Fig. 7.

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Predicted entropy profiles for a halo mass of 1013 M⊙ (blue), 1014 M⊙ (red), and 1015 M⊙ (black). Dashed lines show entropy from gravitational processes only, solid lines include the effects of pre-heating. The mean entropy profile and intrinsic scatter from the REXCESS sample of galaxy clusters, (Pratt et al. 2010), which features a median mass of M500 ∼ 2.5 × 1014 M⊙, is reported as an orange shaded region. The region between the 1014 M⊙ and 1015 M⊙ profiles is shown as a gray shaded region.
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