Open Access

Table F.1

Example of a list of observed stars in clusters Melotte 22, Melotte 25, and NGC 2632. Last column gives remarks on stars that were observed and analysed in DR4, but rejected for the analysis regarding the origin of the trends. Full table is available online.

sobject_id Gaia DR3 source_id Cluster C-G H&R MG BP-RP RUWE Teff log g S/NCCD3 χ2 [Fe/H] Rejected
150109001001324 66733552578791296 Melotte 22 6.794 1.393 3.34 4602.5 4.41 86.7 0.89 -0.15 3
150109001001329 65224442806459008 Melotte 22 7.943 1.811 1.03 3939.7 4.53 46.0 0.88 -0.66
160106001601238 65292234570088064 Melotte 22 2.654 0.383 0.96 7511.0 4.18 349.3 1.8 -0.53
150109001001004 66500013736315264 Melotte 22 9.206 2.443 1.51 4290.7 4.84 7.0 1.01 0.52 3,5
160106001601346 66729880383767168 Melotte 22 1.124 0.101 1.14 8000.0 3.89 489.8 1.71 -0.44 1
150109001001091 64856312568645248 Melotte 22 7.831 1.768 1.08 3604.3 4.37 29.6 0.86 -0.55
160106001601260 68310359628169088 Melotte 22 5.157 1.108 5.59 5006.3 4.32 96.5 0.94 -0.2 1,3
150109001001244 65248151025861120 Melotte 22 7.54 1.746 2.25 4006.6 4.34 50.1 1.03 -1.12 3
160106001601242 68296890611072384 Melotte 22 4.883 0.904 1.05 5690.2 4.34 122.5 0.81 -0.07
160108002001089 65787289680918528 Melotte 22 6.146 1.136 1.07 5079.3 4.62 71.3 0.85 -0.03

1: rejected for being a photometric binary.

2: rejected for being a spectroscopic binary.

3: rejected for RUWE > 1.4.

4: rejected for spectral fitting giving χ2 > 3.0.

5: rejected for large vr error.

6: rejected for low S/N.

7: rejected after visual inspection.

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