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Table 2.
Input parameters for the code CIGALE.
| Parameters | Values |
|---|---|
| Star formation history: | |
| Delayed star formation history + additional burst | |
| e-folding time of the main stellar population model (Myr) | 1000, 2000, 3000, 5000, 7000 |
| e-folding time of the late starburst population model (Myr) | 5000 |
| Mass fraction of the late burst population | 0.001, 0.01, 0.03, 0.1, 0.3 |
| Age (Myr) | 1000, 2000, 3000, 4000, 5000, 6500, 10000 |
| Age of the late burst (Myr) | 10, 40, 70 |
| Delayed star formation history | |
| e-folding time of the main stellar population model (Myr) | 1000, 2000, 3000, 4000, 5000, 6500, 8000 |
| Age (Myr) | 500, 1000, 3000, 4000, 5000, 6000, 7000, 8000, 9000, |
| 10000, 12000 | |
| Mass fraction of the late burst population | 0.0 |
| Single stellar population Bruzual & Charlot (2003) | |
| Initial mass function | Chabrier (2003) |
| Metallicities (solar metallicity) | 0.02 |
| Age of the separation between the young and the old star population (Myr) | 10 |
| Dust attenuation law Charlot & Fall (2000) | |
| AV in the Birth Clouds | 0, 0.05, 0.1, 0.3, 0.8, 1.2, 1.7, 2.3, 2.8, 3.3, 3.8, 4.0, 4.2 |
| Power law slopes of the attenuation in the birth clouds | −0.7 |
| BC to ISM factor (Av ISM/Av BC) | 0.5, 0.8 |
| slope ISM | −0.7 |
| Dust emission: | |
| Draine et al. (2014) | |
| Mass fraction of PAH | 1.12, 2.5, 3.19 |
| Minimum radiation field (Umin) | 5.0, 10.0, 25.0 |
| Power law slope dU/dM (Uα) | 2.0, 2.8 |
| Fraction illuminated from Umin to Umax (γ) | 0.02 |
| Dale et al. (2014) | |
| AGN fraction | 0 |
| Power law slope dU/dM (Uα) | 2.0 |
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