Figure 8 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 8.

Ratio of observed concentration to theoretical predictions for the XMM-Newton cluster observations of Ettori et al. (2011). The shaded area represents the 1σ boundary for the theoretical predictions. Each data point actually represents observations of multiple clusters.

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