Table D.1.
Comparison between the SC ages estimated in this work and literature values.
| ID | log t (Our) | log t (Lit.) | Reference | Simbad Name |
|---|---|---|---|---|
| YMCA-0049 | 9.60 | 9.66 ± 0.02 | 1 | L 32 |
| YMCA-0050 | 9.70 | 9.72 ± 0.04 | 1 | ESO 51-9 |
| YMCA-0051 | 9.20 | 9.20 ± 0.05 | 1 | HW 84 |
| YMCA-0056 | 9.25 | 9.10 ± 0.10 | 2 | KMHK 5 |
| YMCA-0058 | 9.30 | 9.30 ± 0.10 | 2 | KMHK 11 |
| YMCA-0059 | 9.25 | 9.21 ± 0.05 | 3 | NGC 1644 |
| YMCA-0065 | 9.20 | 9.30 ± 0.02 | 4 | KMHK 1751 |
| YMCA-0070 | 10.10 | 10.07 ± 0.02 | 3 | NGC 2257 |
| YMCA-0072 | 9.00 | 9.08 ± 0.05 | 5 | KMHK 1760 |
Notes: The different columns display: YMCA SC IDs, ages estimated in this study, ages from previous studies with references, literature IDs from SIMBAD Astronomical Database. Our estimated uncertainty for SC ages is σlog t = 0.2 dex, as described in Sect. 6.3. References are: (1) Parisi et al. (2014); (2) Piatti et al. (2018); (3) Milone et al. (2023); (4) Piatti & Bastian (2016); (5) Maia et al. (2019).
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