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That the models are based on the astropy modeling framework.
The users should be directed to the astropy modeling pages for more help on using these models.
One especially important point that should be documented up front: calling the object with a phase angle produces the phase corrected absolute magnitude.
That the models do not include rh and delta corrections, i.e., they do not produce apparent magnitudes.
These two points could be illustrated with an example that plots apparent magnitude versus time. Perhaps a simplified version of the following:
I believe the distance correction is built-in. If one passes a DataClass object that contains rh and/or delta fields as input to the object, then the appropriate correction will be applied behind the scene. I will double-check and make this clear in the docstrings.
The documentation, particularly https://sbpy.readthedocs.io/en/stable/sbpy/photometry.html, but also the class docstrings, seems to be missing two key concepts regarding the disk integrated phase function models:
These two points could be illustrated with an example that plots apparent magnitude versus time. Perhaps a simplified version of the following:
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