Fig. 1.
Venn diagram of the 102 cluster members observed by Kepler/K2. The numbers indicate the quantity of stars in each corresponding subset. Stars included from the individual studies are: all those listed by Gaia Collaboration (2018a, GC18), those labeled P or Y by Curtis et al. (2013, Cu13), and those listed in Cantat-Gaudin et al. (2018, CG18) or Olivares et al. (2019, Ol19) with membership probability greater than 0.5.
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