });
-}
-
-/// Near-circular regime: e ≈ 1e-12
-fn bench_near_circular(c: &mut Criterion) {
-    let mut rng = StdRng::seed_from_u64(0xFEEDFACE);
-    let samples = 10_000usize;
-    let e = 1e-12;
-
-    c.bench_function("solve_kepler_equation/near_circular_e=1e-12", |b| {
-        b.iter_batched(
-            || {
-                (0..samples)
-                    .map(|_| {
-                        let w = rand_angle(&mut rng);
-                        let lambda = align_lambda_with_periapsis(rand_angle(&mut rng), w);
-                        let h = e * w.sin();
-                        let k = e * w.cos();
-                        (h, k, lambda, w)
-                    })
-                    .collect::>()
-            },
-            |cases| {
-                for (h, k, lambda, w) in cases {
-                    let equ = make_equinoctial(h, k, lambda);
-                    let f = equ
-                        .solve_kepler_equation(black_box(lambda), black_box(w))
-                        .unwrap();
-                    black_box(f);
-                }
-            },
-            BatchSize::LargeInput,
-        )
-    });
-}
-
-/// Fixed “stress” case (from a previous failing input), useful for stability profiling.
-fn bench_fixed_stress(c: &mut Criterion) {
-    // Example numbers; feel free to replace with your own worst-case input.
-    let e = 0.75_f64;
-    let w = -2.823_013_355_485_587_6_f64;
-    let lambda = 5.930_860_541_086_263_f64;
-    let h = e * w.sin();
-    let k = e * w.cos();
-    let lambda = align_lambda_with_periapsis(lambda, w);
-    let equ = make_equinoctial(h, k, lambda);
-
-    c.bench_function("solve_kepler_equation/fixed_stress_case", |b| {
-        b.iter(|| {
-            let f = equ.solve_kepler_equation(black_box(lambda), black_box(w));
-            black_box(f.ok());
-        })
-    });
-}
-
-criterion_group!(
-    name = benches;
-    config = Criterion::default();
-    targets = bench_typical, bench_high_e, bench_near_circular, bench_fixed_stress
-);
-criterion_main!(benches);
diff --git a/examples/gauss_iod_once.rs b/examples/gauss_iod_once.rs
deleted file mode 100644
index d8db3e5..0000000
--- a/examples/gauss_iod_once.rs
+++ /dev/null
@@ -1,95 +0,0 @@
-#![cfg(feature = "jpl-download")]
-use std::env;
-
-use camino::Utf8Path;
-use rand::rngs::StdRng;
-use rand::SeedableRng;
-
-use std::{thread, time::Duration};
-
-use outfit::prelude::*; // Import most common Outfit types and traits
-
-/// Run Gauss IOD on a single trajectory and return the best orbit and RMS.
-///
-/// Arguments
-/// -----------------
-/// * `env_state`: The global environment (ephemeris, EOP, error model).
-/// * `traj_set`: The trajectory container with parsed observations.
-/// * `traj_number`: The object identifier present in `traj_set`.
-///
-/// Return
-/// ----------
-/// * `Ok((Option, f64))` — the best orbit (if any) and its RMS in mas.
-/// * `Err(OutfitError)` — if the IOD pipeline fails.
-///
-/// See also
-/// ------------
-/// * [`ObservationIOD::estimate_best_orbit`] – High-level Gauss IOD entry point.
-/// * [`IODParams`] – Controls triplet selection and stochastic noise.
-/// * [`ErrorModel::FCCT14`] – Default astrometric error model used here.
-fn run_iod_once(
-    env_state: &mut Outfit,
-    traj_set: &mut TrajectorySet,
-    traj_number: &ObjectNumber,
-) -> Result<(GaussResult, f64), OutfitError> {
-    let obs = traj_set
-        .get_mut(traj_number)
-        .expect("trajectory not found in set");
-    let mut rng = StdRng::seed_from_u64(42);
-
-    let params = IODParams::builder()
-        .n_noise_realizations(10)
-        .noise_scale(1.1)
-        .max_obs_for_triplets(obs.len())
-        .max_triplets(30)
-        .build()?;
-
-    obs.estimate_best_orbit(env_state, &ErrorModel::FCCT14, &mut rng, ¶ms)
-}
-
-/// Minimal driver: load three test trajectories, run IOD for the requested object once.
