Fig. 8
Parameter likelihoods for different DM density distributions in the case of B07 stellar masses. The virial mass corresponding to each parameter combination is shown in colour coding; 90 × 1010 M⊙, 110 × 1010 M⊙, and 130 × 1010 M⊙ levels are indicated with solid contours. For the Einasto, NFW, and Moore DM profile, the virial mass is almost the same.
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