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Table B.1

Potential members of NGC 1261 (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)
4733677211487164160 47.885 −55.633 1.779 −1.770 0.987 18.795 67.906 5.324 −1.309 0.211 0.605
4733699790131324544 48.065 −55.287 1.419 −2.153 0.630 19.606 67.236 7.805 −1.480 0.380 0.825
4733781635030255232 48.139 −55.296 1.519 −1.886 0.964 18.977 76.810 2.578 −1.362 0.114 0.929
4733699893210538112 48.061 −55.261 1.690 −2.024 1.115 16.158 69.496 0.694 −1.088 0.021 0.971
4733781665091557760 48.149 −55.286 1.499 −1.817 0.999 17.861 74.026 1.240 −1.167 0.065 0.853
4733795585081224320 48.244 −55.189 1.476 −1.685 0.754 19.532 71.751 7.563 −1.751 0.250 0.640
4733711158908171392 48.726 −55.672 1.830 −2.243 0.812 18.816 70.250 3.164 −1.288 0.182 0.913
4733782283566915584 48.269 −55.226 1.622 −1.974 0.615 19.625 76.777 6.650 −1.466 0.246 0.857
4726956244798037120 44.930 −58.684 2.269 −2.879 0.672 18.926 35.518 3.020 −1.052 0.179 0.955
4733700335591309824 47.942 −55.289 1.675 −2.272 0.878 18.602 69.332 1.498 −1.335 0.079 0.966

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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