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Table 2.

Parameter grid adopted for the CIGALE SED modeling from UV to decameter ranges.

Star formation history: sfhdelayedbq
τmain [Myr] 1000, 2000, 4000
agemain [Myr] 7000
agebq [Myr] 500, 1000
rSFR 1.25, 1.5, 3.0
Stellar population synthesis: bc03
IMF Chabrier (1)
Metallicity Z 0.02
Separation age [Myr] 1000
Nebular emission: nebular
log U −2.5, −3.0
Gas metallicity Zgas 0.02
Dust attenuation: dustatt_modified_starburst
E(B − V)lines 0.5
E(B − V)factor 0.44
UV bump wavelength [nm] 217.5
UV bump width [nm] 35.0
UV bump amplitude 3.0
Power-law slope δ −0.4, −0.20
Dust emission: dl2014
qPAH [%] 3.19, 4.58, 5.95
Umin 1, 2, 3, 5
α 2.0, 2.1, 2.2, 2.4
γ 0.01, 0.05
Radio emission: radio_extra
FIR/radio q (SF only), qIR, SF 2.3, 2.6, 2.9
SF synch. slope, αsf 0.9
LF amp. νbreak (×SF), ALF 1.4, 1.6, 2.0
LF slope, αLF 1.5
HF slope (extra), αSF 1.0, 1.2
Break freq. (MHz), νbreak 57
FF optical depth νff, τff 1.0, 3.0, 5.0
FF pivot freq. (MHz), νff 100
FF opacity slope, βff 2.1, 2.3, 2.5

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