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Table 3.
Assumptions used for the sensitivity analysis.
| Model | Stellar lib. | IMF | Max zf | Z/Z⊙ | Prior shapes | SFH |
|---|---|---|---|---|---|---|
| (metallicity-age) | ||||||
| BC03 | MILES | Chabrier | 6 | 0.02–2.5 | log-lin | SSP |
| BC03 | MILES | Chabrier | 11 | 0.02–2.5 | log-lin | SSP |
| BC03 | MILES | Chabrier | 6 | 0.02–2.5 | lin-lin | SSP |
| BC03 | MILES | Chabrier | 6 | 0.02–2.5 | log-log | SSP |
| BC03 | MILES | Chabrier | 6 | 0.02–2.5 | lin-lin | Top-hat 0.5 Gyr |
| BC03 | STELIB | Chabrier | 6 | 0.02–2.5 | log-lin | SSP |
| Maraston | MILES | Kroupa | 6 | 0.02–2.5 | log-lin | SSP |
| BC03 | STELIB | −1.5 slope | 6 | 0.2–2.5 | log-lin | SSP |
| BC03 | STELIB | Salpeter | 6 | 0.2–2.5 | log-lin | SSP |
| BC03 | STELIB | −3.5 slope | 6 | 0.2–2.5 | log-lin | SSP |
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