Fig. 6
ELODIE (red) and SOPHIE (blue) RV and residuals from the best-fit Keplerian model for HD 222155 as a function of barycentric Julian date. The best-fit Keplerian model is represented by the black curve with a reduced χ2 equal to 2.2. The planet has a period of 10.9 yr in a non-significant eccentric orbit (
), and a minimum mass of 1.90 MJup.
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