Linear and non-linear limb-darkening coefficients for the photometric bands R I J H K.

Details Linear and non-linear limb-darkening coefficients for the photometric bands R I J H K. Linear and non-linear limb-darkening coefficients for the photometric bands R I J H K.

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26as..114..247c&link_type=abstract

Astronomy and Astrophysics Supplement, v.114, p.247

Astronomy and Astrophysics

Astrophysics

161

Stellar Atmospheres, Limb-Darkening, Eclipsing Binaries, Infrared

Scientific paper

We have computed limb-darkening coefficients for five commonly used near infrared photometric bands, namely R, I, J, H, and K, using the stellar atmosphere models by Kurucz (1993). Since the behaviour of the specific intensities is very dependent on the range of effective temperatures considered, we have adopted three analytical approximations to the limb darkening: linear, quadratic and square root. The least-squares method has been adopted for the fit of the limb-darkening coefficients to the model atmospheres.

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