A new non-linear limb-darkening law for LTE stellar atmosphere models III. Sloan filters: Calculations for -5.0 ≤ log [M/H] ≤ +1, 2000 K ≤ Teff ≤ 50 000 K at several surface gravities

Details A new non-linear limb-darkening law for LTE stellar atmosphere models III. Sloan filters: Calculations for -5.0 ≤ log [M/H] ≤ +1, 2000 K ≤ Teff ≤ 50 000 K at several surface gravities A new non-linear limb-darkening law for LTE stellar atmosphere models III. Sloan filters: Calculations for -5.0 ≤ log [M/H] ≤ +1, 2000 K ≤ Teff ≤ 50 000 K at several surface gravities

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...428.1001c&link_type=abstract

Astronomy and Astrophysics, v.428, p.1001-1005 (2004)

Astronomy and Astrophysics

Astrophysics

177

Stars: Atmospheres, Stars: Binaries: Eclipsing, Stars: Low Mass, Brown-Dwarfs, Stars: Planetary Systems

Scientific paper

Continuing our studies on stellar atmospheres (Claret \cite{Claret00}, \cite{Claret04}), we present in this paper the limb-darkening coefficients for the Sloan photometric system. The calculations cover a wide range of values of log g, Teff, metallicities and microturbulent velocities. The atmosphere models used are ATLAS and PHOENIX. In addition to the traditional applications of the limb-darkening coefficients, the present ones will be useful since the Sloan filters are now being used in the interpretation of light curves of extrasolar transiting planets, for example. The present calculations may also be useful, as a complement, for the Kepler mission, dedicated to the search for terrestrial planets.
Tables 2 to 11 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/428/1001 Additional data are available on CD ROMs.

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