This, combined with simultaneous wavelength phasecurves (Issue #6), can allow you to simultaneously find the albedo and temperature map of a planet when fitting the model to a real lightcurve (or multiple phasecurves e.g. TESS and Spitzer). The albedo map would affect the heat deposited in each region. It wouldn't be self-consistent (e.g. temperature wont affect albedo), just a fairly low order spherical harmonic map or something like that.
This, combined with simultaneous wavelength phasecurves (Issue #6), can allow you to simultaneously find the albedo and temperature map of a planet when fitting the model to a real lightcurve (or multiple phasecurves e.g. TESS and Spitzer). The albedo map would affect the heat deposited in each region. It wouldn't be self-consistent (e.g. temperature wont affect albedo), just a fairly low order spherical harmonic map or something like that.
Good for a v2 release