Open Access
Table C.1.
Parameters adopted in the CIGALE fit.
| Parameter | Value |
|---|---|
| Delayed SFH (Ciesla et al. 2015) | |
| τmain [Myr] | 100, 250, 500 |
| τburst [Myr] | 10, 50 |
| fburst | 0.0, 0.5, 0.99 |
| Agemain [Myr] | 500, 800, 1000 |
| Ageburst [Myr] | 1, 5, 10 |
| Single stellar population (Bruzual & Charlot 2003) | |
| IMF | Chabrier (2003) |
| Metallicity | 0.02 |
| Ageseparation [Myr] | 10 |
| Nebular emission (Inoue 2011) | |
| log U | -2.0 |
| fesc | 0.0 |
| fdust | 0.0 |
| Line width [km s−1] | 300.0 |
| Dust attenuation (Calzetti et al. 2000) | |
| E(B − V)line | 0.03, 0.1, 0.3, 1, 3 |
| fE(B − V) | 0.44 |
| λUV, bump [nm] | 217.5 |
| FWHMUV, bump [nm] | 35.0 |
| AUV, bump [nm] | 0.0 |
| δ | 0.0 |
| Extinction law of emission lines | the Milky Way |
| RV | 3.1 |
| Dust emission (Dale et al. 2014) | |
| AGN fraction | 0.0 |
| αIR, AGN | 0.25, 1.0, 4.0 |
| AGN model (Stalevski et al. 2016) | |
| τ9.7 | 3, 7, 11 |
| p | 1.0 |
| q | 1.0 |
| oa [deg] | 10, 30, 50, 70, 80 |
| Rratio | 20 |
| Mcl | 0.97 |
| i [deg] | 0, 20, 40, 60, 80, 90 |
| fAGN | 0.1,0.5,0.99 |
| Extinction law of polar dust | Calzetti et al. (2000) |
 |
0.03, 0.1, 0.3, 1, 3 |
 [K] |
30, 100, 300, 1000 |
| Emissivity of polar dust | 1.6 |
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