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Fig. 5


X-ray luminosity as a function of the spectroscopic temperature for observations (red squares) and simulations. Arrows indicate the change of the cluster properties starting from the case without the AGN (open circles) to with the AGN (filled circles). The shaded area shows the 1σ uncertainty of the best-fit REXCESS LxT scaling relation, which was derived for clusters above 2 keV.

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