Table 5.
Input models and main parameters for the CIGALE code.
| sfh_delayed | |
|---|---|
| τ (main) [Myr] | 150, 200, 300, 500, 700, 1000, |
| 1500, 3000, 5000, 10000 | |
| Age (main) [Myr] | 200, 300, 500, 700, 1000, |
| 1500, 3000, 5000, 10000 | |
| bc03 | |
| Initial mass function | Chabrier |
| Metallicity | 0.02 |
| nebular | |
| log10U | −3 |
| Emission | True |
| dustatt_modified_starburst | |
| EBV lines [mag] | 0, 0.5, 1, 1.5, 2, 2.5, 3, 3.5, 4, 4.5 |
| EBV factor | 0.44 |
| RV | 3.1 |
| fritz2006 | |
| rratio | 10, 60, 150 |
| τ | 0.1, 1, 6 |
| β | −0.5 |
| γ | 0, 4 |
| Opening angle [deg] | 60, 100 |
| Disk type | Schartmann et al. (2005) spectrum |
| δ | −0.36 |
| fracAGN | 0, 0.1, 0.25, 0.5 |
| redshifting | |
| Redshift | 0, 1, 2, …, 15 |
Notes. The models used are: a delayed star formation history with optional exponential burst; Bruzual & Charlot (2003) single stellar population; a continuum and line nebular emission model; a modified Calzetti et al. (2000) dust attenuation law; AGN models from Fritz et al. (2006); and a redshifting model that also includes the intergalactic medium from Meiksin (2006).
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