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Table 1.
Parameters adopted for the SED fitting using CIGALE.
| Parameter | Description | Value |
|---|---|---|
| SFH - Delayed Model | ||
| Age_main | Stellar age | 200, 500, 700, 1000, 2000 |
| 3000, 4000, 5000 Myr | ||
| τ_main | e-folding time of the stellar population | 1500, 2000, 3000, 4000, 5000, |
| 7000, 10 000, 12 000 Myr | ||
| Age_burst, τ_burst | Age and e-folding time of the late burst | 10 000 Myr, 50 Myr |
| F_burst | Mass fraction of the late burst population | 0.0, 0.005, 0.01, 0.015, 0.02, 0.05, |
| 0.10, 0.15, 0.18, 0.20 | ||
| Stellar emission Bruzual & Charlot (2003) | ||
| IMF | Initial mass function | Chabrier |
| Z | Abundance | 0.02 |
| Dust attenuation Charlot & Fall (2000) | ||
| Av_ISM | V band extinction in the ISM | 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9, 1.0, |
| 1.5, 2.0, 2.5, 3.0, 3.5, 4.0 | ||
| Nebular emission | ||
| log U | Logarithm of the Ionization parameter | −2.0 |
| Line_width | Width of the line in km s−1 | 300.0 |
| Dust Dale et al. (2014) | ||
| α | Power law index of the sum of the dust templates | 2.0 |
| frac_AGN | AGN fraction | 0.0 |
| AGN module skirtor2016: Stalevski et al. (2016) | ||
| i | Viewing angle | 30, 70 |
| Delta | Power law index of the optical slope | −0.36 |
| fAGN | AGN fraction | 0.0, 0.1, 0.2, 0.3, 0.4, 0.5, |
| 0.6, 0.7, 0.8, 0.9, 0.99 | ||
| E(B − V) | Extinction in the polar direction | 0.0, 0.2, 0.4 |
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