This article has 2 errata:
[https://doi.org/10.1051/0004-6361/202039217]
[https://doi.org/10.1051/0004-6361/201832698e]
Table D.3
Example of part of a list of possible cluster members.
| source_id | RA | Dec | G (phot_g_mean_mag) |
|---|---|---|---|
| 4689633627542489728 | 6.77396 | –71.99619 | 19.378 |
| 4689634074221208320 | 6.48790 | –72.01599 | 17.090 |
| 4689638128697225216 | 5.61038 | –72.13231 | 19.695 |
| 4689637514491268480 | 5.75409 | –72.11833 | 17.506 |
Notes. Here we list the first four entries of the compilation of members of the globular cluster NGC 104. The full table for this cluster is available at the CDS, along with separate tables for each of the rest of the globular clusters in our sample, each of the 9 dSph, the Bootes I UFD, and the LMC and SMC. The stars in these lists were selected and used to determine the astrometric parameters of the corresponding objects following either the procedures described inSect. 2.1 (for the clusters and dwarfs) or in Sect. 2.2 (for the LMC and SMC).
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