Top : radial velocities along with the median model (black line) for TOI-375. Our model is composed of three different Keplerian components. Bottom : Keplerian components of the full model presented in the top panel. The 9.4-day variation is from TOI-375 b, the transiting exoplanet detected by TESS. The two additional 118.7 and 289.9-day signals observed in our radial-velocities have been identified as likely candidate exoplanets (c and d) given no obvious stellar activity origin.