Best fit Schechter models corresponding to maximum likelihood for the total, star-forming, and quiescent samples (solid colored curves) based on the observed data (colored points). Fits for the median posterior will be similar for symmetric parameter posterior distributions, which are found in all but the last bin shown here. Kernel convolved fits are shown by the dashed curves. Fits measured using the continuity model are shown in gray solid curves. Lower panels indicate the fraction of quiescent galaxies ℱ_QG ≡ Φ_QG/(Φ_SF + Φ_QG) as a function of log₁₀(ℳ/ℳ_⊙) for the data (colored points) and maximum likelihood fits (solid curve). Since the star-forming and quiescent fits are not required to sum to the total fit, changing the definition to ℱ_QG ≡ Φ_QG/Φ_Total as reported by Ilbert et al. (2013) and Davidzon et al. (2017) produces the dotted curves with noticeably lower ℱ_QG at high ℳ.