Similar to Fig. A.1, but for the 84 joint HARPS+CARMENES RVs obtained during the time interval in which the two spectrograph WFs overlap (February–June 2017). The HARPS and CARMENES RVs are plotted as blue and red markers, respectively. The phase-folded RVs depicting planetary signals are binned for clarity. The rms of the residual time-series assuming a one- and two-planet model are 4.26 and 3.62 m s⁻¹, respectively.MAP RV models. GLSP periodicities.