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Home Page: https://spotter.readthedocs.io
License: MIT License
Approximate forward models of fluxes and spectra time-series of non-uniform stars
Home Page: https://spotter.readthedocs.io
License: MIT License
With that we could add Gaussian spots, or load a starry map for tests
Should the covering fraction of the chord be computed relative to the sphere or the visible disk?
Add a function to calculate theta and phi for a uniform distribution of spots
Add methods to compute covering fractions, in and out of transit
Add facula to stellar maps. This requires to store two maps in Star
, for spots and faculae, as well as computing their respecting limb-variations.
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