SHMR in the form of the ratio f_⋆ ≡ M_⋆/f_bM_h as a function of stellar mass (left) and halo mass (right) for the sample of spiral galaxies in SPARC (blue diamonds, PFM19) and for the sample of ellipticals and lenticulars in SLUGGS (red circles, this work). The halo masses of late types are estimated from HI rotation curves, those of early types from the kinematics of the GC system. For comparison, we show also the abundance matching SHMR from Moster et al. (2013, grey band).