starbug2 0.2.6

JWST PSF photometry in complex crowded fields.

StarBugII

JWST PSF photometry in dusty crowded fields. Last updated: v0.2.6

GitHUB: https://github.com/conornally/starbug2

PYPI: https://pypi.org/project/starbug2

Installation

pip install starbug2

--- OR ---

git clone https://github.com/conornally/starbug2.git
python -m build
pip install .

After the package is installed, there are a few steps required to initialise Starbug.

WEBBPSF Is a dependency of Starbug that has its own initialisation process. The full installation is documented on https://webbpsf.readthedocs.io/en/latest/installation.html however it requires two main steps. Download the data file on the website, named something like webbpsf-data-X.X.X.tar.gz and expand it into a directory, then add append to your .bashrc (or equivalent) export "WEBBPSF=PATH/TO/DIRECTORY".

PSFDIR This is the folder where starbug stores its relevant data files. By default this is "${HOME}/.local/share/starbug". Make sure this folder exists, or if you wish to save them elsewhere, change the folder (permanently) in "starbug2/starbug2/param/default.param [PSFDIR]", or (temporarily) in a local starbug.param file.

PSF FILES Starbug requires PSF files to be generated for the filters you are using. To do so, run starbug2 --generate-psf and they will be generated into "PSFDIR"

Usage

Starbug II - JWST PSF photometry
usage: starbug2 [-ABCDfhMPv] [-b bgdfile] [-d apfile] [-o directory] [-p file.param] [-s opt=val] image.fits ...
   -A  --artific         : run artificial star tests
   -B  --background      : run background estimation
   -b  --bgdfile         : load background (-bgd.fits) file
   -C  --clean           : run source cleaning before photometry 
   -d  --apfile  ap.fits : load a source detection (-ap.fits) file to skip the source detection step
   -D  --detect          : run source detection
   -f  --find            : attempt to find associated -ap -bgd files
   -h  --help            : display uasage information
   -M  --match           : match outputs from all input image files
   -n  --ncores      num : number of CPU cores to split process between
   -o  --output      dir : output directory
   -p  --param   a.param : load parameter file
   -P  --photom          : run psf photometry
   -s  --set      option : set value in parameter file at runtime (-s SIGSKY=3)
   -v  --verbose         : display verbose outputs

   --> Single run commands
       --init          (in prep.) : Initialise starbug into system
       --generate-psf             : Generate ALL the PSF files to "PSFDIR"
       --local-param              : Make a local copy of the default parameter file
       --generate-region   a.fits : Make a ds9 region file with a detection file
       --clean-table       a.fits : Clean up an individual table
       --generate-run      *.fits : Generate a simple run script
       --version                  : Print starbug2 version

See starbug-manual.pdf for more detailed instructions.