pith. sign in

arxiv: astro-ph/0506569 · v2 · submitted 2005-06-24 · 🌌 astro-ph

The Transit Light Curve Project. IV. Five Transits of the Exoplanet OGLE-TR-10b

Matthew J. Holman , Joshua N. Winn , Cesar I. Fuentes , Joel D. Hartman , K.Z. Stanek , Guillermo Torres , Dimitar D. Sasselov , B. Scott Gaudi
show 2 more authors
R. Lynne Jones Wesley Fraser
This is my paper
classification 🌌 astro-ph
keywords photometryradiusexoplanetfivelightogle-tr-10bplanetarytransit
0
0 comments X
read the original abstract

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 R_P = 1.06 +/- 0.08 R_Jup and the stellar radius to be R_S = 1.10 +/- 0.07 R_sun. 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.