AstroPhot
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A fast, flexible, automated, and differentiable astronomical image 2D forward modelling tool for precise parallel multi-wavelength photometry
**Is your feature request related to a problem? Please describe.** For data which is in the very low SNR domain, where individual photon/electron counts are discernable, the proper likelihood model...
I'm not sure if this is more a request for guidance or a real feature request. I'm interested in trialing a 2D PSF model, but not (yet) brave enough to...
Writing this at the same time as Issue #196 Please can i check that what is extracted as node['flux'].value is in fact log(flux), and not flux? I think this is...
Once again let me say that i am blown away by the power of this wonderful tool. So much ***fun***. I am currently working to build an image calibration pipeline,...
**Is your feature request related to a problem? Please describe.** In models such as Sersic there is a very strong covariance between `n`, `Re`, and `Ie`. This strong covariance may...
**Is your feature request related to a problem? Please describe.** I should have a unit test to ensure this works int he basic version
**Is your feature request related to a problem? Please describe.** Some images are too large to fit at native resolution, other images are large and the object is also large...
**Is your feature request related to a problem? Please describe.** AstroPhot can fit PSF models live, but we need to be able to account for complex features of emperical PSFs....
Fair enough and beyond the scope here. Probably something to add to the documentation of specifying models. _Originally posted by @wmwv in https://github.com/Autostronomy/AstroPhot/pull/116#discussion_r1338934765_
**Is your feature request related to a problem? Please describe.** Current WCS support doesn't support SIP **Describe the solution you'd like** Add a SIP option to the WCS class. Either...