HARPS radial velocity search for planets in the Scorpius-Centaurus association - A combination with the HARPS and SOPHIE young nearby stars (YNS) surveys

Open Access

Fig. C.6

Posterior distributions of the MCMC fit performed on the HD 108904 RV and HD 108904 B relative astrometry simultaneously. From top to bottom: RV offset to take into account that the RVs are relative to a reference (V₀), RV jitter amplitude (jitter), semimajor axis (sma_b), eccentricity (ecc_b) argument of periastron (parg_b), period (per_b), mass (m_b), inclination (I_b) and longitude of the ascending node (O_b) of HD 108904 B.

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