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Table 1.
X-CIGALE modules and input variable parameters used to create the stellar and AGN components of the composite models.
| Stellar component | ||||
|---|---|---|---|---|
| Star formation history and dust attenuation: | ||||
| Delayed modeled with a recent burst | ||||
| Age of the main population | agemain | 1.5, 2, 3, 4, 5, 7 Gyr | ||
| e-folding time | τmain | 0.5,1,2,3,4,5 Gyr | ||
| Age of the burst | ageburst | 100, 500 Myr | ||
| Burst stellar mass fraction | fburst | 0.0, 0.01, 0.02, 0.05, 0.1, 0.15, 0.2 | ||
| Dust absorption & re-emission | ||||
| Calzetti 2000 law, | E(B − V) | 0.05, 0.1, 0.2, 0.3, 0.4, 0.5 | ||
| Dale et al. IR templates | α slope | 1.5, 2.0, 2.5 | ||
| AGN component: SKIRTOR2016 | ||||
| Viewing angle | 30 deg | |||
| AGN dust luminosity fraction | fAGN | 0,0 to 0.9 (0.1 step) | ||
| Polar dust extinction law | SMC, Gaskell2004 (G04) | |||
| E(B-V) of polar dust | E(B − V)pd | 0.0,0.01, 0.1, 0.15, 0.2, 0.25, 0.3 | ||
| Temperature of Polar dust | Tpd | 100, 500, 1000, 2000 K | ||
Notes. We refer to Yang et al. (2020) for the description and values of the input fixed parameters which are not described here. See text for details.
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