Open Access
Table D.1
Alternative parameters used in SED fitting with CIGALE.
| Parameter | Symbol | Values |
|---|---|---|
| Stellar population models: M05 (Maraston 2005) | ||
| Initial mass function | IMF | Salpeter (1955) |
| Metallicity | Z | 0.0004, 0.004, 0.008, 0.02, 0.05 |
| SFH: non-parametric SFH | ||
| Age of the oldest stars in the galaxy (Gyr) | age | 0.1, 0.5, 1, 3, 4.5, 6, 8, 10, 13 |
| Seeds of different SFH | N_SFH | 1000 |
| Dust attenuation: Charlot & Fall (2000) | ||
| V-band attenuation in the interstellar medium | AV_ISM | 0.01, 0.1, 0.4, 0.7, 1.1, 1.5, 2, 2.5, 3, 3.5, 5 |
| Dust emission: Dale et al. (2014) | ||
| AGN fraction | fracAGN | 0 |
| Alpha slope | α | 0.0625, 0.6875, 1.2500, 2.0, 3.0, 4.0 |
| AGN: Stalevski et al. (2012, 2016) | ||
| inclination, i.e., viewing angle | AGNPSY [deg] | 0, 10, 20, 40, 70, 90 |
| Contribution of the AGN to the total LIR | AGNFRAC | 0, 0.01, 0.1, 0.3, 0.5, 0.7, 0.9 |
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