Corner plot showing the posterior distributions of the main internal structure parameters of HD 6860 b. The titles of each column correspond to the median and 1σ, which are also shown with dashed lines. This displays the results of the MCMC analysis, and the corrected RV time-series is presented. This analysis involves fitting a model that consists of an offset, an RV jitter, the semi-amplitude (K_b), the orbital period (P_b), the orbital eccentricity (e_b), the periastron angle (ω_b), the mean anomaly (MA_b), the slope (RV lin.tr), the mean longitude λ_b, the minimum mass (m sin i), and the semimajor axis (a_b).