-/// Usage:
-///   gauss_iod_once  [--verbose]
-/// Example:
-///   gauss_iod_once K09R05F --verbose
-fn main() -> Result<(), OutfitError> {
-    let mut args = env::args().skip(1).collect::>();
-    let verbose = if let Some(pos) = args.iter().position(|a| a == "--verbose") {
-        args.remove(pos);
-        true
-    } else {
-        false
-    };
-
-    let object = args
-        .first()
-        .cloned()
-        .unwrap_or_else(|| "K09R05F".to_string());
-    let obj = ObjectNumber::String(object);
-
-    // Warm environment (will read DE440 from cache if already downloaded).
-    let mut env = Outfit::new("horizon:DE440", ErrorModel::FCCT14)?;
-
-    // Parse observations (adjust paths if needed).
-    let mut set = TrajectorySet::new_from_80col(&mut env, Utf8Path::new("tests/data/2015AB.obs"));
-    set.add_from_80col(&mut env, Utf8Path::new("tests/data/8467.obs"));
-    set.add_from_80col(&mut env, Utf8Path::new("tests/data/33803.obs"));
-
-    // Run IOD once for the requested object.
-    let (best, rms) = run_iod_once(&mut env, &mut set, &obj)?;
-
-    thread::sleep(Duration::from_millis(500)); // pause 0,5 s
-
-    // Run IOD once for the requested object.
-    let (best2, rms2) = run_iod_once(&mut env, &mut set, &obj)?;
-
-    if verbose {
-        eprintln!("[gauss_iod_once] object = {obj:?}, rms(mas) = {rms}");
-        eprintln!("[gauss_iod_once] orbit = {:?}", best.get_orbit());
-
-        eprintln!("[gauss_iod_once] object = {obj:?}, rms(mas) = {rms2}");
-        eprintln!("[gauss_iod_once] orbit = {:?}", best2.get_orbit());
-    }
-
-    Ok(())
-}
diff --git a/examples/parquet_to_orbit.rs b/examples/parquet_to_orbit.rs
deleted file mode 100644
index 3f94f8d..0000000
--- a/examples/parquet_to_orbit.rs
+++ /dev/null
@@ -1,659 +0,0 @@
-#![cfg(feature = "jpl-download")]
-#![allow(non_snake_case)]
-use camino::Utf8Path;
-use outfit::trajectories::trajectory_fit::TrajectoryFit;
-use rand::rngs::StdRng;
-use rand::SeedableRng;
-
-use outfit::constants::ObjectNumber;
-use outfit::initial_orbit_determination::gauss_result::GaussResult;
-use std::collections::{BTreeMap, HashMap};
-use std::hash::BuildHasher;
-
-use outfit::prelude::*;
-
-// ======================= orbit classification =======================
-
-/// A coarse taxonomy for small-body orbits in the Solar System.
-#[derive(Debug, Clone, Copy, PartialEq, Eq, PartialOrd, Ord)]
-enum OrbitClass {
-    /// Interior-Earth Objects: a < 1 AU and Q < 0.983 AU (entirely inside Earth's orbit)
-    Atira,
-    /// a < 1 AU and Q > 0.983 AU (crosses Earth's orbit from the inside)
-    Aten,
-    /// a ≥ 1 AU and q ≤ 1.017 AU (Earth-crossing from the outside)
-    Apollo,
-    /// 1.017 < q < 1.3 AU (near-Earth but non-crossing)
-    Amor,
-    /// Near-Earth Object fallback: q < 1.3 AU but not Atira/Aten/Apollo/Amor
-    Neo,
-    Hungaria,
-    MainBelt,
-    Hilda,
-    Centaur,
-    /// Trans-Neptunian Object
-    Tno,
-    /// a < 1 AU (non-Atira/Aten) — inner resonant / Vulcanoid-like
-    Inner,
-    Other,
-}
-
-/// Classify an orbit using simple rules on a, e (→ q, Q) and inclination i (rad).
