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Table 4.
Input parameters of the important physical models used to fit the SEDs of our sample with CIGALE.
| Parameter | Values |
|---|---|
| Star formation history | |
| Delayed | |
| Stellar age [Gyr] | Equally-spaced 32 values in [0.5, 8] |
| e-folding time (τ) [Gyr] | Equally-spaced 22 values in [0.5, 6] |
| Dust attenuation laws (a) | |
| (Calzetti et al. 2000) | |
| Color excess of young stars E(B − V) mag | 10 values in [0.1, 1] |
| Color excess of old stars (fatt) | 0.1, 0.3, 0.5, 0.8, 1.0 |
| (Charlot & Fall 2000) | |
V-band attenuation in the ISM ( ) mag |
30 values in [0.3–3] |
Av /( ) |
0.1, 0.3, 0.5, 0.8, 1 |
| Power law slope of the ISM | −0.7 |
| Power law slope of the BC | −0.7 |
| Dust emission | |
| (Draine et al. 2014) | |
| Mass fraction of PAH | 1.12, 2.50, 3.90, 5.26, 6.63 |
| Minimum radiation field (Umin) | 1, 5, 15, 25, 35 |
| Power law slope (α) | 2 |
| Dust fraction in PDRs (γ) | 5 values in [0.01, 0.2] |
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