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Table 1. List of the input parameters of CIGALE, based mostly on Buat et al. (2011).

From: Dusty Universe viewed by AKARI far infrared detector

  Symbol Range
Star formation history   
metallicities (solar metalicity) Z 0.2
τ of old stellar population models in Gyr τ 1 1. 3. 10.
ages of old stellar population models in Gyr t1 13
ages of young stellar population models in Gyr t1 0.025 0.05 0.1 0.3 1.0
fraction of young stellar population fySP 0.001 0.01 0.1 0.999
Dust attenuation   
slope correction of the Calzetti law δ −0.3 −0.2 −0.1 0. 0.1 0.2
V-band attenuation for the young stellar population Av,ySP 0.15 0.30 0.45 0.60 0.75 0.90 1.05 1.2 1.35 1.5 1.65 1.8 1.95 2.10
Reduction factor of the dust attenuation at 5500 Å for old stellar population models fatt 0.0 0.5 1.0
Dust emission   
IR power-law slope α SED 0.5 1.0 1.5 1.75 2.0 2.25 2.5 4.0
Ldust fraction of AGN model fAGN 0. 0.1 0.25