Transiting exoplanets characterization with the SOPHIE spectrograph at OHP

Details Transiting exoplanets characterization with the SOPHIE spectrograph at OHP Transiting exoplanets characterization with the SOPHIE spectrograph at OHP

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..777h&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.777

Physics

Scientific paper

The SOPHIE environmentally-stabilized echelle spectrograph at Haute-Provence Observatory is widely used for the radial velocity follow-up of photometric surveys for transiting planets detections, including ground- and space-based projects (SuperWASP, HAT, CoRoT, Kepler...). Such spectroscopic observations are mandatory to establish the planetary nature of transiting candidates and to characterize the detected planetary systems. Ground-based spectrographs as SOPHIE will be an essential part for the detection, characterization, and study of planets detected by the future surveys as PLATO and TESS.

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