Same as Fig. 3, but comparing our SHMR with others that are representative of studies based on different techniques: abundance matching (Rodríguez-Puebla et al. 2015), weak lensing (Mandelbaum et al. 2016), satellite kinematics (More et al. 2011), and a combination of thereof (Dutton et al. 2010). Blue colour is used for late types, red colour is used for early types. The insets show the comparison to the estimates of f_⋆ for late-type galaxies by Lapi et al. (2018). We omit the errorbars here for clarity.