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Limb darkening parameters from Claret+2011 and Claret 2017

Uses a Monte Carlo interpolation routine to propagate uncertaintes in stellar parameters to uncertainties in limb darkening parameters, e.g. for informative priors in Bayesian transit analysis.

Supports the following limb darkening laws and photometric bands:


  • linear
  • quadratic
  • square-root
  • logarithmic
  • nonlinear


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