Table C.3
Membership analysis and candidate selections (see the exemplified Table C.8 for cluster NGC 2516).
| Column name | Description |
|---|---|
| CNAME | GES object name from coordinates |
| RV_mem | Membership: RV |
| PM_mem | Membership: Proper motions |
| Parallax_mem | Membership: Parallax |
| CMD_mem | Membership: CMD |
| logg_mem | Membership: logg (intermediate-age and old clusters) |
| gamma_mem | Membership: γ index (young clusters) |
| Met_mem | Membership: [Fe/H] metallicity |
| Li_mem | Membership: EW(Li) |
| Cantat_Gaudin_2018 | Members from Cantat-Gaudin et al. (2018) (a) |
| Randich_2018 | Members from Randich et al. (2018) (a) |
| Jackson_2021_MEM3D | Members from Jackson et al. (2022) (a), (b) |
| Jackson_2021_MEMQG | Members from Jackson et al. (2022)(a), (c) |
| Final | Final candidate members (d) |
| Particular_cases | Final column listing particular cases (e) |
Notes. (a)Additional columns, whenever possible, listing candidates according to relevant Gaia studies from the literature. (b)Jackson et al. (2022) – MEM3D refers to the membership using the full data set. (c)Jackson et al. (2022) – MEMQC refers to the probability computed using data set filtered to remove targets with suspect Gaia data. (d) ‘Y’=members; ‘n’=Non-members. (e)Particular cases include the Li-rich giant outliers (listed as ‘Li-rich G’), strong accretors (‘Strong accretor’), and the SB1 and SB2 binary stars (‘SB1’ and ‘SB2’) listed by GES iDR6 and Merle et al. (2017, 2020).
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