Table 6.
Example of candidate members observed and available in a few clusters.
| Cluster | N GES | N GES | N C-T | N C-T | N C-T | Members | GES/C-T | GES/C-T |
|---|---|---|---|---|---|---|---|---|
| observed | G ≤ 18 | d ≤ 12.5′ | prob ≥ 0.7 | prob ≥ 0.9 | J+2021 | prob ≥ 0.7 | prob ≥ 0.9 | |
| NGC 6709 | 730 | 664 | 223 | 158 | 76 | 125 | 0.79 | 1.64 |
| NGC 6705 | 1066 | 1012 | 2439 | 883 | 245 | 526 | 0.60 | 2.15 |
| NGC 6802 | 197 | 183 | 753 | 270 | 100 | 55 | 0.20 | 0.55 |
| NGC 2355 | 208 | 190 | 314 | 222 | 88 | 139 | 0.63 | 1.58 |
| NGC 2158 | 616 | 490 | 1633 | 1186 | 647 | 346 | 0.29 | 0.53 |
| NGC 2420 | 562 | 509 | 513 | 331 | 121 | 384 | 1.16 | 3.17 |
| NGC 2243 | 710 | 521 | 531 | 479 | 327 | 538 | 1.12 | 1.65 |
| Berkeley 39 | 899 | 675 | 562 | 508 | 382 | 507 | 1.00 | 1.33 |
| Berkeley 36 | 739 | 356 | 374 | 112 | 51 | 212 | 1.89 | 4.16 |
Notes. N GES is the number of stars in Gaia-ESO final data release; C-T stands for Cantat-Gaudin et al. (2018), Cantat-Gaudin & Anders (2020); J+21 stands for Jackson et al. (2021), their Tables 4, 5; the last two columns give the fractions of stars assumed as member by J+21 and C-T (for the latter, membership probability larger than 0.7 and 0.9 were selected.
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