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Fig. 4


Observed mass functions and corresponding Schechter function fits for galaxies at different clustercentric distances (R/R200 ≤ 1 and R/R200 > 1) for the ICBS survey (left panel) and EDisCS (right panel). Black crosses and solid lines represent cluster regions, and red empty stars and dotted lines the cluster outskirts. Mass function normalisations, errorbars, labels and in-sets are as in Fig. 2. In both panels, no statistical differences are detected between the mass functions of galaxies located at different clustercentric distances.

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