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We report here the discovery of two planet candidates as a result of ourplanet-search programme biased in favour of high-metallicity stars, using theELODIE spectrograph at the Observatoire de Haute Provence. One of them has aminimum mass m_2\sin{i} = 2.5 M_Jup and is orbiting the metal-rich star HD43691with period P = 40 days and eccentricity e = 0.14. The other planet has aminimum mass m_2\sin{i} = 5.6 M_Jup and orbits the slightly metal-rich starHD132406 with period P = 974 days and eccentricity e = 0.34. Both stars werefollowed up with additional observations using the new SOPHIE spectrograph thatreplaces the ELODIE instrument, allowing an improved orbital solution for thesystems.

Elodie metallicity-biased search for transiting Hot Jupiters IV. Intermediate period planets orbiting the stars HD43691 and HD132406