Stellar Limb-Darkening Coefficients (Sing, 2010)

Physics

Scientific paper

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Models: Atmosphere, Binaries: Eclipsing, Planets

Scientific paper

These are calculations of limb-darkening coefficients used to describe the intensity profiles of stars for the CoRot and Kepler exoplanet missions.
The full version of the tables can be also be found at http://vega.lpl.arizona.edu/~singd/ which also includes an IDL program to read and interpolate the tables.
(2 data files).

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