Generalized Lomb–Scargle periodograms of HD 102365 RVs. The orange curve corresponds to CCF-derived RVs, the blue curve shows RVs obtained with TILARA using down-weighting, and the red curve shows RVs obtained with TILARA using sigma-clipping. Horizontal dashed lines indicate the 1% FAP for each dataset (overlapping for the three methods). The vertical dashed line and shaded region mark the expected orbital period of HD 102365 b (122.1 ± 0.3 days). No significant peak is observed at the planet’s period in either dataset.