All Tables

• Table 1: Observed and estimated parameters for HD 118203. (See text for references on the quoted values.)
• Table 2: ELODIE radial velocities of HD 118203. All data are relative to the solar system barycentre. Given uncertainties correspond to photon-noise errors.
• Table 3: ELODIE best Keplerian orbital solution obtained for HD 118203 as well as the inferred planetary parameters. For eccentric orbits T is defined as the time of the peri-astron passage.
• Table 4: Observed and estimated parameters for HD 149143. (See text for references on the quoted values.)
• Table 5: ELODIE radial velocities of HD 149143. All data are relative to the solar system barycentre.
• Table 6: ELODIE derived Keplerian orbital solution obtained for HD 149143 as well as the inferred planetary parameters. Both the quasi-circular and circular solutions are given because the derived eccentricity is only marginally significant. For the eccentric orbit T is defined as the time of the peri-astron passage whereas for the circular orbit T indicates the maximum of radial velocities.