TODO.txt

- Interpolate my own rotation curves from photometric distributions?
    - Compare the above for Newtonian, Relativistic, MONDian, and MOUNDian dynamics
    - Compare best-fit DM halos?
- All photometric and velocity curve data is calculated with stellar mass-to-light ratios \Upsilon_{star} = 1 M_sol/L_sol
    - Is this a good assumption? Does other data support this, or would there be a better way to approximate mass distributions?
    - Add a way to vary this as a hyperparameter
        - Further allow variation over bulge/disk ratios individually?
            - This would only make sense if we have some reason to believe that average stellar mass is radially dependant (and this doesn't come from photometric data somehow), and therefore mass-to-luminosity ratios would be different in the disk vs bulge (or even to a higher degree of granularity)
- Individual to galaxy parameters?
    - gas fraction? -> for irregulars especially
    - Gas distribution within galaxies is non-trivial and requires outside data models.
    - stellar mass-to-light ratios (for bulge and disk)?