Estimating limb-darkening parameters from stellar atmosphere models

[ericagol]

• [ ] Numerically compute transit light curves for a range of b & r from the complete spherical limb-darkening model.
• [ ] For each model atmosphere, fit the light curves with a series limb-darkening model (based on Y_{lm} expansion), and see what l is necessary to go to in order to fit the simulated light curves to a required (fractional) precision.
• [ ] Report these best-fit parameters as a function of wavelength and stellar parameters.