Fig. 3

Radial profile of the stellar-to-total matter ratio of MACSJ1206 (left), MACSJ0329 (center), and RXJ1347 (right). The upper panels only consider red sequence galaxies, whereas lower panels consider red galaxies and BCGs. The multi-step function and the shading indicate soundly derived values (posterior mean) and 68 % errors (highest posterior interval), whereas points and error bars are approximate (see text).
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