Fig. 5.
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Distribution of trace ϵ/σ02 for a few ranges in halo mass (histograms). The dotted curve shows the expected (zero-mean, unit variance Gaussian) distribution at unconstrained positions; the dashed curve, at positions with λ3 ≥ 0 (Eq. 21). More massive haloes have larger ϵ/σ02, but the distribution around the mean is approximately independent of mass.
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