Distributions of the physical properties estimated for our candidate QGs from the SED fitting with CIGALE. Clockwise, from the top left to the bottom right: goodness of fit expressed as reduced χ²; galaxy redshift; stellar mass; SFR; dust mass; and the linear offset of the galaxy’s observed SFR from the SFR expected from the modelled MS (Δ_MS in log scale) as a function of redshift. To guide the eye, we also plot a dashed red line that marks the value that is four times lower than the MS.