Final RV model for Gl 382. The top panel shows the raw RV data with offsets removed, plotted for the SPIRou, HARPS, and CARMENES instruments (RMS = 5.79 m.s⁻¹). The second row illustrates the correction for stellar activity using GPs, with individual GP contributions shown for each grouped instrument. The bottom panel presents the residuals after removing all modeled signals (RMS = 1.90 m.s⁻¹). The rightmost column contains log BF periodograms highlighting significant periods in the RV data, the significance level of 5 is indicated by the horizontal red dashed line.