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We report on the results from the radial-velocity follow-up program performedto establish the planetary nature and to characterize the transiting candidatesdiscovered by the space mission CoRoT. We use the SOPHIE at OHP, HARPS at ESOand the HIRES at Keck spectrographs to collect spectra and high- precisionradial velocity (RV) measurements for several dozens dif- ferent candidatesfrom CoRoT. We have measured the Rossiter- McLaughlin effect of severalconfirmed planets, especially CoRoT- 1b which revealed that it is anotherhighly inclined system. Such high-precision RV data are necessary for thediscovery of new tran- siting planets. Furthermore, several low mass planetcandidates have emerged from our Keck and HARPS data.

Radial velocity follow-up of CoRoT transiting exoplanets