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Could you provide some narrative documentation for the returns from fit_im?
crowdsource/crowdsource/crowdsource_base.py
Lines 695 to 696 in d0bb2eb
| res = (stars, model+sky, sky+msky, psf) | |
| return res |
My attempt:
starsis the star catalogmodel + skyis the sum of the stellar model and the "background" modelsky + mskyis the .... sky model? It's low-resolution. I'm not sure how to differentiatesky,msky, andmodel, though I suspectmodelis the stars-only image?psfis the fitted PSF (or the original PSF if refitting isn't used)
Which return value would you consider the best representation of the star-subtracted image? i.e., the best representation of the extended emission?
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