Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius
A. Leger, D. Rouan, J. Schneider, P. Barge, M. Fridlund, B. Samuel, M., Ollivier, E. Guenther, M. Deleuil, H.J. Deeg, M. Auvergne, R. Alonso, S., Aigrain, A. Alapini, J.M. Almenara, A. Baglin, M. Barbieri, H. Bruntt, P., Borde, F. Bouchy, J. Cabrera, C. Catala, L. Carone

TL;DR
This paper reports the discovery of CoRoT-7b, the first Super-Earth with a measured radius, identified through transit observations and supported by extensive ground-based follow-up to confirm its planetary nature.
Contribution
It presents the first measurement of a Super-Earth's radius using transit data combined with ground-based observations, confirming its planetary status.
Findings
CoRoT-7b has a radius of approximately 1.68 Earth radii.
The orbital period of CoRoT-7b is about 0.8536 days.
Radial velocity data suggest an upper mass limit of 21 Earth masses.
Abstract
We report the discovery of very shallow (DF/F = 3.4 10-4), periodic dips in the light curve of an active V = 11.7 G9V star observed by the CoRoT satellite, which we interpret as due to the presence of a transiting companion. We describe the 3-colour CoRoT data and complementary ground-based observations that support the planetary nature of the companion. Methods. We use CoRoT color information, good angular resolution ground-based photometric observations in- and out- of transit, adaptive optics imaging, near-infrared spectroscopy and preliminary results from Radial Velocity measurements, to test the diluted eclipsing binary scenarios. The parameters of the host star are derived from optical spectra, which were then combined with the CoRoT light curve to derive parameters of the companion. We examine carefully all conceivable cases of false positives, and all tests performed support the…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
