2006A&A...446..717D

We report the discovery of a new planet candidate orbiting the subgiant star HD118203 with a period of P=6.1335days. The best Keplerian solution yields an eccentricity e=0.31 and a minimum mass m₂sini=2.1M_Jup for the planet. This star has been observed with the ELODIE fiber-fed spectrograph as one of the targets in our planet-search programme biased toward high-metallicity stars, on-going since March 2004 at the Haute-Provence Observatory. An analysis of the spectroscopic line profiles using line bisectors revealed no correlation between the radial velocities and the line-bisector orientations, indicating that the periodic radial-velocity signal is best explained by the presence of a planet-mass companion. A linear trend is observed in the residuals around the orbital solution that could be explained by the presence of a second companion in a longer-period orbit. We also present here our orbital solution for another slightly evolved star in our metal-rich sample, HD149143, recently proposed to host a 4-d period Hot Jupiter by the N2K consortium. Our solution yields a period P=4.09days, a marginally significant eccentricity e=0.08 and a planetary minimum mass of 1.36M_Jup. We checked that the shape of the spectral lines does not vary for this star as well.