Table 3
Percentages of the total stellar mass in three different stellar subpopulations: young (younger than 0.5 Gyr), intermediate (older than 0.5 Gyr and younger than 5.0 Gyr), and old (older than 5.0 Gyr).
| Approach | Young | Intermediate | Old |
| (%) | (%) | % | |
|
|
|||
| CMD | 4.3 | 49.0 | 46.7 |
| STECKMAP | 4.2 | 49.4 | 46.4 |
| ULySS “SSP” | 3.9 | 51.4 | 44.7 |
| ULySS “const. SFR” | 2.4 | 51.3 | 46.3 |
| STARLIGHT “SSP” | 9.0 | 54.9 | 36.1 |
| STARLIGHT “const. SFR” | 7.7 | 33.1 | 59.2 |
| Bica (*) | 2.0 | 10.0 | 88.0 |
Notes. In the cases of ULySS and STARLIGHT we show the results from the SSP and the mock spectral template approaches. We include the Bica (*) analysis for historical comparison. For information about the Bica analysis see Appendix A.
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