Phase-folded RV evolution of TOI-1710 determined from the SOPHIE (in blue) and the HARPS-N (in orange) observations. Top panel: RV variation relative to a fitted instrumental offset (see text for details). The solid line and its light blue overlay correspond to the orbital solution presented in this study (Sect. 4.1) with its relative lσ uncertainty, respectively, and used to compute the residuals in the bottom panel.