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Power-2 limb-darkening coefficients for the uvby, UBVRIJHK, SDSS ugriz, Gaia, Kepler, and TESS photometric systems

Claret, A.; Southworth, John

Power-2 limb-darkening coefficients for the uvby, UBVRIJHK, SDSS ugriz, Gaia, Kepler, and TESS photometric systems Thumbnail


Authors

A. Claret



Abstract

Context. Limb darkening is an important stellar phenomenon and must be accounted for in the study of stellar spectra, eclipsing binaries, transiting planetary systems, and microlensing events. The power-2 limb-darkening law provides a good match to the specific intensities predicted by stellar atmosphere models: it is better than other two-parameter laws and is only surpassed by the four-parameter law.

Aims. Predictions of the limb-darkening coefficients for the power-2 law are not widely available. We therefore compute them, using stellar atmosphere models generated by the ATLAS (plane-parallel) code.

Methods. Limb-darkening coefficients were computed for the space missions Gaia, Kepler, and TESS as well as for the photometric systems uvby, UBVRIJHK, and SDSS ugriz. The calculations were performed by adopting the Levenberg–Marquardt least-squares minimisation method and were computed with a resolution of 100 equally spaced viewing angles. We used 9586 model atmospheres covering 19 metallicities, effective temperatures of 3500–50 000 K, log g values from 0.0 to 5.0, and microturbulent velocities of 0, 1, 2, 4, and 8 km s-1.

Results. We confirm the superiority of the power-2 law, in terms of the quality of the fits, over other two-parameter laws. This is particularly relevant for the quadratic law, which is widely used.

Conclusions. We recommend the use of the power-2 law in cases where a two-parameter law is needed.

Citation

Claret, A., & Southworth, J. (2022). Power-2 limb-darkening coefficients for the uvby, UBVRIJHK, SDSS ugriz, Gaia, Kepler, and TESS photometric systems. Astronomy & Astrophysics, 664, Article A128. https://doi.org/10.1051/0004-6361/202243827

Journal Article Type Article
Acceptance Date Jun 3, 2022
Online Publication Date Aug 18, 2022
Publication Date 2022-08
Journal Astronomy & Astrophysics
Print ISSN 0004-6361
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 664
Article Number A128
DOI https://doi.org/10.1051/0004-6361/202243827
Publisher URL https://www.aanda.org/articles/aa/abs/2022/08/aa43827-22/aa43827-22.html

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