Table 3.
Reddenings used for the individual clusters in Fig. 10.
| Cluster | EB − V | EGBP − GRP | Ref. | [Fe/H] | Ref. | |
|---|---|---|---|---|---|---|
| NGC 6819 | 0.15 | ⇒ | 0.201 | 1 | 0.05 | 6 |
| NGC 6811 | 0.048 | ⇒ | 0.065 | 2 | −0.05 | 6 |
| Hyades | 0.027 | ⇒ | 0.036 | 3 | 0.13 | 7 |
| M 67 | 0.04 | ⇒ | 0.054 | 4 | 0.03 | 8 |
| Ru 147 | 0.075 | ⇐ | 0.1 | 5 | 0.12 | 6 |
Notes. Calculated reddenings use the relationship 1.339 ⋅ EB − V = EGBP − GRP (Casagrande & VandenBerg 2018) and the arrow indicates the direction of the calculation.
References. (1) Meibom et al. (2015); (2) Curtis et al. (2019); (3) Joner et al. (2006); (4) Barnes et al. (2016a); (5) this work; (6) Donor et al. (2020); (7) Netopil et al. (2016); (8) Casamiquela et al. (2017, 2019).
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