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Table 1

Basic parameters of the investigated objects.

Cluster name Alternative names N [Fe/H]a log(Age[yr])b Turn-off mass M Rmean kpc |zmax| kpc
Alessi 1 Casado-Alessi 1 4 −0.01 ± 0.01 9.16 1.62 8.13 0.24
Basel 11b FSR 887 3 0.04 ± 0.03 8.36 3.20 9.02 0.07
COIN-Gaia 30 1 −0.04 8.41 3.08 8.84 0.18
Collinder 350 2 −0.04 ± 0.12 8.77 2.23 7.71 0.19
Collinder 463 2 −0.06 ± 0.02 8.06 4.26 9.00 0.18
Gulliver 51 1 −0.17 8.56 2.64 9.25 0.14
IC4756 Collinder 386, Melotte 210 12 0.00 ± 0.04 9.11 1.70 7.25 0.08
NGC 2437 M46, Melotte 75 6 −0.02 ± 0.08 8.48 2.89 8.69 0.30
NGC2509 Melotte 81, Collinder 171 3 0.21 ± 0.01 9.18 1.60 8.68 0.30
NGC 2548 M 48, Melotte 85 3 0.05 ± 0.06 8.59 2.64 9.04 0.28
NGC 2632 M44, Praesepe, Melotte 88 4 0.14 ± 0.04 8.83 2.18 7.90 0.13
NGC 2682 M67 4 0.04 ± 0.03 9.63 1.17 8.39 0.60
NGC6800 1 0.11 8.61 2.64 7.43 0.10
NGC 6991 5 0.04 ± 0.06 9.19 1.60 8.05 0.15
NGC7086 Collinder 437 2 −0.08 ± 0.03 8.29 3.44 8.09 0.11
NGC 7209 Melotte238, Collinder 444 2 −0.03 ± 0.07 8.63 2.53 7.90 0.15
NGC 752 Melotte 12 3 0.08 ± 0.02 9.07 1.76 8.01 0.23
Ruprecht 171 7 −0.07 ± 0.06 9.44 1.29 8.24 0.65
Stock 2 8 −0.02 ± 0.06 8.60 2.60 8.09 0.10
Tombaugh 5 3 0.02 ± 0.07 8.27 3.55 9.04 0.18
UBC3 Alessi 161 1 0.00 8.10 4.15 6.94 0.19
UBC60 COIN-Gaia 11 2 0.18 ± 0.05 8.90 2.04 8.27 0.08
UBC 131 Alessi 116, UPK 84 3 0.05 ± 0.03 9.00 1.85 8.48 0.22
UBC 141 1 −0.02 9.32 1.45 7.62 0.27
UBC 169 2 0.06 ± 0.03 8.47 2.96 8.37 0.21
UBC 194 1 0.06 8.36 3.26 8.57 0.24
UBC 577 Alessi 191 3 −0.05 ± 0.02 9.44 1.30 7.79 0.32
UPK219 1 0.07 8.17 3.88 9.15 0.08
Theia 1214_1c 1 0.14 8.69 d 2.78 d 7.95 0.23
Theia 1214_3c 1 –0.25 9.83 d 1.08 d 9.31 0.62

Notes. (a)The mean [Fe/H] of individual measured values for stars of each cluster in Dal Ponte et al. (2025). (b)Ages are taken from Cantat-Gaudin et al. (2020). (c)This association is inferred to be a part of NGC 752, as a tidal tail (Dal Ponte et al. 2025), but we treat it as a separate entity in this study. (d)For the Theia 1214 stars, the age and mass were derived in this study.

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