SHMR for each of the redshift bins in this work. This was obtained by doing abundance matching using the best-fit functional forms of the SMF and the HMF by Watson et al. (2013). The top panel shows stellar mass as a function of the inferred halo mass, while the bottom panel shows the ratio between the two as a function of halo mass. The right axis indicates the SFE, ${ϵ}_{\star }=M_{\star }{M}_{\mathrm{h}}^{-1}{f}_b^{-1}$, and the shaded gray region marks ϵ_⋆ ≥ 100%. The lines and their confidence intervals are shown only in the M_⋆ range probed by our SMF measurements.