Table 1
Input parameters for CIGALE.
| Parameter | Value | Units |
|---|---|---|
| Pop. synth. mod. | Bruzual & Charlot (2003) | |
| Dust model | Draine & Li (2007) | |
| IMF | Salpeter | |
| Metallicity | 0.02 | |
| Age | 1–301, step 2 | Myr |
| Extinction law | Calzetti | |
| E(B−V) | 0.0,0.1,0.2,0.3,0.4 | mag |
| UV bump amplitude | 0, 1.5, 3 | |
| QPAH | 0.47, 3.90, 7.32 | |
| Umin | 0.1, 1.0, 5.0, 10.0 | |
| α | 1.5, 2.0, 2.5 | |
| γ | 0.01, 0.3, 1.0 |
Notes. Line 1: population synthesis model. Line 2: dust model. Line 3: IMF. Line 4: stellar metallicity. Line 5: age interval andsampling. Line 6: extinction law (Calzetti et al. 2000). Line 7: attenuation. Line 8: amplitude of the UV bump (Noll et al. 2009). Line 9: mass fraction of the dust composed of PAH particles containing <103 atoms (Draine & Li 2007). Line 10: diffuse interstellar radiation field (Draine & Li 2007). Line 11: power-law index of the interstellar radiation field (Draine & Li 2007). Line 12: fraction of the dust mass that is close to OB associations and is exposed to a stellar radiation field with intensity U > Umin (Draine & Li 2007).
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