Marcus Hughes
Marcus Hughes
As mentioned in #93 , the model gets zeroed out or set to NaNs so that when it is applied it produces blank regions of the corrected image. - [...
As identified in #93, there is little way to know which stars are used when building a model. - [ ] Create a response from building a model that shows...
Before passing from Python to C, we could convert any integer or wrong endianness patch to the right format. That would remove a hazard from the user.
It would be good to create a guide for new users on how to adjust parameters (psf window size, target psf parameters, alpha, epsilon, etc.) to deal with commonly seen...
When this package was `astropy` affiliated, @WilliamJamieson suggested we transition the functional model fitting from `lmfit` to `astropy.modeling`. This has the benefit of removing a dependency from the package since...
Pickles are inherently unsafe and can have portability issues. We should use a different format. I'm unsure what is a better alternative off-hand. https://github.com/punch-mission/regularizepsf/blob/ded2c7b0cc4790e6f4b690214c1d2288aea78448/regularizepsf/corrector.py#L165-L172
I believe the process of extracting all the stars from an image could be parallelized using Dask. This would speed up model building. In general, we should optimize the model...
As it works right now, you only get the model back and no information about the process building the model. For example, it would potentially be good to know how...
It takes a while to build a model from many images. It would be nice to know how long you have left. We could use `tqdm` or some other tool...