Luminosity profile as a function of projected radius (left) and sSFR as a function of stellar mass (right) for the galaxies in our samples. The thick lines indicate the median of each sample, and shaded regions are the error on the median calculated from 500 bootstrap resampling of the data. We use the same method to calculate errors through the entire paper. Our kinematics-based selection criteria reproduce the expected traits from the different morphologies, such as quiescence and steep luminosity profiles in spheroid-dominated objects versus active star formation and shallower luminosity profiles in disc-dominated samples.