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Table 1
Input parameters of the code CIGALE.
| Paramater | Values |
|
|
|
| Star formation history | |
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|
|
| τ e-folding time of the main stellar population model [Myr] | 6000, 4000, 3000 |
| τ e-folding time of the late starburst population model [Myr] | 35, 30, 25, 15, 10, 8 |
| Mass fraction of the late burst population | 0.3, 0.2, 0.1, 0.001 |
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|
|
| Single stellar population | |
|
|
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| Initial mass function | Salpeter (1955) |
| Metallicities (solar metallicity) | 0.2 |
| Age of the separation between the young and the old star population [Myr] | 10 |
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|
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| Attenuation curve | |
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| Slope correction of the Calzetti law | 0.0 |
| Color excess of the stellar continuum light for the yought stellar population | 0.15, 0.3, 0.5 |
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| Dust emission | |
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| IR power-law slope | 0.0625, 0.5, 0.9375, 1.3125, 1.75, 2.0, 2.1250, 2.1875, 2.3750, 2.75, 3.1875, 3.7500 |
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| AGN emission | |
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| Ratio of the maximum to minimum radius of the dust torus | 60 |
| Optical depth at 9.7 microns | 1.0, 6.0 |
| Radial dust distribution in the torus | −0.5 |
| Angular dust distribution in the torus | 0.0 |
| Angular opening angle of the torus [deg] | 100.0 |
| Angle between equatorial axis and the line of sight [deg] | 0.001, 89.900 |
| Fractional contribution of AGN | 0.01, 0.15, 0.25, 0.3, 0.35, 0.4, 0.45,0.55 |
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