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Fig. 3.


MAMPOSSt marginal distributions (diagonal panels) and covariances for model 24 (non-Einasto model with the strongest BIC evidence) in sigv-stacked pseudo-cluster. The red stars and arrows show the parameters with the highest likelihoods. The priors are flat within the panels and zero outsize, except for the tracer NFW scale radii rE, rS0, and rS, for which the priors are Gaussian distributions with means in the middle and extending to ±3σ on the panel edges.

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