Image Details
Caption: Figure 4.
[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. We included in a black horizontal line, the value of [Fe/H] for the UMA cluster (A. M. Boesgaard et al. 1988). We also included as a vertical line, the value of [Fe/H] for COCONUTS-2 A and [M/H] for COCONUTS-2 b (See Section 5.2). The dotted vertical lines show the uncertainty in these two values. These measurements agree with the distribution of the moving group within the uncertainty, supporting the membership of COCONUTS-2 to the group.
© 2026. The Author(s). Published by the American Astronomical Society.