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Table B.1.

CIGALE modules and input parameters used for all the fits. BC03 means Bruzual & Charlot (2003), and the Chabrier IMF refers to Chabrier (2003).

Parameters Symbol Range (Ph. 2, DL2014) Range (Ph. 2, PL+OT_MBB)
Target sample Individual Hi-z LBGs Individual Hi-z LBGs

Delayed SFH and recent burst

e-folding time scale of the delayed SFH τmain [Myr] 500 500

Age of the main population Agemain[Myr] 101 log values in [2 - 1200] 101 log values in [2 - 1200]

Burst fburst No burst No burst

SSP

SSP BC03 BC03

Initial mass function IMF Chabrier Chabrier

Metallicity Z 0.004 0.004

Nebular emission

Ionization parameter logU -2.5, -2.0, -1.5 -2.5, -2.0, -1.5
Line width [km/s] 100 100


Dust attenuation law

Color excess for both the old and young stellar populations E_BV_lines 101 log values in [0.01, 1.0] 101 log values in [0.01, 1.0]

Bump amplitude uv_bump_amplitude 0.0 0.0

Power law slope power law_slope 0.0 0.0

Dust emission (DL2014)

Mass fraction of PAH qPAH 0.47

Minimum radiation field Umin 17.0

Power law slope dU/dM ≈ Uα α 2.4

Dust fraction in PDRs γ 0.54

Dust emission (PL + OT_MBB)

Dust temperature Tdust 54.1

Emissivity βRJ 0.87

Slope of the MIR power law αMIR 2.0

No AGN emission

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