• Detect deeply dust-embedded sources in NIRCam and MIRI images
• Full suite of photometry tools
• Powerful modular and simple GNU Linux standard command line interface
StarbugII requires webbpsf installed on the system to function fully.
$~ pip install starbug2
$~ starbug2 --initImportant
If you make use of StarbugII in any published or presented work, please include a citation.
StarbugII uses methods and datatypes from astropy and photutils, please acknowledge them accordingly.
See the full documentation for the complete installation and detailed guides to using the photometric routines. Basic usage information is produced by running:
StarbugII - JWST PSF photometry
usage: starbug2 [-ABDfGhMPSv] [-b bgdfile] [-d apfile] [-n ncores] [-o ouput] [-p file.param] [-s opt=val] image.fits ...
-A --apphot : run aperture photometry on a source list
-B --background : run background estimation
-D --detect : run source detection
-G --geom : calculate geometric stats on source list
-M --match : match outputs from all input image files
-P --psf : run psf photometry
-S --subbgd : subtract background from image
-b --bgdfile : load background (-bgd.fits) file
-d --apfile ap.fits : load a source detection (-ap.fits) file to skip the source detection step
-f --find : attempt to find associated -ap -bgd files
-h --help : display uasage information
-n --ncores num : number of CPU cores to split process between
-o --output dir : output directory
-p --param a.param : load parameter file
-s --set option : set value in parameter file at runtime (-s SIGSKY=3)
-v --verbose : display verbose outputs
--> Single run commands
--init : Initialise Starbug (post install)
--local-param : Make a local copy of the default parameter file
--update-param : Update an out-of-date local parameter file
--generate-psf : Generate a single PSF. Set FILTER, DET_NAME, PSF_SIZE with -s
--generate-region a.fits : Make a ds9 region file with a detection file
--generate-run *.fits : Generate a simple run script
--version : Print starbug2 version
--apply-zeropint a.fits : Apply a zeropoint (-s ZP_MAG=1.0) to a.fits
--calc-instr-zp a.fits : Calculate and apply an instrumental zero point onto a.fits
--> typical runs
$~ starbug2 -vD -p file.param image.fits //Source detect on image with a parameter file
$~ starbug2 -vDM -n4 images*.fits //Source detect and match outputs of a list of images
$~ starbug2 -vd image-ap.fits -BP image.fits //PSF photometry on an image with a source file (image-ap.fits)
To see more detailed information on an option, run [OPTION] --help:
$~ starbug2 -D --help
See https://starbug2.readthedocs.io for full documentation.StarbugII Matching
usage: starbug2-match [-BCGfhvX] [-e column] [-m mask] [-o output] [-p file.param] [-s KEY=VAL] table.fits ...
-B --band : match in "BAND" mode (does not preserve a column for every frame)
-C --cascade : match in "CASCADE" mode (left justify columns)
-G --generic : match in "GENERIC" mode
-X --exact : match in "EXACTVALUE" mode
-e --error column : photometric error column ("eflux" or "stdflux")
-f --full : export full catalogue
-h --help : show help message
-m --mask eval : column evaluation to mask out of matching e.g. -m"~np.isnan(F444W)"
-o --output file.fits : output matched catalogue
-p --param file.param : load starbug parameter file
-s --set option : set value in parameter file at runtime (-s MATCH_THRESH=1)
-v --verbose : display verbose outputs
--band-depr : match in "old" band mode
--> typical runs
$~ starbug2-match -Gfo outfile.fits tab1.fits tab2.fits
$~ starbug2-match -sMATCH_THRESH=0.2 -sBRIDGE_COL=F444W -Bo out.fits F*W.fits