TESS Cycle 5 CPD. All the periods shown here have powers above the threshold for this cycle. P_rot measurements identified for removal due to source confusion either by GVC objects or by other cluster members are marked with orange crosses. A significant fraction of these P_rot are <0.5 days, faster than we would expect for stars earlier than mid-K at this age, for example (see D. J. Fritzewski et al. 2021a).