-///
-/// Rules (coarse):
-/// -----------------
-/// * q = a(1-e), Q = a(1+e)
-/// * **Atira**: a < 1.0 AU and **Q < 0.983 AU** (entirely interior to Earth's orbit)
-/// * **Aten**:  a < 1.0 AU and **Q > 0.983 AU** (Earth-crossing from the inside)
-/// * **Apollo**: a ≥ 1.0 AU and q ≤ 1.017 AU
-/// * **Amor**: 1.017 < q < 1.3 AU
-/// * **NEO**: q < 1.3 AU (and not Atira/Aten/Apollo/Amor)
-/// * **Hungaria**: 1.78 ≤ a ≤ 2.0 AU and i > 16°
-/// * **Hilda**: a ≈ 3.9 AU (here 3.7–4.1 AU)
-/// * **Main belt**: 2.0 ≤ a ≤ 3.5 AU and e < 0.35
-/// * **Centaur**: 5 < a < 30 AU
-/// * **TNO**: a ≥ 30 AU
-/// * **Inner**: a < 1 AU (non-Atira/Aten)
-/// * **Other**: fallback
-fn classify_orbit(a: f64, e: f64, i_rad: f64) -> OrbitClass {
-    let q = a * (1.0 - e);
-    let Q = a * (1.0 + e);
-    let i_deg = i_rad.to_degrees();
-
-    // Use aphelion Q to split Atira vs Aten when a<1 AU
-    if a < 1.0 && Q < 0.983 {
-        return OrbitClass::Atira;
-    }
-    if a < 1.0 && Q > 0.983 {
-        return OrbitClass::Aten;
-    }
-    if a >= 1.0 && q <= 1.017 {
-        return OrbitClass::Apollo;
-    }
-    if q > 1.017 && q < 1.3 {
-        return OrbitClass::Amor;
-    }
-    if q < 1.3 {
-        return OrbitClass::Neo;
-    }
-
-    if (1.78..=2.0).contains(&a) && i_deg > 16.0 {
-        return OrbitClass::Hungaria;
-    }
-    if (3.7..=4.1).contains(&a) {
-        return OrbitClass::Hilda;
-    }
-    if (2.0..=3.5).contains(&a) && e < 0.35 {
-        return OrbitClass::MainBelt;
-    }
-    if (5.0..30.0).contains(&a) {
-        return OrbitClass::Centaur;
-    }
-    if a >= 30.0 {
-        return OrbitClass::Tno;
-    }
-    if a < 1.0 {
-        return OrbitClass::Inner;
-    }
-    OrbitClass::Other
-}
-
-/// Extract a reference to `KeplerianElements` from a `GaussResult` if available.
-fn kepler_of(res: &GaussResult) -> Option<&outfit::KeplerianElements> {
-    match res {
-        GaussResult::CorrectedOrbit(k) => k.as_keplerian(),
-        GaussResult::PrelimOrbit(k) => k.as_keplerian(),
-    }
-}
-
-// ======================= reporting structs =======================
-
-#[derive(Debug, Clone)]
-struct ErrorStats {
-    count: usize,
-    samples: Vec,
-    attempts_sum: usize,
-    attempts_n: usize,
-}
-
-#[derive(Debug, Clone)]
-struct OrbitElementStats {
-    // distribution statistics for successes
-    a_min: f64,
-    a_max: f64,
-    a_mean: f64,
-    a_median: f64,
-    a_p95: f64,
-    e_min: f64,
-    e_max: f64,
-    e_mean: f64,
-    e_median: f64,
-    e_p95: f64,
-    i_min: f64,
-    i_max: f64,
-    i_mean: f64,
-    i_median: f64,
-    i_p95: f64, // radians
-    q_min: f64,
-    q_max: f64,
-    q_mean: f64,
-    q_median: f64,
-    q_p95: f64,
-    Q_min: f64,
-    Q_max: f64,
-    Q_mean: f64,
-    Q_median: f64,
-    Q_p95: f64,
-    // class counts
-    class_counts: BTreeMap,
-}
-
-#[derive(Debug, Clone)]
-struct IodBatchSummary {
-    total_objects: usize,
-    succeeded_total: usize,
-    corrected_count: usize,
-    prelim_count: usize,
-    failed_total: usize,
-
-    // RMS stats on successes
-    rms_min: f64,
-    rms_max: f64,
-    rms_mean: f64,
-    rms_median: f64,
-    rms_p95: f64,
-
-    // Attempts aggregated from NoViableOrbit
-    attempts_sum: usize,
-    attempts_mean: f64,
-    attempts_p95: f64,
-
-    // Errors (stable kind → stats)
-    error_stats: BTreeMap<&'static str, ErrorStats>,
-
-    // Orbit elements & classes (only successes)
-    elements: Option,
-
-    // Top/bottom objects by RMS
-    best_k: Vec<(ObjectNumber, f64)>,
-    worst_k: Vec<(ObjectNumber, f64)>,
-}
-
-// ======================= summarizer =======================
-#[allow(clippy::type_complexity)]
-fn summarize_estimates(
-    results: &HashMap, S>,
-    k: usize,
-) -> IodBatchSummary
-where
-    S: BuildHasher,
-{
-    const MAX_SAMPLES_PER_KIND: usize = 3;
