Table D.1
Parameters of star clusters are presented here.
| cluster | cluster | RA | Dec | log(age/yr) | Av | distance | [Fe/H] | Teff, IRFM | Teff, isochrone | NBSS | NMS | fBSS/MS |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| name | type | (deg) | (deg) | (mag) | (pc) | (dex) | (K) | (K) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) |
| NGC104 | GC | 6.175 | −72.024 | 10.070 ± 0.011 | 0.124 | 4367 | −0.65 | 5903 ± 92 | 5995 | 415 | 13691 | 0.06 ± 0.002 |
| NGC288 | GC | 13.381 | −26.529 | 10.064 ± 0.002 | 0.031 | 9000 | −0.8 | 6066 ± 116 | 6173 | 150 | – | – |
| NGC362 | GC | 15.885 | −70.781 | 10.068 ± 0.013 | 0.155 | 9090 | −1.3 | 6248 ± 160 | 6368 | 137 | 1578 | 0.171 ± 0.011 |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
| Berkeley39 | OC | 116.893 | −4.735 | 9.811 ± 0.029 | 0.394 | 4156 | 0.0 | 5932 ± 84 | 6038 | 22 | 264 | 0.14 ± 0.025 |
| Berkeley32 | OC | 104.738 | 6.379 | 9.686 ± 0.022 | 0.553 | 3321 | −0.3 | 6286 ± 125 | 6403 | 14 | 139 | 0.151 ± 0.035 |
| Collinder261 | OC | 189.802 | −68.492 | 9.898 ± 0.065 | 0.999 | 2706 | 0.1 | 5772 ± 72 | 5865 | 64 | 460 | 0.228 ± 0.025 |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
Notes. The complete table is made available at the CDS. The list of columns represented here is: (1) Name of the cluster; (2) whether it is a globular cluster (GC) or open cluster (OC); (3) and (4) represents central coordinates of the cluster, (5) age of the cluster in log scale, (6) extinction (AV) towards the cluster, (7) distance to the cluster, (8) metallicity of the cluster, (9) mean effective temperature of BSS populations in that cluster using IRFM method, (10) mean effective temperature of BSS populations in that cluster using isochrone method; (11) number of BSSs detected in that cluster; (12) number of main sequence (MS) stars in the luminosity range between the MS turn-off (MSTO) and MSTO+1 mag in that cluster; (13) fractional BSSs population to MS populations.
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