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Table 3.
Parameters and values for the modules used with CIGALE.
Parameter | Model/values |
---|---|
Star formation history: delayed model and recent burst | |
Age of the main population | 500, 1000, 3000, 5000, 7000 Myr |
e-folding time | 500, 1000, 3000, 5000, 7000 Myr |
Age of the burst | 20, 200 Myr |
e-folding time of the burst | 50 Myr |
Burst stellar mass fraction | 0.0, 0.1 |
Simple stellar population: Bruzual & Charlot (2003) | |
Initial mass function | Chabrier (2003) |
Metallicity | 0.02 (Solar) |
Galactic dust extinction | |
Dust attenuation recipe | Modified Calzetti et al. (2000) |
E(B − V)young | 0.0, 0.1, 0.25, 0.5, 0.75, 0.9 |
![]() |
217.5 nm |
Galactic dust emission: Dale et al. (2014) | |
α slope in dMdust ∝ U−αdU | 1.0, 1.5, 2.0, 2.5, 3 |
Nebular | |
log U | −2.0 |
Width lines | 300 km s−1 |
AGN module: SKIRTOR | |
Torus optical depth at 9.7 microns τ9.7 | 3, 7 |
Torus density radial parameter p | 1.0 |
Torus density angular parameter q | 1.0 |
Angle between the equatorial plan and edge of the torus | 40° |
Ratio of the maximum to minimum radii of the torus | 20 |
Viewing angle | 30° (type 1), 70° (type 2) |
Disk spectrum | Schartmann (2005) |
Power-law index modifying the optical slope of the disk | −0.36 |
AGN fraction | 0.01, 0.1, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9, 0.99 |
Extinction law of polar dust | SMC |
E(B − V) of polar dust | 0.0, 0.01, 0.05, 0.1, 0.5, 1.0 |
Temperature of polar dust | 100 K |
Emissivity of polar dust | 1.6 |
X-ray module | |
AGN photon index Γ | 1.8 |
αox | −1.9, −1.75, −1.6, −1.45, −1.3, −1.15, −1.0 |
Maximum deviation from the αox − L2500 Å relation | 0.4 |
LMXB photon index | 1.56 |
HMXB photon index | 2.0 |
Total number of models per redshift | 5 544 000 |
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