Parameters of the fits to the RV time series of GJ 508.2 as a function of the orbital period. The differential ln ℒ of the fit with respect to the maximum value, the fitted RV semi-amplitude and eccentricity, and the corresponding planet minimum mass are shown from top to bottom. Dahsed blue and solid black lines correspond, respectively, to fits considering only RVs from CARMENES VIS, and considering both VIS and NIR RVs simultaneously. The dot-dashed blue line in the top panel indicates the threshold corresponding to Δ ln ℒ=5, and the vertical dotted lines, the corresponding orbital period.