-
-    let mut rms_values: Vec<(ObjectNumber, f64, bool)> = Vec::new();
-    let mut corrected_count = 0usize;
-    let mut prelim_count = 0usize;
-
-    let mut buckets: BTreeMap<&'static str, ErrorStats> = BTreeMap::new();
-    let mut attempts_all: Vec = Vec::new();
-
-    // collect successful orbit elements
-    let mut a: Vec = Vec::new();
-    let mut e: Vec = Vec::new();
-    let mut i: Vec = Vec::new();
-    let mut q: Vec = Vec::new();
-    let mut Q: Vec = Vec::new();
-    let mut class_counts: BTreeMap = BTreeMap::new();
-
-    for (obj, res) in results {
-        match res {
-            Ok((orbit_res, rms)) => {
-                let corrected = matches!(orbit_res, GaussResult::CorrectedOrbit(_));
-                if corrected {
-                    corrected_count += 1;
-                } else {
-                    prelim_count += 1;
-                }
-                rms_values.push((obj.clone(), *rms, corrected));
-
-                if let Some(kep) = kepler_of(orbit_res) {
-                    let a_au = kep.semi_major_axis;
-                    let e_ = kep.eccentricity;
-                    let i_rad = kep.inclination;
-                    let q_au = a_au * (1.0 - e_);
-                    let Q_au = a_au * (1.0 + e_);
-                    a.push(a_au);
-                    e.push(e_);
-                    i.push(i_rad);
-                    q.push(q_au);
-                    Q.push(Q_au);
-
-                    let cls = classify_orbit(a_au, e_, i_rad);
-                    *class_counts.entry(cls).or_default() += 1;
-                }
-            }
-            Err(e) => {
-                let (stable_key, sample_msg, attempts) = flatten_error_for_bucket(e);
-                let entry = buckets.entry(stable_key).or_insert_with(|| ErrorStats {
-                    count: 0,
-                    samples: Vec::new(),
-                    attempts_sum: 0,
-                    attempts_n: 0,
-                });
-                entry.count += 1;
-                if let Some(n) = attempts {
-                    entry.attempts_sum += n;
-                    entry.attempts_n += 1;
-                    attempts_all.push(n);
-                }
-                if entry.samples.len() < MAX_SAMPLES_PER_KIND {
-                    entry.samples.push(sample_msg);
-                }
-            }
-        }
-    }
-
-    let total_objects = results.len();
-    let succeeded_total = corrected_count + prelim_count;
-    let failed_total = total_objects.saturating_sub(succeeded_total);
-
-    // ----- RMS stats
-    let mut rms_only: Vec = rms_values.iter().map(|(_, r, _)| *r).collect();
-    rms_only.sort_by(|a, b| a.partial_cmp(b).unwrap());
-    let (rms_min, rms_max, rms_mean, rms_median, rms_p95) = if rms_only.is_empty() {
-        (f64::NAN, f64::NAN, f64::NAN, f64::NAN, f64::NAN)
-    } else {
-        let min = *rms_only.first().unwrap();
-        let max = *rms_only.last().unwrap();
-        let mean = rms_only.iter().sum::() / (rms_only.len() as f64);
-        let median = percentile_sorted(&rms_only, 50.0);
-        let p95 = percentile_sorted(&rms_only, 95.0);
-        (min, max, mean, median, p95)
-    };
-
-    // ----- attempts stats
-    attempts_all.sort_unstable();
-    let attempts_sum = attempts_all.iter().copied().sum::();
-    let attempts_mean = if attempts_all.is_empty() {
-        f64::NAN
-    } else {
-        attempts_sum as f64 / attempts_all.len() as f64
-    };
-    let attempts_p95 = if attempts_all.is_empty() {
-        f64::NAN
-    } else {
-        percentile_sorted_usize(&attempts_all, 95.0) as f64
-    };
-
-    // ----- orbit element stats
-    let elements = if a.is_empty() {
-        None
-    } else {
-        a.sort_by(|x, y| x.partial_cmp(y).unwrap());
-        e.sort_by(|x, y| x.partial_cmp(y).unwrap());
