Morphology-stellar mass classification for a LSST-like survey including both type-1 and type-2 galaxies. Blue dotted lines correspond to galaxies with a relatively small bulge, red dashed to those with a large bulge. The different symbols distinguish different stellar mass bins. The range where we assume the measurement has a bias below 10% is highlighted (derived using our results from the type-1 only profiles). The classification ranges are described in the top table in Fig. 17. The black solid line is the measurement for the host cluster shown for visual reference.