Table 3
Reference data for 14 globular clusters used in the construction of the combined HRD (Fig. 3).
| NGC | DM | Age | [Fe/H] | E(B − V) | Memb |
|---|---|---|---|---|---|
| (Gyr) | |||||
| 104 | 13.266 | 12.75a | −0.72 | 0.04 | 21580 |
| 288 | 14.747 | 12.50a | −1.31 | 0.03 | 1953 |
| 362 | 14.672 | 11.50a | −1.26 | 0.05 | 1737 |
| 1851 | 15.414 | 13.30c | −1.18 | 0.02 | 744 |
| 5272 | 15.043 | 12.60b | −1.50 | 0.01 | 9086 |
| 5904 | 14.375 | 12.25a | −1.29 | 0.03 | 3476 |
| 6205 | 14.256 | 13.00a | −1.53 | 0.02 | 10311 |
| 6218 | 13.406 | 13.25a | −1.37 | 0.19 | 3127 |
| 6341 | 14.595 | 13.25a | −2.31 | 0.02 | 1432 |
| 6397 | 11.920 | 13.50a | −2.02 | 0.18 | 10055 |
| 6656 | 12.526 | 12.86c | −1.70 | 0.35 | 9542 |
| 6752 | 13.010 | 12.50a | −1.54 | 0.04 | 10779 |
| 6809 | 13.662 | 13.50a | −1.94 | 0.08 | 8073 |
| 7099 | 14.542 | 13.25a | −2.27 | 0.03 | 1016 |
Notes. Data on distance moduli (DM), [Fe/H] and E(B–V) from Harris (1996), 2010 edition, (a) Dotter et al. (2010), (b) Denissenkov et al. (2017), (c) Powalka et al. (2017) for age estimates. Memb: cluster members with photometry after application of photometric filters.
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