Image Details
Caption: Figure 5.
[Fe/H] and [M/H] measurements for the candidate members of CUMA collected from the APOGEE DR17, GALAH DR3, RAVE DR6, and LAMOST DR7 catalogs. In the left panel we show the metallicity as a function of the probability of belonging to the CUMA group, and in the right panel is the distribution of values. We included the value of [Fe/H] for COCONUTS-2 A and [M/H] for COCONUTS-2 b as five-point stars in the left panel and as horizontal lines in the right panel. The dotted horizontal lines show the uncertainty in these two values. We also included in a black horizontal line, the value of [Fe/H] for the UMA cluster (A. M. Boesgaard et al. 1988).
© 2026. The Author(s). Published by the American Astronomical Society.