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Table 2
CIGALE input parameters and their ranges whenever appropriate.
| Parameter | Value |
|
|
|
| SFH | Delayed |
| Age (Gyr) | 0.1, 0.5, 1, 2, 3, 4, 5, |
| 6, 7, 8, 9, 10, 11, 12, 13 | |
| e-folding time in Gyr (τmain) | 0.5, 1, 3, 5, 6, 10, 20 |
| Possible quenching or burst (rSFR) | 0., 0.1, 0.2, 0.3, 0.4, 0.5, 0.6, |
| 0.7, 0.8, 0.9, 1., 2., 4., 8., 16. | |
| Duration of the episode in Gyr | 0.1, 0.4 |
|
|
|
| Stellar population models | Bruzual & Charlot (2003) |
| IMF | Salpeter |
| Metallicity | 0.02 |
|
|
|
| Dust attenuation E(B−V) | 0.01, 0.05, 0.1, 0.15, 0.2, 0.25, |
| 0.3, 0.35, 0.4, 0.45, 0.5, 0.6, 0.7, 0.9 | |
|
|
|
| Dust template | Dale et al. (2014) |
|
|
|
| IR power-law slope (αb) | 1.5, 2.5 |
|
|
|
| AGN template | Fritz et al. (2006) |
|
|
|
| Ratio between outer and inner radius of the torus (rratio) | 60 |
| Optical depth at 9.7 μm (τ) | 1, 6 |
| Parameter linked to the radial dust distribution in the torus (β) | −0.5 |
| Parameter linked to the angular dust distribution in the torus (γ) | 0 |
| Angular opening angle of the torus (θ) | 100 |
| Angle with line of sight (ψ) | 0, 90 |
| fracAGN | 0.0, 0.05, 0.1, 0.15, 0.2, |
| 0.3, 0.4, 0.5, 0.6, 0.8 | |
|
|
|
| Number of models per redshift bin (Delta(z) = 0.01): | 2 808 000 |
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