Table A.2
Cluster parameters.
| Cluster | N |  (µas) |
 (mas/yr) |
µδ (mas/yr) | RV (km/s) | E(B − V) | NPCA | θ | ac (º) | alim | ∈ × 100 | N RRL |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| NGC 5139 | 69415 | 190 ± 9 | −3.245 ± 0.620 | −6.787 ± 0.590 | 234.5 ± 0.9 | 0 12 | 147516 | 164±1 | 0 326 | 0 693 | 6.4 ± 0.2 | 190 |
| NGC 104 | 53656 | 226 ± 10 | 5.272 ± 0.531 | −2.547 ± 0.562 | −16.8 ± 0.4 | 0 04 | 102838 | 47 ± 2 | 0 325 | 0 684 | 5.9 ± 0.4 | 2 |
| NGC 6752 | 20431 | 254 ± 10 | −3.161 ± 0.458 | −4.042 ± 0.462 | −26.7 ± 1.0 | 0 04 | 38979 | 156±12 | 0 209 | 0 440 | 2.3 ± 0.6 | 0 |
| … | … | … | … | … | … | … | … | … | … | … | … | … |
Notes. The complete version of this table is available at the CDS. Cluster name, number of cluster members used for the determination of the astrometric parameters, proper motion in right ascension and declination together with the error on the mean, radial velocity and error on the median. The main source of color excess measurements is the Harris (2010) catalog, for FSR 1758 we used the value provided by Romero-Colmenares et al. (2021). Number of cluster members used for the determination of ac, alim (see Sect. 3.2), position angle and number of RRLs in each cluster.
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