Comparison of the SFR distributions for our final sample of galaxies (black) and our parent sample (orange), separated by depth of the field (SF, MF, and DF; see MUSCATEL description in Sec. 2.1). The blue line shows the fraction of galaxies from the parent sample in our final sample, in each SFR bin. The right-side y-axis indicates the fraction shown by the blue line. In the top-left corner of each panel is indicated the field depth, and the number of galaxies in the final/parent sample.