Table 1
Results of the membership analysis.
| Gaia DR3 source id | Cluster | Likelihood | Prior | Posterior | RVflag | SOS | Classifier | G23 | C17 | New | Final | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 4689637956899105792 | NGC 104 (47 Tuc) | 0.3405 | 1 | 0.3405 | False | True | True | True | True | False | True | |
| 6045834869114826496 | NGC 6144 | 1.0000 | 1 | 1.0000 | False | True | True | True | False | False | True | |
| 2342907756640334848 | NGC 288 | 0.9996 | 1 | 0.9996 | False | True | True | True | False | False | True | |
| 2342908787434423040 | NGC 288 | 0.9897 | 1 | 0.9897 | False | True | True | True | True | False | True | |
| … | … | … | … | … | … | … | … | … | … | … | … | … |
Notes. The complete version of this table is available at the CDS. RV flag is a Boolean column if True, it indicates that the SOS radial velocity was used to compute the likelihood. The columns SOS, classifier, G23, and C17 serve as boolean indicators, that specify if the source is included in the catalog at the top. The final column indicates the sources that are part of our final sample, as explained in Sect. 4.1.
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