Posterior distributions of the semi-amplitude K_b (top panel), orbital period P_b (middle panel), and eccentricity e_b (bottom panel) of the candidate planet Gl514 b derived from a GP QPC analysis of the HARPSterra+CARMENES VIS RVs after removing an increasing number of CARMENES measurements, beginning from the last epoch. Vertical lines indicate the 16th, 84th (dashed), and 50th (solid) percentiles for the whole HARPS_TERRA+CARMENES dataset. Here, ∆ ln Z denotes the Bayesian evidence difference between a model with and without a Keplerian included.