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Fig. 9.

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Representation of the models p(Imain|LX, z, NH, Texp, bkg) and p(Icosmo|LX, z, NH, Texp, bkg) for fixed values of cluster redshift z, two different values for the luminosity LX, and local galactic absorption NH, in addition to a nominal background level and a range of exposure times Texp (along the x-axis). The shaded regions indicate the approximate 68% confidence range output of the model.

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