Fig. 16
Cumulative number density of the 44 photometric members of XMMU J0338.7 + 0030 as a function of their cluster-centric distances. The mean number density of those members within a concentric, circular annulus delimited by radii of 1′ and 2′ is reproduced together with upper and lower limits (red solid and short-dashed lines, respectively) computed as in Gehrels (1986).
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