Figure 6 from Dark Matter Halo Profiles of Massive Clusters: Theory versus Observations

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Dark Matter Halo Profiles of Massive Clusters: Theory versus Observations

Authors: Suman Bhattacharya, Salman Habib, Katrin Heitmann, and Alexey Vikhlinin

Bhattacharya et al. 2013 The Astrophysical Journal 766 32.

Provider: AAS Journals

Caption: Figure 6.

c ₂₀₀– M ₂₀₀ distribution at z = 0 (full sample) when wCDM parameters are varied, following the characterization of Figure 4. The scatter is larger at high masses due to lower numbers of halos in high-mass bins.

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