Table 2
List of the 510 stars that were selected from GES iDR4 as probable members and analyzed in this paper.
| CNAME | Cluster | T eff | δ T eff | log g | δlog g | [Fe/H] | δ[Fe/H] | log ϵAl | δlog ϵAl | log ϵMg | δlog ϵMg |
| (K) | (K) | (dex) | (dex) | (dex) | (dex) | (dex) | (dex) | (dex) | (dex) | ||
|
|
|||||||||||
| 12593863-7051321 | NGC 4833 | 4673 | 124 | 1.308 | 0.246 | –1.844 | 0.103 | 5.61 | 0.07 | 5.94 | 0.13 |
| 13000316-7053486 | NGC 4833 | 4675 | 132 | 1.207 | 0.239 | –1.920 | 0.106 | 5.60 | 0.07 | 5.59 | 0.13 |
| 12585746-7053278 | NGC 4833 | 4678 | 127 | 1.316 | 0.261 | –2.024 | 0.119 | 5.29 | 0.07 | 5.73 | 0.14 |
| 12592040-7051156 | NGC 4833 | 4623 | 123 | 1.130 | 0.252 | –1.922 | 0.101 | 5.55 | 0.07 | 5.50 | 0.13 |
| 12593089-7050304 | NGC 4833 | 4613 | 123 | 1.112 | 0.254 | –1.920 | 0.108 | 5.55 | 0.07 | 5.66 | 0.14 |
| 12594306-7053528 | NGC 4833 | 4635 | 117 | 1.070 | 0.235 | –1.890 | 0.111 | 5.61 | 0.07 | 5.69 | 0.13 |
Notes. The table is available in its entirety at the CDS, here we show a portion to illustrate its contents. The reported errors are the result of the complex GES homogenization procedure and thus include random and systematic error sources.
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