Figure 3 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 3.

c– M distribution at a mass bin centered at 1.5 × 10 ¹⁴ h ⁻¹ M _☉ using results from the HACC simulation at z = 0. The lines show a Gaussian distribution with standard deviation σ _c/ c ~ 0.33.

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