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Table 1
Galaxy and AGN parameters adopted to generate mock galaxy SEDs.
| Parameter | Value | Description |
|
|
||
| Dust attenuation | ||
| E(B − V)∗ | 0.2 | |
|
|
||
| Dust template: Draine & Li (2007) | ||
| qPAH(%) | 3.19 | Mass fraction of PAH to the total dust mass. |
| Umin | 8.0 | Min. intensity of the interstellar radiation field. |
| Umax | 106 | Max. intensity of the interstellar radiation field. |
| γ(%) | 2 | Relative contribution between dust heated in photodissociation. |
| regions, and dust heated by diffuse stellar population. | ||
|
|
||
| AGN emission | ||
| Rmax/Rmin | 60 | Ratio between outer and inner radius of the torus. |
| τ9.7 | 1.0 (for int. type) | Optical depth at 9.7 μm. |
| 6.0 (for Type-1 and Type-2) | ||
| β | –0.5 | Linked to the radial dust distribution in the torus. |
| γ | 0.0 | Linked to the angular dust distribution in the torus. |
| ψ | 0.001 (for int. type and Type-2) | Angle with line of sight. |
| 89.9 (for Type-1) | ||
| θ | 100 | Angular opening angle of the torus. |
| fracAGN | 0., 0.05, 0.1, 0.15, 0.2, 0.25, 0.3, | Contribution of the AGN to the total LIR. |
| 0.35, 0.4, 0.45, 0.5, 0.55, 0.6, 0.7 | ||
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