Open mkelley opened 1 year ago
Thanks to @talister for the initial feedback. No good deed goes unpunished, so may ask you to review the updates 😸
The users should be directed to the astropy modeling pages for more help on using these models.
This is done near the fitting examples, but I think something at the top-level description would be a big help.
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.
Thanks for looking into it!
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: