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Table E.1.
Parameter space in CIGALE
| model | parameter | values |
|---|---|---|
| SFH | e-folding time of the main population | 500, 1500, 3500, 5500 Myrs |
| delayed τ+starburst | age the main population | 500, 1000,1700, 2300, 3500 Myrs |
| e-folding time of the late starburst population | 10000 Myrs | |
| age of the late starburst population | 30,80,120 Myrs | |
| mass fraction of the late starburst population | 0.0,0.05, 0.1, 0.2, 0.25, 0.3 | |
| SSP | IMF | Salpeter |
| Bruzual & Charlot (2003) | metallicity | solar |
| dust attenuation | V-band attenuation in the birth clouds | 0, 0.1, 0.4, 0.7, 1.1, 1.5, 1.9, 2.5, 3, 3.5 |
| double power-law | power-law slope of the attenuation in the birth clouds | -0.7 |
| AvISM/ AvBC | 0.8 | |
| power-law slope of the attenuation in the ISM | -0.7 | |
| dust emission | Mass fraction of PAH | 1.12 |
| Draine et al. (2014) | minimum radiation field | 5,15,40 |
| power-law slope α in dM/dU ∝Uα | 2 | |
| AGN templates | Full opening angle of the dust torus | 100° |
| Fritz et al. (2006) | viewing angle | 10,30,40,60,70,90° |
| AGN fraction | 0.0,0.1, 0.2, 0.3, 0.45, 0.6, 0.75, 0.9, 0.99 | |
| AGN templates | average edge-on optical depth at 9.7 micron | 7, 11 |
| SKITOR | half opening angle | 40 ° |
| viewing angle | 10, 30, 40, 60, 70, 90 ° | |
| AGN fraction | 0.0,0.1, 0.2, 0.3, 0.45, 0.6, 0.75, 0.9, 0.99 | |
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