-        i.sort_by(|x, y| x.partial_cmp(y).unwrap());
-        q.sort_by(|x, y| x.partial_cmp(y).unwrap());
-        Q.sort_by(|x, y| x.partial_cmp(y).unwrap());
-
-        let a_stats = (
-            a[0],
-            *a.last().unwrap(),
-            mean(&a),
-            percentile_sorted(&a, 50.0),
-            percentile_sorted(&a, 95.0),
-        );
-        let e_stats = (
-            e[0],
-            *e.last().unwrap(),
-            mean(&e),
-            percentile_sorted(&e, 50.0),
-            percentile_sorted(&e, 95.0),
-        );
-        let i_stats = (
-            i[0],
-            *i.last().unwrap(),
-            mean(&i),
-            percentile_sorted(&i, 50.0),
-            percentile_sorted(&i, 95.0),
-        );
-        let q_stats = (
-            q[0],
-            *q.last().unwrap(),
-            mean(&q),
-            percentile_sorted(&q, 50.0),
-            percentile_sorted(&q, 95.0),
-        );
-        let Q_stats = (
-            Q[0],
-            *Q.last().unwrap(),
-            mean(&Q),
-            percentile_sorted(&Q, 50.0),
-            percentile_sorted(&Q, 95.0),
-        );
-
-        Some(OrbitElementStats {
-            a_min: a_stats.0,
-            a_max: a_stats.1,
-            a_mean: a_stats.2,
-            a_median: a_stats.3,
-            a_p95: a_stats.4,
-            e_min: e_stats.0,
-            e_max: e_stats.1,
-            e_mean: e_stats.2,
-            e_median: e_stats.3,
-            e_p95: e_stats.4,
-            i_min: i_stats.0,
-            i_max: i_stats.1,
-            i_mean: i_stats.2,
-            i_median: i_stats.3,
-            i_p95: i_stats.4,
-            q_min: q_stats.0,
-            q_max: q_stats.1,
-            q_mean: q_stats.2,
-            q_median: q_stats.3,
-            q_p95: q_stats.4,
-            Q_min: Q_stats.0,
-            Q_max: Q_stats.1,
-            Q_mean: Q_stats.2,
-            Q_median: Q_stats.3,
-            Q_p95: Q_stats.4,
-            class_counts,
-        })
-    };
-
-    // ----- Top/Bottom K by RMS
-    rms_values.sort_by(|a, b| a.1.partial_cmp(&b.1).unwrap());
-    let best_k = rms_values
-        .iter()
-        .take(k)
-        .map(|(o, r, _)| (o.clone(), *r))
-        .collect();
-    let worst_k = rms_values
-        .iter()
-        .rev()
-        .take(k)
-        .map(|(o, r, _)| (o.clone(), *r))
-        .collect();
-
-    IodBatchSummary {
-        total_objects,
-        succeeded_total,
-        corrected_count,
-        prelim_count,
-        failed_total,
-        rms_min,
-        rms_max,
-        rms_mean,
-        rms_median,
-        rms_p95,
-        attempts_sum,
-        attempts_mean,
-        attempts_p95,
-        error_stats: buckets,
-        elements,
-        best_k,
-        worst_k,
-    }
-}
-
-// ======================= printer =======================
-
-fn print_summary(sum: &IodBatchSummary) {
-    println!("\n=== IOD Batch Summary ===");
-    println!("Objects total ........ : {}", sum.total_objects);
-    println!(
-        "  Success total ...... : {}  (Corrected: {}, Prelim: {})",
-        sum.succeeded_total, sum.corrected_count, sum.prelim_count
-    );
-    println!("  Failures total ..... : {}", sum.failed_total);
-
-    println!("\n-- RMS on successes --");
-    println!(
-        "  min / median / mean / p95 / max : {:.6} / {:.6} / {:.6} / {:.6} / {:.6}",
-        sum.rms_min, sum.rms_median, sum.rms_mean, sum.rms_p95, sum.rms_max
-    );
-
-    if let Some(el) = &sum.elements {
-        println!("\n-- Orbit elements (successes only) --");
-        println!(
-            "  a [AU]  : min={:.6}  median={:.6}  mean={:.6}  p95={:.6}  max={:.6}",
-            el.a_min, el.a_median, el.a_mean, el.a_p95, el.a_max
-        );
-        println!(
-            "  e [-]   : min={:.6}  median={:.6}  mean={:.6}  p95={:.6}  max={:.6}",
