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Table 3
Summary of the results from the SFH fit to the highest peak.
| Cluster | Fitted SFH | Fitted SFH of the corresponding |
| of highest peak | highest peak in artificial cluster | |
|
|
||
| NGC 1831 | 924 ± 126 Myr | 949 ± 57 Myr |
| NGC 1847 | 56.7 ± 4.8 Myr | 60.0 ± 1.0 Myr |
| NGC 1850 | 93.4 ± 18.3 Myr | 96.2 ± 5.7 Myr |
| NGC 2004 | 19.5 ± 1.4 Myr | 20.1 ± 1.5 Myr |
| NGC 2100 | 19.5 ± 2.0 Myr | 20.6 ± 1.6 Myr |
| NGC 2136 | 123.3 ± 22.6 Myr | 130.2 ± 9.6 Myr |
| NGC 2157 | 98.3 ± 13.2 Myr | 102.2 ± 8.4 Myr |
| NGC 2249 | 1110 ± 139 Myr | 1235 ± 111 Myr |
|
|
||
| NGC 1856 | 281 ± 33.6 Myr | − |
| NGC 1866 | 177 ± 18.4 Myr | − |
Notes. The last two clusters (NGC 1856 and NGC 1866) are not studied in this work. They were already analyzed by Bastian & Silva-Villa (2013).
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