Fig. 6.

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Predicted entropy profiles for a halo mass of 1013 M⊙ (blue), 1014 M⊙ (red) and 1015 M⊙ (black) respectively, compared with the observed mean entropy profile and intrinsic scatter (orange shaded region) from the REXCESS sample of galaxy clusters, (Pratt et al. 2010), which features a median mass of M500 ∼ 2.5 × 1014 M⊙. To ease comparison with observational data, the predicted entropy has been rescaled by K500 and radius by R500.
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