-            el.e_min, el.e_median, el.e_mean, el.e_p95, el.e_max
-        );
-        println!(
-            "  i [deg] : min={:.6}  median={:.6}  mean={:.6}  p95={:.6}  max={:.6}",
-            el.i_min.to_degrees(),
-            el.i_median.to_degrees(),
-            el.i_mean.to_degrees(),
-            el.i_p95.to_degrees(),
-            el.i_max.to_degrees()
-        );
-        println!(
-            "  q [AU]  : min={:.6}  median={:.6}  mean={:.6}  p95={:.6}  max={:.6}",
-            el.q_min, el.q_median, el.q_mean, el.q_p95, el.q_max
-        );
-        println!(
-            "  Q [AU]  : min={:.6}  median={:.6}  mean={:.6}  p95={:.6}  max={:.6}",
-            el.Q_min, el.Q_median, el.Q_mean, el.Q_p95, el.Q_max
-        );
-
-        println!("\n-- Orbit classes (counts) --");
-        if el.class_counts.is_empty() {
-            println!("  (none)");
-        } else {
-            for (cls, cnt) in &el.class_counts {
-                println!("  {:<10} : {}", format!("{cls:?}"), cnt);
-            }
-        }
-    } else {
-        println!("\n-- Orbit elements --\n  (no successful orbits)");
-    }
-
-    println!("\n-- Failure breakdown (by error kind) --");
-    if sum.error_stats.is_empty() {
-        println!("  (none)");
-    } else {
-        for (kind, stats) in &sum.error_stats {
-            let attempts_avg = if stats.attempts_n > 0 {
-                stats.attempts_sum as f64 / stats.attempts_n as f64
-            } else {
-                f64::NAN
-            };
-            println!(
-                "  {:<28} : {:>4}   attempts(sum/avg on carrying) = {}/{}",
-                kind,
-                stats.count,
-                stats.attempts_sum,
-                fmt_opt(attempts_avg)
-            );
-            for (i, sample) in stats.samples.iter().take(3).enumerate() {
-                println!("      · example[{i}] {sample}");
-            }
-        }
-    }
-
-    println!("\n-- Attempts (global from NoViableOrbit) --");
-    if sum.attempts_sum == 0 && sum.failed_total > 0 {
-        println!("  (no attempts recorded in errors)");
-    } else if sum.failed_total == 0 {
-        println!("  (no failures)");
-    } else {
-        println!(
-            "  sum / mean / p95 : {} / {:.2} / {:.0}",
-            sum.attempts_sum, sum.attempts_mean, sum.attempts_p95
-        );
-    }
-
-    println!("\n-- Best by RMS --");
-    if sum.best_k.is_empty() {
-        println!("  (no successes)");
-    } else {
-        for (obj, rms) in &sum.best_k {
-            println!("  {:>8}  rms={:.6}", display_obj(obj), rms);
-        }
-    }
-
-    println!("\n-- Worst by RMS --");
-    if sum.worst_k.is_empty() {
-        println!("  (no successes)");
-    } else {
-        for (obj, rms) in &sum.worst_k {
-            println!("  {:>8}  rms={:.6}", display_obj(obj), rms);
-        }
-    }
-    println!();
-}
-
-// ======================= small helpers =======================
-
-fn flatten_error_for_bucket(e: &OutfitError) -> (&'static str, String, Option) {
-    use OutfitError::*;
-    match e {
-        NoViableOrbit { cause, attempts } => {
-            let (k, _, _) = flatten_error_for_bucket(cause);
-            (k, format!("{e}"), Some(*attempts))
-        }
-        NoFeasibleTriplets { .. } => ("NoFeasibleTriplets", format!("{e}"), None),
-
-        // Numerical / algebraic failures
-        GaussNoRootsFound => ("GaussNoRootsFound", format!("{e}"), None),
-        PolynomialRootFindingFailed => ("PolynomialRootFindingFailed", format!("{e}"), None),
-        SpuriousRootDetected => ("SpuriousRootDetected", format!("{e}"), None),
-        SingularDirectionMatrix => ("SingularDirectionMatrix", format!("{e}"), None),
-        RmsComputationFailed(_) => ("RmsComputationFailed", format!("{e}"), None),
-        GaussPrelimOrbitFailed(_) => ("GaussPrelimOrbitFailed", format!("{e}"), None),
