Fig. 4.
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Contours of AC detection probability as a function of the total count rate (CR) in the 0.5–2 keV band and the input core radius (rc) from the β model. An exposure time of 10 ks was used along with nominal background value of b = 1. The flux ratio chosen was 0.5, i.e. half the count rate of the cluster is contained within the central AGN.
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