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Table 2.

Model parameters of CIGALE that were used for the SED fitting.

Type Model name Reference Parameters used
Star formation sfhdelayed (Ciesla et al. 2017) age_main = 1000, 2500, 4500, 6000, 8000
history tau_burst = 10000.0
age_burst = 10, 50, 80, 110
f_burst = 0.001, 0.01, 0.03, 0.1, 0.2, 0.3
sfr_A = 10.0,100.0,1000.0,3000.0

Stellar emission bc03 (Bruzual & Charlot 2003) imf = 1(Chabrier)
metallicity = 0.0001,0.02
separation_age = 10

Dust attenuation dustatt_2powerlaws (Charlot & Fall 2000) Av_BC = 0.3, 0.8, 1.2, 1.7, 2.3, 2.8, 3.3, 3.8
slope_BC = −0.7
BC_to_ISM_factor = 0.3, 0.5, 0.8, 1.0
slope_ISM = −0.7
filters = V_B90, FUV

Lyman Continuum lyc_absorption (Inoue 2011) fesc = 0.0,0.5
escape fdust = 0.0,0.5

Dust emission dl2014 (Dale et al. 2014) qpah = 0.47, 1.12, 2.5, 3.9
umin = 5.0, 10.0, 25.0
alpha = 2.0
gamma = 0.02,0.9
AGN fritz2006 (Fritz et al. 2006) r_ratio = 60.0
tau = 1.0,6.0
beta = −0.5
opening_angle = 100.0
psy = 0.001
fracAGNescape = 0.0,0.1,0.2,0.6,0.8

Redshift redshifting (Meiksin 2006) redshift = 0.01–7.5 (or fixed)

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