Total stellar-to-halo mass relation (top panel) and total M_*/M_h (bottom panel) at 0.2 <  z <  0.5 compared to hydrodynamical simulations. The purple dashed and dotted lines show our central and satellite contribution to the total SHMR respectively, with the shaded region showing 1σ confidence interval of the sum of the two. The break in solid purple lines and shaded regions indicate the highest stellar mass probed in our analysis, which we take to be the highest mass bin in the SMF. The transparent purple lines and hatched region is an extrapolation at higher masses. We overplot the SHMRs measured in the hydrodynamical simulations HORIZON-AGN in teal, TNG100 in red, and EAGLE in dark yellow, where the dashed dotted and solid lines show the central, satellite, and total SHMR.