Residuals of our dynamical estimates of f_⋆ relative to the abundance-matching values f_⋆,  AM at the same stellar masses from Moster et al. (2013) versus the disc-to-total ratio D/T (left) and Hubble type T (right), for massive late types (M_⋆ > 5 × 10¹⁰ M_⊙, blue diamonds) and early types (red circles). The grey area shows the scatter of the Moster et al. (2013) SHMR near M_⋆ ∼ 10¹¹ M_⊙. Several early types pile up at D/T = 0 since no disc component could be clearly identified from their photometry.