Cluster data, which were already given in Table 3, with the predictions from a simple quenching model based on Peng et al. (2010) in its most basic form, using UltraVISTA as a starting point. Mass quenching and environmental quenching are assumed to act independently. The blue Schechter function is the best fit to the star-forming galaxy population and the red solid line gives the best fit to the quiescent population. The red line is composed of a mass quenched population (dotted red line), and an environmentally quenched population (dashed line). This model needs 45% additional environmental quenching compared to the field to yield the best fit to the data. Note that the red points have been offset by 0.01 dex for better visibility.