Phase-folded RV curves recovered for the injected synthetic planets with a period of 100.00 days and eccentricity e = 0.00, after applying the down-weighting method. The left panel shows the recovered RV curve for the injected signal with K = 10.00 m s⁻¹, and the right panel the one for K = 2.00 m s⁻¹. In both cases, the solid line represents the best-fit Keplerian model obtained with KIMA, successfully retrieving the injected signal using the RVs derived with TILARA.