Similar to Fig. 4, but changing the reference tracer choice by (from left to right, top to bottom) the spectroscopic lsSFR, the host galaxy morphology, the global host galaxy stellar mass, the local u − r color, the photometric lsSFR, and the local stellar mass. In this figure the α and β have been fixed to that of the reference tracer used in each subplot (see Sect. 6.1). The gray band around the black line is the expected scatter along the diagonal (see Sect. 6.2). The more the data deviate from the model expectation (black line), the less likely it is for the reference tracer to be closely connected to the actual underlying astrophysical origin.