Table A.1
Averaged literature values of fundamental parameters of the studied star clusters.
| Star Cluster | (m − M)0 (mag) | Log(age /yr) | [Fe/H] (dex) | Method | References |
|---|---|---|---|---|---|
| B88 | 19.0 ± 0.10 | 8.12 ± 0.22 | -0.25 ± 0.15 | Photometry | 1;2 |
| B99 | — | 8.10 ± 0.01 | -0.84 ± 0.04 | Photometry; CaII triplet | 5;6 |
| B139 | 19.10 ± 0.11 | 8.06 ± 0.12 | -0.30 ± 0.24 | Photometry | 1;2 |
| B168 | 18.96 ± 0.07 | 9.82 ± 0.06 | -1.08 ± 0.06 | Photometry; CaII triplet | 3;4 |
| BS116 | 18.75 ± 0.12 | 9.27 ± 0.07 | -0.77 ± 0.12 | Photometry | 1 |
| BS121 | — | 9.45 ± 0.08 | -0.66 ± 0.07 | CaII triplet | 7;8 |
| BS188 | 18.61 ± 0.12 | 9.26 ± 0.05 | -0.94 ± 0.06 | Photometry; CaII triplet | 3;4 |
| H86-97 | — | 8.50 ± 0.02 | -0.70 ± 0.04 | Photometry; CaII triplet | 6;9 |
| HW31 | — | 9.28 ± 0.11 | -0.89 ± 0.04 | CaII triplet; Photometry | 2;8;10 |
| HW41 | — | 9.38 ± 0.29 | -0.67 ± 0.05 | CaII triplet; Photometry | 2;8;10 |
| HW47 | — | 9.48 ± 0.07 | -0.96 ± 0.22 | CaII triplet; Photometry | 8;11;12 |
| HW56 | 18.69 ± 0.09 | 9.47 ± 0.04 | -0.90 ± 0.14 | Photometry; CaII triplet | 1;4 |
| HW64 | 19.19 ± 0.08 | 7.47 ± 0.31 | -0.38 ± 0.20 | Photometry | 1 |
| HW67 | 18.71 ± 0.13 | 9.35 ± 0.05 | -0.74 ± 0.12 | Photometry; CaII triplet | 1;6 |
| HW73 | 19.18 ± 0.04 | 8.01 ± 0.08 | -0.32 ± 0.22 | Photometry | 1;2 |
| HW77 | 18.83 ± 0.12 | 9.05 ± 0.04 | -1.02 ± 0.11 | Photometry | 13 |
| HW84 | — | 9.29 ± 0.05 | -0.90 ± 0.05 | Photometry | 7;8;12 |
| HW86 | 18.53 ± 0.09 | 9.15 ± 0.05 | -0.65 ± 0.09 | CaII triplet; Photometry | 7;8;14 |
| IC1655 | 18.66 ± 0.04 | 8.18 ± 0.20 | -0.61 ± 0.18 | Photometry | 1;2 |
| L2 | 18.72 ± 0.10 | 9.59 ± 0.02 | -1.29 ± 0.13 | Photometry; CaT lines | 13;21;22 |
| L3 | 18.64 ± 0.14 | 9.08 ± 0.11 | -0.75 ± 0.33 | Photometry | 10;21;24 |
| L4 | 18.65 ± 0.10 | 9.90 ± 0.06 | -1.08 ± 0.04 | Photometry; CaII triplet | 3;7;8 |
| L6 | 18.70 ± 0.09 | 9.94 ± 0.06 | -1.24 ± 0.03 | Photometry; CaII triplet | 3;7;8 |
| L7 | — | 9.17 ± 0.04 | -0.82 ± 0.06 | CaII triplet; Photometry | 6;7;20 |
| L9 | 18.93 ± 0.07 | 9.22 ± 0.07 | -0.66 ± 0.01 | Photometry; CaII triplet | 6;12;13 |
| L11 | — | 9.48 ± 0.06 | -1.07 ± 0.18 | Deep Photometry; CaII triplet | 7;8;15 |
| L13 | 18.66 ± 0.04 | 8.75 ± 0.08 | -1.05 ± 0.06 | Photometry; CaII triplet | 6;13;18 |
| L17 | — | 9.64 ± 0.06 | -0.84 ± 0.03 | CaII triplet | 7;8 |
| L19 | — | 9.48 ± 0.03 | -0.87 ± 0.02 | Photometry; CaII triplet | 1;19;20 |
| L27 | 18.84 ± 0.10 | 9.55 ± 0.06 | -1.01 ± 0.10 | Photometry; CaII triplet | 2;3;7;19;22;23 |
| L58 | — | 9.13 ± 0.28 | -0.78 ± 0.02 | Photometry; CaII triplet | 2;6;25 |
| L73 | 18.83 ± 0.13 | 9.27 ± 0.04 | -0.65 ± 0.13 | Photometry | 1 |
| L95 | 19.18 ± 0.10 | 7.94 ± 0.34 | -0.36 ± 0.27 | Photometry | 1;2 |
| L100 | 18.81 ± 0.06 | 9.46 ± 0.04 | -0.75 ± 0.08 | Photometry; CaII triplet | 1;4;11 |
| L108 | — | 9.27 ± 0.09 | -0.88 ± 0.18 | CaII triplet; Photometry | 7;8 |
| L110 | 18.95 ± 0.10 | 9.88 ± 0.06 | -1.03 ± 0.05 | Photometry; CaII triplet | 14;7;8 |
| L116 | — | 9.44 ± 0.20 | -1.0 ± 0.11 | Photometry; CaII triplet | 16;17 |
| NGC416 | 18.96 ± 0.07 | 9.78 ± 0.04 | -0.85 ± 0.04 | Photometry; CaII triplet | 23;21;26 |
| NGC458 | 18.74 ± 0.03 | 8.14 ± 0.07 | -0.39 ± 0.08 | Photometry | 1;27 |
| OGLE-SMC 133 | — | 9.80 ± 0.40 | -0.80 ± 0.07 | Photometry; CaII triplet | 2;6 |
References. (1) Piatti (2022); (2) Glatt et al. (2010); (3) Piatti (2022); (4) Dias et al. (2021); (5) Maia et al. (2014); (6) Parisi et al. (2015); (7) Parisi et al. (2009); (8) Parisi et al. (2014); (9) Chiosi et al. (2006); (10) De Bortoli et al. (2022); (11) Parisi et al. (2022); (12) Piatti et al. (2005); (13) Saroon et al. (2023); (14) Oliveira et al. (2023); (15) Livanou et al. (2013); (16) Piatti et al. (2001); (17) Parisi et al. (2022); (18) Nayak et al. (2018); (19) Narloch et al. (2021); (20) Gatto et al. (2021); (21) De Grijs & Bono (2015); (22) Dias et al. (2022); (23) Milone et al. (2023); (24) Dias et al. (2014); (25) Maia et al. (2019); (26) Glatt et al. (2008); (27) Alcaino et al. (2003).
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