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UBV(RI)C photometry of transiting planet hosting stars

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 13 Sep 2011Embargo end date: 01 Jan 2011 South Africa Publisher:Oxford University Press (OUP)Journal:Monthly Notices of the Royal Astronomical Society, volume 418, pages 1,039-1,042 (issn: 0035-8711,

Authors: Maxted, P.F.L.; Koen, Chris; Smalley, B.;

doi: 10.1111/j.1365-2966.2011.19554.x , 10.48550/arxiv.1108.0349

arXiv: http://arxiv.org/abs/1108.0349

handle: 10566/843

UBV(RI)C photometry of transiting planet hosting stars

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Abstract

We present new UBV(RI)_C photometry of 22 stars that host transiting planets, 19 of which were discovered by the WASP survey. We use these data together with 2MASS JHK_S photometry to estimate the effective temperature of these stars using the infrared flux method. We find that the effective temperature estimates for stars discovered by the WASP survey based on the analysis of spectra are reliable to better than their quoted uncertainties.

Accepted for publication in MNRAS. 4 pages, 1 figure

Country

South Africa

Related Organizations

Keele University
United Kingdom
University of the Western Cape
South Africa

Keywords

Earth and Planetary Astrophysics (astro-ph.EP), Planetary systems, Astrophysics - Solar and Stellar Astrophysics, Techniques: spectroscopic, FOS: Physical sciences, Techniques: photometric, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics - Earth and Planetary Astrophysics

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Photometry of transiting planet host stars
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