Notes: Model selection based on Bayesian evidence of the analysis of CCF FWHM and TM RV measurements. Same as in Table 3 but for normal priors around the candidate periods N0.3 for $\mathcal{N}$(P_orb, σ_P) with P_orb the orbital period and σ_P = 0.3 d. npe and npc indicate n Keplerian and circular orbits, and npe0 indicates a Keplerian with narrow prior on eccentricity e with $\sqrt{e}\cos (\omega )$ and $\sqrt{e}\sin (\omega )$ $\mathcal{N}$(0, 0.05). We highlight in bold fonts the reference activity-only model in this dataset, as in Table 3.