Fig. 4.
Panel a: stellar mass distribution of the cluster members with the completeness limit indicated by the red, dashed line. Panel b: completeness of our data set with respect to K-band luminosity. The red dashed line is at K = K⋆+2.0- the magnitude limit of ACReS survey. Panel c: completeness distribution on the sky. The green circle has a radius equal to R200 of the cluster.
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