Normalised histograms of the galaxy properties of our multi-wavelength sub-samples after selection cuts. Histograms show the inclination-corrected values for r_1∕2, n (derived from single Sérsic profile fits to rest-frame g-band light profiles), and log(M_*). The y-axis shows the fraction of galaxies (in that subsample) in each bin. Radio-detected galaxies have a distribution of optical axis-ratios skewed towards edge-on galaxies.