Radiative and mechanical energies in galaxies - I. Contributions of molecular shocks and PDRs in 3C 326 N

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Table C.2.

CIGALE modules and input parameters

Parameter	Symbol	Value
Delayed Star Formation History
e-folding time of main stellar population (Myr)	τ_main	250, 500, 1000, 2000, 4000, 6000, 8000, 10000, 12000, 15000
age of main stellar population (Myr)	age_main	250, 500, 1000, 2000, 4000, 8000, 10000, 12000

Stellar Populations; Bruzual & Charlot (2003)
initial mass function	IMF	Chabrier (2003)
metallicity	Z	0.008

Dust attenuation. Values adopted by Charlot & Fall (2000)
ISM attenuation in the V-band (mag)	$A_{V}^{ISM}$ $\rm{A}_\mathrm{V}^\mathrm{ISM}$	0.05, 0.1, 0.2, 0.3, 0.4, 0.5, 0.6
$A_{V}^{ISM} / (A_{V}^{ISM} {+A}_{V}^{BC})$ $\rm{A}^{\mathrm{ISM}}_\mathrm{V}/(\rm{A}^{\mathrm{ISM}}_\mathrm{V}+\rm{A}^{\mathrm{BC}}_\mathrm{V})$	μ	0.44
Dust Emission; Draine et al. (2014)
mass fraction of PAH	qPAH	1.12, 2.5, 3.19, 4.58, 5.95
minimum radiation field	U_min	5.0, 10.0, 25.0
power-law slope dU/dM ∝ U^α	α	2.0
fraction illuminated from U_min to U_max	γ	0, 0.02

AGN (UV-to-IR) SKIRTOR; Stalevski et al. (2016)
AGN contribution to IR luminosity	f_AGN	0.05, 0.1, 0.2, 0.3
Viewing angle (deg)	θ	60, 70, 80, 90
Polar-dust color excess (mag)	E(B−V)_PD	0, 0.2, 0.4

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