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Table 1
Age and metallicity estimates obtained in this study, compared to previous works.
| Reference | Age (Myr) | Z | Notes |
|
|
|||
| Unresolved stellar population | |||
| This work | ~4–6 | 0.004 | Age from HαEW, Z from strong lines |
| This work | ~4 | 0.008 | Age and Z from SED fitting |
| Resolved stellar population | |||
| Melnick et al. (1989) | ~ 2.5 ± 2 | 0.007 | Age from CMD, Z from strong lines |
| Pandey et al. (2000) | ≲ 1 | – | Age from CMD |
| Sagar et al. (2001) | 3 ± 2 | 0.020 | Age from CMD, solar Z assumed |
| Sung & Bessell (2004) | ≲ 5 | – | Age from CMD |
| Harayama et al. (2008) | ~ 2.5 | 0.020 | Age from CMD, solar Z assumed |
| Melena et al. (2008) | ≲ 4 | 0.020 | Age from CMD, solar Z assumed |
| This work | ≲ 10 | – | Age from CMD |
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