Table 2
Ages from integrated spectroscopy/photometry for the main targets.
| ID | AGE [Gyr]a | ||||
| P05 | Be05+BC03 | Be05+T03 | W10 | F10 | |
|
|
|||||
| B058-G119 | 6.4 ± 4.1 | ... | ... | 2.02 ± 0.10 | 4.000 ± 1.325 |
| B292-G010 | 9.2 ± 3.3 | 2.7 ± 1.2 | 5.9 ± 3.4 | 1.00 ± 0.10 | 0.003 ± 0.000 |
| B337-G068 | 4.9 ± 2.9 | 2.6 ± 1.9 | 6.6 ± 3.2 | 2.03 ± 0.10 | 1.900 ± 0.360 |
| B350-G162 | 9.3 ± 2.3 | 9.8 ± 2.5 | 12.4 ± 4.7 | 1.99 ± 0.10 | 1.278 ± 0.148 |
Notes.
Ages from Puzia et al. (2005, P05); Beasley et al. (2005, Be05); Wang et al. (2010, W10); Fan et al. (2010, F10). Beasley et al. (2005) derived two set of age estimates by comparing the same spectra with two different sets of SPSS models by Bruzual & Charlot (2003, BC03) and Thomas et al. (2003, T03); we report both estimates in this table. Caldwell et al. (2011) do not provide an age estimate for these clusters, but assign a conventional value of 14 Gyr to all of them.
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