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Table 2.
Parameters and values for the modules used with CIGALE for the LLAGN sample.
| Parameter | Model/values |
|---|---|
| Star formation history: delayed model | |
| Age of the main population | 3000, 5000, 7000, 9000, 11 000 Myr |
| e-folding time | 100, 500, 1000, 3000 Myr |
| Burst stellar mass fraction | 0.0 |
| Simple Stellar population: Bruzual & Charlot (2003) | |
| Initial mass function | Chabrier (2003) |
| Metallicity | 0.008 (LMC), 0.02 (Solar) |
| Dust extinction | |
| Dust attenuation recipe | Modified Calzetti et al. (2000) |
| E(B − V)lines | 0.1, 0.3, 0.5, 0.7, 0.9 |
| E(B − V)factor | 0.1, 0.44, 0.7 |
| Power-law slope modifying the attenuation curve | −0.4, 0.0 |
| Dust emission: Themis (Jones et al. 2017) | |
| qHAC | 0.02, 0.17, 0.24 |
| Umin | 0.1, 1.0, 10.0, 50.0 |
| α slope in dMdust ∝ U−αdU | 2.1, 2.5, 2.9 |
| γ | 0.4 |
| AGN module: SKIRTOR | |
| Torus optical depth at 9.7 microns τ9.7 | 3, 11 |
| Torus opening angle | 10°, 70° |
| Viewing angle | 10° (Type I), 80° (Type II) |
| Disk spectrum | ADAF + TDk |
| Delta parameter for the truncated disk | 0, 0.25, 0.5 |
| AGN fraction | 0.001, 0.01, 0.05, 0.1, 0.2, 0.3 |
| E(B − V) of polar dust | 0.0 |
| X-ray module: this paper | |
| AGN photon index Γ | 1.6, 2.0, 2.5, 3.0, 3.5 |
| αIRX | 0, 0.15, 0.3, 0.45, 0.6 |
| Deviation from expected LMXB and HMXB | 0., 0. |
| Total number of models per redshift | 671, 846, 400 |
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