-        RootFindingError(_) => ("RootFindingError", format!("{e}"), None),
-        InvalidFloatValue(_) => ("InvalidFloatValue", format!("{e}"), None),
-        NonFiniteScore(_) => ("NonFiniteScore", format!("{e}"), None),
-
-        // Orbit / reference frame
-        InvalidOrbit(_) => ("InvalidOrbit", format!("{e}"), None),
-        InvalidIODParameter(_) => ("InvalidIODParameter", format!("{e}"), None),
-        InvalidConversion(_) => ("InvalidConversion", format!("{e}"), None),
-        InvalidRefSystem(_) => ("InvalidRefSystem", format!("{e}"), None),
-        VelocityCorrectionError(_) => ("VelocityCorrectionError", format!("{e}"), None),
-
-        // Observation handling
-        ObservationNotFound(_) => ("ObservationNotFound", format!("{e}"), None),
-
-        // Parsing / ingestion
-        NomParsingError(_) => ("NomParsingError", format!("{e}"), None),
-        Parsing80ColumnFileError(_) => ("Parsing80ColumnFileError", format!("{e}"), None),
-        Parquet(_) => ("Parquet", format!("{e}"), None),
-
-        // Error model
-        InvalidErrorModel(_) => ("InvalidErrorModel", format!("{e}"), None),
-        InvalidErrorModelFilePath(_) => ("InvalidErrorModelFilePath", format!("{e}"), None),
-
-        // Ephemerides / SPK
-        InvalidJPLStringFormat(_) => ("InvalidJPLStringFormat", format!("{e}"), None),
-        InvalidJPLEphemFileSource(_) => ("InvalidJPLEphemFileSource", format!("{e}"), None),
-        InvalidJPLEphemFileVersion(_) => ("InvalidJPLEphemFileVersion", format!("{e}"), None),
-        JPLFileNotFound(_) => ("JPLFileNotFound", format!("{e}"), None),
-        InvalidSpkDataType(_) => ("InvalidSpkDataType", format!("{e}"), None),
-
-        // I/O
-        IoError(_) => ("IoError", format!("{e}"), None),
-        UreqHttpError(_) => ("UreqHttpError", format!("{e}"), None),
-        #[cfg(feature = "jpl-download")]
-        ReqwestError(_) => ("ReqwestError", format!("{e}"), None),
-        Utf8PathError(_) => ("Utf8PathError", format!("{e}"), None),
-        UnableToCreateBaseDir(_) => ("UnableToCreateBaseDir", format!("{e}"), None),
-        InvalidUrl(_) => ("InvalidUrl", format!("{e}"), None),
-
-        // Stochastic
-        NoiseInjectionError(_) => ("NoiseInjectionError", format!("{e}"), None),
-    }
-}
-
-fn percentile_sorted(sorted: &[f64], p: f64) -> f64 {
-    if sorted.is_empty() {
-        return f64::NAN;
-    }
-    let q = p.clamp(0.0, 100.0);
-    let idx = ((q / 100.0) * ((sorted.len() - 1) as f64)).round() as usize;
-    sorted[idx]
-}
-
-fn percentile_sorted_usize(sorted: &[usize], p: f64) -> usize {
-    if sorted.is_empty() {
-        return 0;
-    }
-    let q = p.clamp(0.0, 100.0);
-    let idx = ((q / 100.0) * ((sorted.len() - 1) as f64)).round() as usize;
-    sorted[idx]
-}
-
-fn mean(v: &[f64]) -> f64 {
-    if v.is_empty() {
-        f64::NAN
-    } else {
-        v.iter().sum::() / v.len() as f64
-    }
-}
-
-fn display_obj(id: &ObjectNumber) -> String {
-    match id {
-        ObjectNumber::Int(n) => format!("{n}"),
-        ObjectNumber::String(s) => s.clone(),
-    }
-}
-
-fn fmt_opt(x: f64) -> String {
-    if x.is_finite() {
-        format!("{x:.2}")
-    } else {
-        "-".to_string()
-    }
-}
-
-fn main() -> Result<(), OutfitError> {
-    let mut env_state = Outfit::new("horizon:DE440", ErrorModel::FCCT14).unwrap();
-
-    let test_data = "tests/data/test_from_fink.parquet";
-
-    println!("Loading observations from {test_data}");
-    let path_file = Utf8Path::new(test_data);
-
-    let ztf_observer = env_state.get_observer_from_mpc_code(&"I41".into());
-
-    let mut traj_set =
-        TrajectorySet::new_from_parquet(&mut env_state, path_file, ztf_observer, 0.5, 0.5, None)?;
-
-    println!(
-        "Loading done: {} trajectories / {} observations",
-        traj_set.len(),
