Input parameters for CIGALE.
|Pop. synth. mod.||Bruzual & Charlot (2003)|
|Dust model||Draine & Li (2007)|
|Age||1–301, step 2||Myr|
|UV bump amplitude||0, 1.5, 3|
|QPAH||0.47, 3.90, 7.32|
|Umin||0.1, 1.0, 5.0, 10.0|
|α||1.5, 2.0, 2.5|
|γ||0.01, 0.3, 1.0|
Notes. Line 1: population synthesis model. Line 2: dust model. Line 3: IMF. Line 4: stellar metallicity. Line 5: age interval andsampling. Line 6: extinction law (Calzetti et al. 2000). Line 7: attenuation. Line 8: amplitude of the UV bump (Noll et al. 2009). Line 9: mass fraction of the dust composed of PAH particles containing <103 atoms (Draine & Li 2007). Line 10: diffuse interstellar radiation field (Draine & Li 2007). Line 11: power-law index of the interstellar radiation field (Draine & Li 2007). Line 12: fraction of the dust mass that is close to OB associations and is exposed to a stellar radiation field with intensity U > Umin (Draine & Li 2007).
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