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Fig. 9

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The galaxy stellar mass function in the central region of XMMU J2235, as derived from the Ks-band LF (solid symbols). Empty black circles show the stellar mass function derived from individual SED-estimated stellar masses of spectroscopic and photo-z retained members (see text for details). Gray symbols show previous determinations (Kodama & Bower 2003; Strazzullo et al. 2006) at z ~ 1 (squares) and z ~ 1.2 (circles). All mass functions are arbitrarily rescaled. The dotted line shows the mass completeness limit as estimated from the Ks image 10σ completeness.

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