Follow-up of CoRoT transiting exoplanets with HARPS and SOPHIE spectrographs

Details Follow-up of CoRoT transiting exoplanets with HARPS and SOPHIE spectrographs Follow-up of CoRoT transiting exoplanets with HARPS and SOPHIE spectrographs

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009sf2a.conf...21s&link_type=abstract

SF2A-2009: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, held 29 June - 4 July 2009 in

Astronomy and Astrophysics

Astrophysics

Scientific paper

The CoRoT space mission is detecting every semesters several tens of exoplanets transiting candidates. Among this candidates, there are several background eclipsing binairies. The radial velocity follow-up, performed with the high-resolution spectrographs HARPS (3.6m ESO) and SOPHIE (1.93m OHP), consists to measure the mass of companions and allows to characterize the nature of transiting object. For the faintest target (14

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