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Fig. 4.


Best-fit, line-of-sight velocity dispersion profiles for model 1 (gNFW with free T outer anisotropy with TAND) for sigv-stacked pseudo-cluster. The symbols are the data (150 galaxies per radial bin) as in Fig. 2, while the curves and shaded regions respectively show the median predictions of model 1 and their MCMC uncertainties. The vertical gray-shaded region represents r200 and its MCMC uncertainty.

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