Table E.2.

Parameters of the models used in this paper, symbol used, their assumed ranges and summary of other information about the models. The Fritz et al. (2006) model assumes two additional parameters that define the density distribution in the radial direction (β) and azimuthal direction (γ). In this paper we assume β = 0 and γ = 4. The SKIRTOR model (Stalevski et al. 2012) assumes two additional parameters that define the density distribution in the radial direction (p) and azimuthal direction (q). In this paper we assume p = 1 and q = 1. In addition, the SKIRTOR library we used assumes the fraction of mass inside clumps is 97%. There are 4 additional scaling parameters for the starburst, spheroidal, AGN and polar dust models, f_SB, f_s, f_AGN and f_p, respectively.

Parameter	Symbol	Range	Comments
CYGNUS Starburst
Initial optical depth of giant molecular clouds	τV	50-250	Bruzual & Charlot (1993, 2003)
Starburst star formation rate e-folding time	τ*	10-30Myr	Efstathiou et al. (2000), Efstathiou & Siebenmorgen (2009)
Starburst age	t*	5-35Myr	metallicity=solar
CYGNUS Spheroidal Host
Spheroidal star formation rate e-folding time	τs	0.125-8Gyr	Bruzual & Charlot (1993, 2003)
Starlight intensity	ψs	1-17	Efstathiou & Rowan-Robinson (2003), Efstathiou et al. (2021)
Optical depth		0.1-15	metallicity = 40% of solar
CYGNUS AGN torus
Torus equatorial UV optical depth	τUV	250-1450	Smooth Tapered disks
Torus ratio of outer to inner radius	r2/r1	20-100	Efstathiou & Rowan-Robinson (1995), Efstathiou et al. (2013)
Torus half-opening angle	θo	30-75°	Standard galactic dust mixture
Torus inclination	θi	0-90°
Fritz AGN torus
Torus equatorial optical depth at 9.7μm		0.1-10	Smooth Flared disks
Torus ratio of outer to inner radius		10-30	Fritz et al. (2006)
Torus half-opening angle		20-70°	Standard galactic dust mixture
Torus inclination		0-90°
SKIRTOR AGN torus
Torus equatorial optical depth at 9.7μm		3-11	Two-phase flared disks
Torus ratio of outer to inner radius		10-30	Stalevski et al. (2012), Stalevski et al. (2016)
Torus half-opening angle		20-70°	Standard galactic dust mixture
Torus inclination		0-90°