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Table 2.
Summary of parameters of UBC 103, UBC 114 and UBC 587 derived from the isochrone fitting compared with the results from Cantat-Gaudin et al. (2020).
| Age | AV | DM | |
|---|---|---|---|
| (Ma) | (mag) | (mag) | |
| UBC103 | |||
| Cantat-Gaudin | 22 | 1.4 | 12.37 |
| This work | 70 ± 10 | 1.6 | 12.41 |
| UBC114 | |||
| Cantat-Gaudin | 50 | 1.0 | 10.9 |
| This work | < 30 | 1.3 | 10.84 |
| UBC587 | |||
| Cantat-Gaudin | 14 | 3.1 | 12.2 |
| This work | > 3 & < 10 | > 3.3 (1) | 12.44 |
Notes. (1)Although many cluster members form a sequence that can be fitted by AV = 3.3, many others have an obviously higher exinction.
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