Table B.1.
[Fe/H] values for the cluster sample.
| Star cluster | [Fe/H] | Reference | Star cluster | [Fe/H] | Reference | Star cluster | [Fe/H] | Reference |
|---|---|---|---|---|---|---|---|---|
| NGC 1651 | −0.37 ± 0.20 | 1 | SL 8 | −0.40 ± 0.20 | 14 | SL 862 | −0.47 ± 0.07 | 15 |
| −0.82 ± 0.44 | 2 | −0.50 ± 0.30 | 20 | −0.85 ± 0.20 | 14 | |||
| −0.07 ± 0.10 | 3 | |||||||
| −0.63 to −0.45 | 4 | SL 363 | −0.49 ± 0.12 | 15 | L 6 | −1.24 ± 0.03 | 17 | |
| −0.30 ± 0.03 | 5 | −0.90 ± 0.20 | 18 | |||||
| −0.70 ± 0.10 | 6 | SL 388 | −0.65 ± 0.20 | 14 | ||||
| −0.58 ± 0.06 | 21 | L 19 | −0.75 ± 0.10 | 18 | ||||
| NGC 1795 | −0.40 ± 0.10 | 12 | ||||||
| −0.23 ± 0.20 | 1 | SL 509 | −0.54 ± 0.09 | 15 | L 27 | −1.14 ± 0.06 | 17 | |
| −1.18 ± 0.09 | 21 | −1.30 ± 0.30 | 18 | |||||
| NGC 1846 | −0.50 ± 0.10 | 13 | −0.85 ± 0.30 | 20 | ||||
| −0.76 ± 0.20 | 1 | |||||||
| −0.70 ± 0.08 | 19 | SL 549 | −0.70 ± 0.20 | 9 | ||||
| NGC 2155 | −0.55 ± 0.20 | 1 | SL 555 | −0.70 ± 0.20 | 16 | |||
| −0.60 ± 0.20 | 7 | |||||||
| −0.98 to −0.80 | 8 | SL 817 | −0.41 ± 0.05 | 15 | ||||
| −0.44 ± 0.86 | 2 | −0.50 ± 0.20 | 14 | |||||
| ∼−0.80 | 9 | |||||||
| ∼−0.70 | 10 | SL 842 | −0.60 ± 0.20 | 14 | ||||
| ∼−1.0 | 11 | −0.36 ± 0.20 | 1 | |||||
| −0.70 ± 0.10 | 6 |
Notes. Reference (technique) : (1) Olszewski et al. (1991) (low-resolution spectroscopy); (2) Leonardi & Rose (2003) (integrated spectroscopy); (3) Sarajedini et al. (2002) (NIR photometry); (4) Dirsch et al. (2000) (Strömgren photometry); (5) Mucciarelli et al. (2008) (high-resolution spectroscopy); (6) Kerber et al. (2007) (HST photometry); (7) Rich et al. (2001) (HST photometry); (8) Bertelli et al. (2003) (VLT photometry); (9) Piatti et al. (2003) (Washington photometry); (10) Woo et al. (2003) (VLT photometry); (11) Sarajedini (1998) (HST photometry); (12) Glatt et al. (2010) (BVI photometry); (13) Grocholski et al. (2006) (low-resolution spectroscopy); (14) Bica et al. (1998) (Washington photometry); (15) Sharma et al. (2010) (low-resolution spectroscopy); (16) Geisler et al. (2003) (Washington photometry); (17) Parisi et al. (2009) (low-resolution spectroscopy); (18) Piatti et al. (2005) (Washington photometry); (19) Song et al. (2019) (high-resolution spectroscopy); (20) Palma et al. (2016) (Washington photometry); (21) Pieres et al. (2016) (DES photometry).
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