Open Access
Table 1.
CIGALE modules.
| Parameters | Value |
|---|---|
| Delayed SFH with optional exponential burst Boquien et al. 2019 | |
| e-folding time of the main stellar population [106 yr] | 500, 1000.0, 4000.0, 5000.0 |
| Age of the galaxy’s main stellar population [106 yr] | 500, 1000.0, 2000.0, 5000.0 |
| e-folding time of the late starburst population [106 yr] | 50.0 |
| Age of the late burst [106 yr] | 10.0 |
| Mass fraction of the late burst population | 0.00 |
| multiplicative factor controlling the amplitude of SFR if normalization is True | 1.0 |
| SSP Bruzual & Charlot 2003 | |
| Initial mass function | Salpeter 1955 |
| Metallicity | 0.02 |
| Age of separation between the young and old star populations | 10.0 |
| Dust attenuation Charlot & Fall 2000 | |
| Logarithm of the V-band attenuation in the ISM | 0.1, 0.17, 0.28, 0.46, 0.77, 1.29, 2.15, 3.59, 5.99, 10.0 |
| Ratio of V-band attenuation from old and young stars | 0.44 |
| Power-law slope of the attenuation in the ISM | –0.7,–0.5 |
| Power-law slope of the attenuation in the birth cloud | –0.7 |
| Dust emission Draine 2014 | |
| Mass fraction of PAH (qPAH) | 1.12, 2.5, 3.9, 4.58, 5.95, 6.63, 7.32 |
| Minimum radiation field (Umin) | 0.1, 1.0, 10.0, 20.0, 50.0 |
Power-law slope α ( ) |
2.0, 3.0 |
| Fraction illuminated from Umin to Umax | 0.01, 0.1 |
| SKIRTOR AGN | |
| τAGN | 3 |
| oaAGN | 40, 70 |
| RAGN | 20 |
| inclination (i) | 0, 10, 30, 80 |
| fracAGN (computed for the 3-30 micron range) | 0.0, 0.01, 0.03, 0.05, 0.1, 0.2, 0.3, 0.4, 0.5, 0.6 |
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