Best-fit models for clustering and abundance compared with measurements at 0.5 <  z <  0.8. Top: clustering measurements for the 6 mass threshold-selected samples (empty circles with errorbars) along with the best-fit models in solid lines in corresponding colors. Bottom: measurements of the stellar mass function together with the best fit model. The dashed lines show the SMF in the same redshift bin obtained by Davidzon et al. (2017) for comparison.