CMFs used in the (sub-) halo abundance matching in different redshift bins. On the left, solid and dashed lines with shaded area represent the SMF with 1σ uncertainty (best fit to 1/V_max points; with the exception of the redshift bin 0.0 <  z <  0.2, the best fits have been corrected for the Eddington bias) cumulated as described in Sect. 4.1. Solid lines represent the SMF up to the last 1/V_max point, and dashed lines show this at higher masses. On the right, the solid lines are the Despali et al. (2016) CMFs we used to evaluate the SHMR.