Top panel: UV W velocities of TOI-1201 (red dot) and PM J02489–1432E (blue dot) compared against members of young moving groups from Montes et al. (2001), namely Castor (blue), the Hyades Supercluster (HS, orange), the IC 2391 Supercluster (green), the Local Association (LA, red), and Ursa Major (UMa, purple). The ellipses represent the 2σ value of the UV W for each group. The two targets agree with the Hyades Supercluster. Bottom panel: rotational period of TOI-1201 alongside members of the Pleiades (in red) and Praesepe (in green) open clusters from Curtis et al. (2019) and references therein.