Fig. 8
Maximum likelihood best-fit of a projected NFW model (Bartelmann 1996; Navarro et al. 1997) to the distribution of radial distances of the cluster members in the virial region and the binned number density profile with 1σ error bars. Only galaxies with zPetro ≤ 19.64 and in regions of spectroscopic completeness >1/4 have been considered, and the sample has been corrected for incompleteness.
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