Left: evolution of the peak of the SHMR (for our reference case) compared with previous literature works and results of SAMs of galaxy formation and evolution. Dark blue points and error bars represent the fit of our measured SHMR. The model we propose is shown in green, along with 1 and 2σ errors estimated on the posterior distribution of the free parameters of the fit. Right: comparison of the evolution of the halo mass at the peak of the SHMR (for our reference case). Symbols are the same as in the other panel.