Open Access
Table 1.
Input parameters for CIGALE SED fitting.
| Model and input parameters | Values |
|---|---|
| Star formation history: sfhdelayedbq (Ciesla et al. 2017) | |
| e-folding time of the main stellar population model (Myr) | 500, [1000, 10 000] with a spacing of 1000 |
| Age of the main stellar population in the galaxy (Myr) | [10 000, 13 000] with a spacing of 500 |
| Age of the burst/quench episode (Myr) | 100, 200, 400, 600, 800, 1000 |
| Ratio of the SFR after and before the burst/quench (Myr) | 0, 0.2, 0.4, 0.6, 0.8, 1, 1.2, 1.4, 1.6, 1.8, 2 |
| Stellar population: bc03 (Bruzual & Charlot 2003) | |
| Initial mass function | Chabrier (2003) |
| Metallicity | 0.008 |
| Dust attenuation: dustatt_modified_starburst | |
| (Calzetti et al. 2000; Leitherer et al. 2002) | |
| E(B − V)lines, the color excess of the nebular lines (mag) | 0, [0.001, 2] log sampled with 40 values |
| Reduction factor to compute E(B − V)continuum | 0.44 |
| Amplitude of the UV bump | 0.0 |
| Slope delta of the power law modifying the attenuation curve | 0.0 |
| Extinction law for attenuating emission lines flux | Milky Way (Cardelli et al. 1989) |
| RV | 3.1 |
| Dust emission: dale2014 (Dale et al. 2014) | |
| AGN fraction | 0.0 |
| Slope of the interstellar radiation field (α) | 2.0 |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.