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Fig. 6.


Radial profiles of mass over number density ratios from MAMPOSSt for model 24 (NFW mass profile, top), and model 21 (gNFW mass profile, bottom), for E (red), S0 (green), and S (blue) galaxies, for sigv-stacked pseudo-cluster. The normalization is explained in Eqs. (24)–(26). The horizontal lines are shown to highlight how well mass follows number.

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