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[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:
http://adsabs.harvard.edu/abs/2013PASP..125.1514M
Bibcode:
2014ascl.soft02021M

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ascl:1402.021
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