Comparison of the properties estimated using different techniques of the galaxies in the W4 selection of sample 𝒫. (a) WISE and ProSpect estimates of stellar mass plotted against the GAMA stellar masses. (b) WISE and ProSpect estimates of SFR plotted against the GAMA SFRs. (c) SFR_GAMA–SFR22_WISE distribution colour-coded with S/N values. (d) SFR_GAMA–SFR22_WISE distribution colour-coded with redshift. (e) SFR_GAMA–SFR12_WISE distribution colour-coded with S/N values. (f) SFR_GAMA–SFR12_WISE distribution colour-coded with redshift. The solid coloured lines in panels (a) and (b) show the corresponding linear fit function of the population, as labelled. The dashed black lines in all the panels show the 1:1 correlation line.