Open Access
Table A.1.
CIGALE parameters used for the SED fitting.
| Parameter | Values | Description |
|---|---|---|
| SFH (sfhdelayed) | ||
| τmainagemainτburstageburstfburst | 1.0, 2.0, 5.0, 7.0 [Gyr]1.0, 3.0, 5.0, 8.0, 11.0, 12.0 [Gyr]10.0 [Gyr]0.001, 0.01, 0.1, 0.3 [Gyr]0.0, 0.15, 0.30 | e-folding time of the main stellar populationAge of the main stellar population in the galaxye-folding time of the late starburst populationAge of the late burstMass fraction of the late burst population |
| Stellar component (bc03) | ||
| IMFZSeparation age | 10.0210 [Myr] | Initial mass function: 1 (Chabrier 2003)MetallicityAge of the separation betweenthe young and the old star populations |
| Dust attenuation | ||
| (dustatt_modified_cf00) | ||
 slope ISMslope BC |
0.3, 1.7, 2.8, 3.30.3, 0.5, 0.8, 1.0-0.7-0.7 | V-band attenuation in the interstellar mediumRatio of the BC-to-ISM attenuationPower law slope of the attenuation in the ISMPower law slope of the attenuation in the BC |
| Dust emission (dl2014) | ||
| qPAHUminαγ | 0.47, 2.5, 3.90.1, 1.0 5.0, 10.0, 25.0, 40.01.0, 2.0, 3.00.0, 0.02 | Mass fraction of PAHMinimum radiation fieldDust emission power law slopeIlluminated fraction |
| AGN component (fritz2006) | ||
| rratioτβγOpening angleΨfAGN | 60.00.6, 1.0, 3.0-0.50.0100.00.001, 30.100, 89.990.0, 0.1, 0.15, 0.25, 0.50 | Ratio of the maximum to minimum radii of the dusty torusEquatorial optical depth at 9.7 μm Radial dust distribution within the torusAngular dust distribution within the torusFull opening angle of the dusty torusAngle between equatorial axis and line of sightAGN fraction |
Notes: The first column reports the name of the templates as well as each individual parameter. In the second column the parameters are reported, and in the third column the descriptions of the parameters are given.
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