Fig. 4
CR-to-thermal pressure ratio, XCR = ⟨PCR⟩/⟨Pth⟩ at the radial distance from the Perseus cluster center, R/Rvir (red lines), and integrated up to R/Rvir (blue lines), using the simulation-based analytical model of CRs (Pinzke & Pfrommer 2010). The simulation model (dashed) is contrasted to a model that has been scaled by the MAGIC constraints obtained in this work (solid).
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