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[ascl:1612.018] pylightcurve: Exoplanet lightcurve model

pylightcurve is a model for light-curves of transiting planets. It uses the four coefficients law for the stellar limb darkening and returns the relative flux, F(t), as a function of the limb darkening coefficients, an, the Rp/R* ratio and all the orbital parameters based on the nonlinear limb darkening model (Claret 2000).

Code site:
https://github.com/ucl-exoplanets/pylightcurve
Appears in:
http://adsabs.harvard.edu/abs/2016ApJ...832..202T
Bibcode:
2016ascl.soft12018T

ascl:1612.018
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