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Fig. 8

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UVW velocity diagram for TOI-1801 (gold star) and LP 375-24 (orange star). The members of the Castor moving group (200–400 Myr), the Hyades supercluster (Hs; 600–800 Myr), the IC 2391 supercluster (35–55 Myr), the Local Association (LA; 10–300 Myr), and the Ursa Major group (UMa; ~400 Myr) from Montes et al. (2001) are included. The ellipses represent the 3σ values of UVW for each young moving group. The inset in the upper left panel shows a zoom-in on the region with the stars. The locations of both stars agree with that of members of the Hyades supercluster.

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