Fig. 9.
Histograms of the W1 magnitudes for the morphologically classified possible cluster members within a cluster-centric distance R = 100′ (black), the sub-sample of spectroscopically confirmed cluster members (blue), and the sub-sample of galaxies without spectroscopic redshifts (red). The two dashed vertical lines indicate the magnitude limits for MLS_W1b and MLS_W1.
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