ASCL Code Record
[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
- Used in:
- https://ui.adsabs.harvard.edu/abs/2016ApJ...832..202T
- Bibcode:
- 2016ascl.soft12018T
Preferred citation method:
Please see citation information here: https://github.com/ucl-exoplanets/pylightcurve#pylightcurve
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