Comparison of the main global properties of our primary galaxy sample as retrieved from three different SED fitting runs. The properties presented here are the stellar mass (M_⋆), the average specific SFR over the last 100 Myrs (sSFR_100 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 opacity of the diffuse dust component (${\widehat{\tau }}_{\mathrm{dust},2}$) in the V band, and the dust attenuation slope index (n). We compare the distributions of our fiducial run with those from the spectroscopy-only (top row), and photometry-only (bottom row) run. Contours enclose 20%, 50% and 80% of the total data. The dashed orange line shows the one-to-one relation.