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Fig. 2

image

Radial profile of the characteristic stellar mass (upper panels), faint-end slope α (central panels) and projected surface stellar mass density (bottom panels) of the three clusters (MACSJ1206, MACSJ0329, and RXJ1347, from left to right). The central-left panel report the fitted linear trend. Arrows indicate rΔ values and are from Merten et al. (2014). The surface stellar mass density Σ is in M/Mpc2 units.

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