Open Access

Table A.1.

Input parameters used in SED fitting with CIGALE.

Parameter Values
Delayed star formation history

e-folding time of the main stellar population model (Myr) 100, 300, 500, 1500
Age of the main stellar population 300, 500, 800, 1000, 2500,
in the galaxy (Myr) 3500, 4500, 6000, 7000
e-folding time of the late starburst population model (Myr) 10000
Age of the late burst (Myr) 10
Mass fraction of the late burst population 0
Normalise the SFH to produce one solar mass True

Stellar population synthesis Bruzual & Charlot (2003)

Initial mass function Chabrier (2003)
Metalicity 0.02
Age of the separation between the young and the old star populations (Myr) 10

Dust emission Dale et al. 2014

AGN fraction 0
α slope 2.0

Dust attenuation Charlot & Fall (2000)

V-band attenuation in the interstellar medium 0.0, 0.05, 0.1, 0.2, 0.4, 0.75,
1.0, 1.5, 1.75, 2.0, 2.2, 2.5, 3.0
μ 0.8
Power law slope of the attenuation in the ISM -0.7
Power law slope of the attenuation in the birth clouds -0.7

Dust attenuation Calzetti et al. (2000)

E(B-V)l 0.0,0.05, 0.1, 0.2, 0.3, 0.4, 0.5,
0.6, 0.7, 0.8,0.9, 1.0 ,1.3, 1.5
E_BV factor 0.44
Central wavelength of the UV bump in nm 217.5
Width (FWHM) of the UV bump in nm 35.0
Amplitude of the UV bump 0
Slope delta of the power law modifying the attenuation curve 0
Extinction law to use for attenuating the emission lines flux Milky Way
Ratio A_V / E(B-V) 3.1

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.