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Table 2
Various combinations of the basic parameters that we explore in our stellar models.
| SFH | Extinction law | Nebular emission |
|
|
||
| Exp. declining | Calzetti/SMC | with/without |
| constant rate | ′′ | ′′ |
| Exp. rising | ′′ | ′′ |
Notes. There are a total of ten scenarios, to which we add the commonly used one, that supposes CSFR, Calzetti, no nebular emission, and the age prior of tmin = 100 Myr.
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