Table A.1.
First ten of the 44 HRS+LRS clusters.
| Cluster | RA | Dec | log (age) | (m − M)0 | AV | AGTO | [Fe/H] |
|---|---|---|---|---|---|---|---|
| Blanco1 | 0.853 | −29.958 |  |
 |
 |
 |
0.000 |
| IC2391 | 130.292 | −52.991 |  |
 |
 |
 |
0.000 |
| IC2602 | 160.613 | −64.426 |  |
 |
 |
 |
0.000 |
| IC2714 | 169.373 | −62.719 |  |
 |
 |
 |
0.020 |
| IC4665 | 266.554 | +5.615 |  |
 |
 |
 |
−0.030 |
| IC4756 | 279.649 | +5.435 |  |
 |
 |
 |
0.000 |
| Melotte20 | 51.617 | +48.975 |  |
 |
 |
 |
0.140 |
| Melotte22 | 56.601 | +24.114 |  |
 |
 |
 |
0.000 |
| Melotte71 | 114.383 | −12.065 |  |
 |
 |
 |
−0.270 |
| NGC0188 | 11.798 | +85.244 |  |
 |
 |
 |
0.000 |
Notes. The values of log(age), distance moduli, and extinctions AV correspond to the median of each BASE-9 posterior distribution. AGTO column reports the extinction in G at the turnoff of each cluster. Uncertainties are given and correspond to the 16th (superscript) and 84th (subscript) percentiles of posterior distribution. [Fe/H] column lists the metallicity used in BASE-9 computations (the complete list is available at the CDS).
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