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Table 1

Clusters used as template data set to select SFRs and other stellar clusters.

Literature name Flag Reference l (deg) b (deg) r50 (deg) d (pc) log t (yr) N
[LK2002] Cl10 1 Le Duigou & Knodlseder (2002) 79.867 −0.908 0.886 1557 167
65.78-2.61 2 Avedisova (2002) 66.153 −3.123 1.194 1324 134
Rosette 3 Zucker et al. (2020) 206.438 −1.903 2.025 1571 7.1 810
NGC 6530 4 Dias et al. (2002) 6.060 −1.287 1.020 1364 635
NGC 6531 5 Dias et al. (2002) 7.585 −0.338 1.634 1350 8.6 804
UBC386 6 Cantat-Gaudin & Anders (2020) 100.562 8.694 1.147 1280 6.8 193
Ass Cyg OB9 7 Sitnik (2003) 78.753 1.778 2.293 1339 8.1 616
Serpens South molecular cloud 8 Fernández-López et al. (2014) 29.364 2.870 0.976 920 123
CygOB7 CO Complex 9 Dutra & Bica (2002) 92.653 2.529 0.950 1123 46
BRC 27 10 Rebull et al. (2013) 224.621 −2.244 3.027 1233 6.9 1709
[DB2002b] G352.16+3.07 11 Otrupcek et al. (2000) −7.866 3.002 4.764 1169 7.0 2357
IC 1396 12 Zucker et al. (2020) 99.236 4.733 7.407 945 7.4 3140
[MML2017] 2399 13 Miville-Deschênes et al. (2017) 33.890 0.643 2.543 609 130
Chamaeleon II 14 Zucker et al. (2020) −56.363 −14.720 2.452 200 41
Cepheus 15 Zucker et al. (2020) 108.911 4.359 9.748 923 8.2 11445
NGC 7039 16 Cantat-Gaudin & Anders (2020) 88.350 −1.717 5.322 767 7.3 1048
[YDM97] CO 14 17 Yonekura et al. (1997) 104.508 13.950 3.039 350 124
Serpens 18 Zucker et al. (2020) 28.783 3.082 10.166 455 7.2 2388
IC 348 19 Cantat-Gaudin & Anders (2020) 160.790 −15.812 11.430 334 7.4 2661
Chamaeleon I 20 Zucker et al. (2020) −62.781 −15.444 3.099 192 156
Taurus 21 Zucker et al. (2020) 172.114 −15.302 4.551 131 112
Ophiuchus 22 Zucker et al. (2020) −8.024 18.781 12.655 144 2398
Corona Australis 23 Zucker et al. (2020) −0.132 −17.592 3.291 155 107
[DB2002b] G302.72+4.67 24 Dutra & Bica (2002) −57.143 4.739 5.854 112 235
Pozzo 1 25 Cantat-Gaudin & Anders (2020) 261.858 −8.321 13.343 398 8.3 6001
ASCC32 26 Cantat-Gaudin & Anders (2020) 237.327 −9.186 9.878 818 8.4 4416
LacOB1 27 Chen & Lee (2008) 96.762 −15.032 11.268 548 7.4 2367
RSG8 28 Cantat-Gaudin & Anders (2020) 109.331 −1.212 12.055 468 7.4 2900
NGC 2451B 29 Cantat-Gaudin & Anders (2020) 253.198 −7.499 9.513 401 7.6 2826
NGC 2232 30 Cantat-Gaudin & Anders (2020) 215.533 −7.983 13.427 372 7.2 1703
Sco OB2 UCL 31 de Zeeuw et al. (1999) −29.000 16.813 15.052 145 1189
IC 2602 32 Cantat-Gaudin & Anders (2020) −70.259 −5.011 6.825 151 7.6 315
NGC 2516 33 Cantat-Gaudin & Anders (2020) −86.236 −15.931 6.881 427 7.6 1156
Melotte 20 34 Cantat-Gaudin & Anders (2020) 147.504 −6.461 8.867 174 7.7 414
Melotte 22 35 Cantat-Gaudin & Anders (2020) 166.573 −23.406 5.882 137 7.9 296
NGC 2422 36 Cantat-Gaudin & Anders (2020) 230.995 3.061 6.238 500 8.0 347
Alessi 12 37 Cantat-Gaudin & Anders (2020) 67.678 −11.723 3.977 546 8.1 127
NGC 3532 38 Cantat-Gaudin & Anders (2020) −72.815 2.279 4.851 561 8.6 88
IC 6451 39 Cantat-Gaudin & Anders (2020) −19.939 −7.821 1.257 1068 9.2 86
NGC 6087 40 Cantat-Gaudin & Anders (2020) −32.077 −5.426 2.532 1007 8.0 77
Alessi 62 41 Cantat-Gaudin & Anders (2020) 53.676 8.773 3.561 622 8.4 87
UPK 33 42 Cantat-Gaudin & Anders (2020) 27.965 0.108 3.931 518 8.4 111
NGC 1647 43 Cantat-Gaudin & Anders (2020) 180.355 −16.861 2.141 606 8.6 272
NGC 6124 44 Cantat-Gaudin & Anders (2020) −19.205 6.078 5.404 648 8.3 1102
NGC 6494 45 Cantat-Gaudin & Anders (2020) 9.714 2.980 5.537 755 8.6 680
IC 4725 46 Cantat-Gaudin & Anders (2020) 14.022 −4.595 4.807 669 8.1 788
Alessi 44 47 Cantat-Gaudin & Anders (2020) 37.075 −11.510 7.285 587 8.2 637
Stock2 48 Cantat-Gaudin & Anders (2020) 133.371 −1.160 8.292 384 8.6 727
NGC 2168 49 Cantat-Gaudin & Anders (2020) 186.647 2.327 2.616 928 8.2 118
DSHJ2320.1+5821A 50 Kronberger et al. (2006) 111.248 −2.785 2.394 1131 243
UPK 143 51 Cantat-Gaudin & Anders (2020) 91.810 0.514 1.752 934 8.4 262
Collinder421 52 Cantat-Gaudin & Anders (2020) 79.429 2.527 1.061 1265 8.4 154

Notes. Flag is the value assigned to each cluster to characterise a given observed CAMD shape. r50 is the radius in which half of the identified members are concentrated, d is the distance obtained by inverting the median value of the member parallaxes and N is the number of members. Flag = [1, 28] are assigned to clusters with ages t ≲ 10 Myr, Flag = [29, 36] are assigned to clusters with ages 10 ≲ t/ Myr ≲ 100, Flag = [37,52] are assigned to clusters with ages t ≳ 100 Myr.

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