Fig. 13.
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Average weak-lensing mass bias as a function of the cluster halo mass M200 for different lens redshifts. We consider all clusters with M200 > 1014 M⊙, which is above the minimum mass expected to be selected in the photometric catalogue (Sartoris et al. 2016), and which are relatively constant with redshift. The right and top subpanels are the same as in Fig. 6.
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