NASA-Planetary-Science / sbpy

A Python package for small bodies research
https://sbpy.org/
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Improve HG, HG12, etc. documentation #386

Open mkelley opened 10 months ago

mkelley commented 10 months ago

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:

import numpy as np
import matplotlib.pyplot as plt
from astropy.time import Time
import astropy.units as u
from astropy.visualization import time_support
from sbpy.photometry import HG1G2
from sbpy.data import Ephem

time_support()  # allow plotting Time objects with matplotlib

epochs={
    "start": Time("2022-09-26 23:14"),
    "stop": Time("2023-03-01"),
    "step": 1 * u.day,
}
eph = Ephem.from_horizons("didymos", epochs=epochs, location="500")
m_HG1G2 = HG1G2(H=18.11, G1=0.84, G2=0.05)

m = m_HG1G2(eph["phase"]) + 5 * np.log10(eph["rh"] / u.au * eph["delta"] / u.au)

plt.clf()
ax = plt.gca()
plt.plot(eph["date"], m)
ax.invert_yaxis()
mkelley commented 10 months ago

Thanks to @talister for the initial feedback. No good deed goes unpunished, so may ask you to review the updates 😸

mkelley commented 10 months ago

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.

jianyangli commented 10 months ago

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.

mkelley commented 10 months ago

Thanks for looking into it!