Journal
ASTROPHYSICAL JOURNAL
Volume 655, Issue 2, Pages 1103-1109Publisher
IOP PUBLISHING LTD
DOI: 10.1086/510342
Keywords
planetary systems stars : individual (OGLE-TR10) techniques : photometric
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We present I and B photometry of five distinct transits of the exoplanet OGLE-TR-10b. By modeling the light curves, we find the planetary radius to be RP (1:06 +/- 0:08) R-Jup and the stellar radius to be R-S 1:10 +/- 0:07 R (circle dot). The uncertainties are dominated by statistical errors in the photometry. Our estimate of the planetary radius is smaller than previous estimates that were based on lower precision photometry, and hence the planet is not as anomalously large as was previously thought. We provide updated determinations of all the system parameters, including the transit ephemerides.
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