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Table B.2

Potential members of NGC 1904 (extract).

Gaia ID RA Dec µα µδ GBP−GRP G vrad σmeasv$\sigma _{{\rm{meas}}}^v$ [Fe/H] σmeas[Fe/H]$\sigma _{{\rm{meas}}}^{[Fe/H]}$ P
(Gaia DR3) (ICRS) (ICRS) (mas/ yr) (mas/ yr) (mag) (mag) (km/s) (km/s)
2957895907481574400 81.104 −24.870 2.445 −1.127 0.711 19.544 205.160 6.007 −2.508 0.535 0.775
2957939651729098752 81.030 −24.566 2.574 −1.574 1.227 14.504 207.580 0.664 −1.370 0.012 0.989
2957989400330136832 80.963 −24.418 2.341 −1.597 0.774 18.982 209.795 2.962 −1.738 0.176 0.980
2958540702332043264 81.865 −23.248 2.365 −1.455 0.865 18.851 207.331 5.594 −1.696 0.465 0.921
2958601935683680000 80.723 −23.726 2.457 −1.549 0.851 18.704 207.234 3.453 −1.607 0.182 0.987
2957934738286530688 81.031 −24.633 2.441 −1.637 0.943 17.690 205.437 1.150 −1.520 0.063 0.995
2957939686088825472 81.039 −24.558 2.508 −1.536 1.542 13.022 210.836 0.661 −1.106 0.007 0.875
2957944943128920064 81.233 −24.463 2.768 −1.600 0.626 19.410 206.844 6.250 −2.362 0.268 0.894
2957989469049599616 80.928 −24.437 2.338 −1.653 0.623 19.785 219.664 16.169 −2.329 0.397 0.836
2957989679507575936 80.944 −24.399 2.529 −1.639 1.044 16.192 204.357 0.702 −1.559 0.024 0.997

Notes. The full list is available at the CDS. The columns from left to right correspond to the following: the Gaia DR3 ID, current positions on the sky, proper motions, colours, magnitudes, line-of-sight velocities, error on the velocities, S5 metallicity, error on the metallicity, and the membership probability of each star to belong the cluster.

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