Fig. 10.

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Distributions of the main global properties of our primary galaxy sample. The properties presented here are the stellar mass (M⋆), the average SFR over the last 100 Myrs (SFR100 Myrs), the specific SFR100 Myrs (sSFR100 Myrs), the mass-weighted stellar age (t⋆, mw), the light-weighted stellar age (t⋆, lw) weighted by the bolometric luminosity, the stellar metallicity (Z⋆), the dust attenuation slope index (n), the dust opacity of the birth-clouds () and diffuse dust component (
) in the V band, and the PAH mass fraction (qPAH). The KDE distribution is shown in red, while the solid black line shows the median value. The black dotted and dashed lines indicate the 16th and 84th percentiles of each distribution, respectively.
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