Gravity and limb-darkening coefficients for the<i>Kepler</i>, CoRoT,<i>Spitzer</i>,<i>uvby</i>,<i>UBVRIJHK</i>, and Sloan photometric systems
A. ClaretInstituto de Astrofísica de Andalucía, CSIC, Apartado 3004, 18080 Granada, SpainS. BloemenInstituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
2011en
ABI
Abstract
Aims. The complex physics of close binary stars is made even more challenging by the proximity effects that affect it. Understanding the influence of these proximity effects is one of the most important tasks in theoretical stellar astrophysics. It is crucial to know how the specific intensity is distributed over the stellar disk for a correct modelling of the light curves of eclipsing binaries and planetary transits. To provide theoretical input for light curve modelling codes, we present new calculations of gravity- and limb-darkening coefficients for a wide range of effective temperatures, gravities, metallicities, and microturbulent velocities.
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