Top panel: cluster data points for the different galaxy types within R500. The curves show a basic quenching model inspired by the formalism presented in Peng et al. (2010), with the UltraVISTA SMF in the redshift range 0.5 < z < 0.7 g point. Bottom panel: difference between the data (total distribution of quenched galaxies) in the cluster compared to the prediction from the model. This suggests a relative removal/destruction of low-mass galaxies and the expected build-up of BCGs.
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