Transit comparison between Visit 1 (blue) and Visit 2 (red). ESPRESSO exposures are indicated by the colored symbols. Vertical dashed lines indicate transit contacts. Top panel: best-fit model light curves to the EulerCam photometry obtained simultaneously with the ESPRESSO transits, used to scale disk-integrated CCFs to their correct relative flux level. Bottom panel: RV centroids of the disk-integrated CCFs, computed from spectra Doppler-corrected for the stellar Keplerian motion and linear drifts with phase. The spot occultation visible in Visit 2 photometry, occurring within the red-shaded window, induces a clear deviation to the nominal RM anomaly in RV, which has also been found in Cristo et al. (2024).