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Fig. 3

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Dependence of the observed fraction of CC objects, cobs, on the 0.1–2.4 keV luminosity (left) and the redshift (right). In both cases, the black or blue data show the simulation results for case I or case II, respectively (see text). The dashed red lines show the input fraction of CC objects, cinp, which was fixed to 0.38 for the simulations.

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