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.
Laws
- linear
- quadratic
- square-root
- logarithmic
- nonlinear
Bands
- B
- C
- H
- I
- J
- K
- Kp
- T
- R
- S1
- S2
- S3
- S4
- U
- V
- b
- g*
- i*
- r*
- u
- u*
- v
- y
- z*