[ascl:1402.021]
PyGFit: Python Galaxy Fitter
PyGFit measures PSF-matched photometry from images with disparate pixel scales and PSF sizes; its primary purpose is to extract robust spectral energy distributions (SEDs) from crowded images. It fits blended sources in crowded, low resolution images with models generated from a higher resolution image, thus minimizing the impact of crowding and also yielding consistently measured fluxes in different filters which minimizes systematic uncertainty in the final SEDs.
- Code site:
-
http://www.baryons.org/pygfit/
- Described in:
-
https://ui.adsabs.harvard.edu/abs/2013PASP..125.1514M
- Bibcode:
- 2014ascl.soft02021M