Median kinematic ages (τ_kin) versus their median isochronal ages (τ_iso) for clusters NGC 2264 N (red), NGC 2264 S (green), and Coll 95 (orange). The plot is divided into nine panels, with the three subgroups as rows: all YSOs (top panel), YSOs moving away from the cluster center (middle panel), and YSOs with closest approach distances within r₅₀ and current distances outside of r₅₀ (lower panel). Columns denote the different isochrone models used, with Baraffe (left), PARSEC (middle), and SPOTS (right). The plot denotes photometric color used (BP-RP or G-RP) using symbols (BP-RP marked by a plus, G-RP marked by an X.) The error bars on each value are the 16th and 84th percentiles of the distribution of either kinematic or isochronal ages.