-        traj_set.total_observations()
-    );
-
-    println!("Trajectory Set statistics:");
-    println!(
-        "{:#}",
-        traj_set.obs_count_stats().expect("TrajSet is empty")
-    );
-    println!("--------------------------\n");
-
-    let mut rng = StdRng::from_os_rng();
-
-    let params = IODParams::builder()
-        .n_noise_realizations(10)
-        .noise_scale(1.1)
-        .max_obs_for_triplets(12)
-        .max_triplets(30)
-        .build()?;
-
-    println!("Estimating orbits with params: {params:#}");
-    println!("Orbit estimation in progress... (this may take a while)");
-
-    let orbits = traj_set.estimate_all_orbits(&env_state, &mut rng, ¶ms);
-
-    println!("Orbit estimation done.");
-
-    let summary = summarize_estimates(&orbits, 5);
-    print_summary(&summary);
-
-    Ok(())
-}
diff --git a/src/initial_orbit_determination/mod.rs b/src/initial_orbit_determination/mod.rs
index c63f45f..a66a392 100644
--- a/src/initial_orbit_determination/mod.rs
+++ b/src/initial_orbit_determination/mod.rs
@@ -255,11 +255,6 @@ pub struct IODParams {
     pub newton_max_it: usize,
     /// Maximum allowed imaginary part magnitude for complex roots promoted to real (AU).
     pub root_imag_eps: f64,
-
-    // --- Multi-threading (if enabled) ---
-    #[cfg(feature = "parallel")]
-    /// Number of trajectory batches to process in parallel (if `> 1` and `rayon` feature enabled).
-    pub batch_size: usize,
 }
 
 impl IODParams {
@@ -341,10 +336,6 @@ impl Default for IODParams {
             newton_eps: 1.0e-10,
             newton_max_it: 50,
             root_imag_eps: 1.0e-6,
-
-            // Multi-threading (if enabled)
-            #[cfg(feature = "parallel")]
-            batch_size: 4,
         }
     }
 }
@@ -465,13 +456,6 @@ impl IODParamsBuilder {
         self
     }
 
-    // --- Multi-threading (if enabled) ---
-    #[cfg(feature = "parallel")]
-    pub fn batch_size(mut self, v: usize) -> Self {
-        self.params.batch_size = v;
-        self
-    }
-
     // ---- Numeric helpers for PartialOrd (handle NaN as invalid) ----
 
     /// Return true iff x > 0.0 and comparable (i.e., not NaN).
@@ -780,16 +764,6 @@ impl fmt::Display for IODParams {
                 "Max Gauss solutions kept"
             )?;
 
-            // --- Multi-threading (if enabled) ---
-            #[cfg(feature = "parallel")]
-            {
-                line!(
-                    "batch_size           = {}",
-                    self.batch_size,
-                    "Number of trajectory batches to process in parallel"
-                )?;
-            }
-
             Ok(())
         } else {
             write!(
diff --git a/src/outfit_errors.rs b/src/outfit_errors.rs
index c78e691..6f403c2 100644
--- a/src/outfit_errors.rs
+++ b/src/outfit_errors.rs
@@ -230,9 +230,6 @@ pub enum OutfitError {
     #[error("Gauss preliminary orbit determination failed: {0}")]
     GaussPrelimOrbitFailed(String),
 
-    #[error(transparent)]
-    Parquet(#[from] parquet::errors::ParquetError),
-
     #[error("No viable orbit could be determined after {attempts} attempts: {cause}")]
     NoViableOrbit {
         cause: Box,
@@ -296,7 +293,6 @@ impl PartialEq for OutfitError {
             (UreqHttpError(_), UreqHttpError(_)) => true,
             (IoError(_), IoError(_)) => true,
             (ReqwestError(_), ReqwestError(_)) => true,
-            (Parquet(_), Parquet(_)) => true,
 
             (UnableToCreateBaseDir(a), UnableToCreateBaseDir(b)) => a == b,
             (Utf8PathError(a), Utf8PathError(b)) => a == b,
diff --git a/tests/data/test_data_traj_str.parquet b/tests/data/test_data_traj_str.parquet
new file mode 100644
index 0000000000000000000000000000000000000000..52300babe06ae47dc1cd9e0e8b9cd87260352f8e
GIT binary patch
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