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Table 1.

CIGALE grid parameter values adopted for the modelling described.

Parameter Values Description
Star formation history (SFH): Delayed
τmain 5–8000 (in steps of 10) e-folding time of the main stellar population model (Myr).
Age 200–13 260 (in steps of 10) Age of the oldest stars in the galaxy (Myr).

Single-age stellar population (SSP): Bruzual & Charlot (2003)
imf 1 Initial mass function Chabrier (2003)
Metallicity 0.02 solar
Separation Age 10 Age of the separation (to differentiate) between the young and the old star populations (Myr).

Dust attenuation: Calzetti et al. (2000)
E(B − V)young 0.015, 0.02, 0.04, 0.06, 0.1, 0.2, 0.3, 0.9, 1.0 Color excess of the stellar continuum light for the young population.

Dust emission: dl2014
Qpah 1.12, 1.77, 2.50, 3.19 Mass fraction of PAH
Umin 5.0, 6.0, 7.0, 8.0, 10.0, 12.0, 15.0, 17.0, 20.0, 25.0 Minimum radiation field
Alpha 2.0, 2.1, 2.2, 2.3, 2.4, 2.5, 2.6, 2.7, 2.8 the power-law distribution (dMd ∝ UαdU)
Gamma 0.02 Fraction illuminated from Umin to Umax

AGN model: Fritz et al. (2006)
Rmax/Rmin 30.0, 60.0, 100.0, 150.0 Ratio of the maximum to minimum radii of the dust torus.
τ 0.3, 0.6, 1.0, 2.0, 3.0, 6.0, 10.0 Optical depth at 9.7 μm.
β −1.00, −0.75, −0.50, −0.25, 0.00 Beta from the power-law density distribution for the radial component of the dust torus (Eq. (3) of Fritz 2006).
γ 0.0, 2.0, 4.0, 6.0 Gamma from the power-law density distribution for the polar component of the dust torus (Eq. (3) of Fritz et al. 2006).
Opening angle (θ) 60.0, 100.0, 140.0 Full opening angle of the dust torus (Fig. 1 of Fritz et al. 2006).
ψ 0.001, 10.1, 20.1, 30.1, 70.1, 89.990 Angle between equatorial axis and line of sight.
fAGN 0.0, 0.05, 0.1, 0.15, 0.2, 0.25, 0.3, 0.35, 0.4, 0.45, 0.5, 0.55, 0.6, 0.65, 0.7, 0.75, 0.8, 0.85, 0.9, 0.95, 0.99 Fraction of AGN torus contribution to the IR luminosity (fracAGN in Eq. (1) of Ciesla et al. 2015)

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