Fig. 8.
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Typical SB X-ray flux versus 1.4 GHz flux at different redshifts computed for an AGN with log Lbol = 43 (upper panel) and log Lbol = 46 (lower panel). Error bars show the 1σ distribution values due to the scatter in the Lbol − LHX relation (vertical error bar), and in the L1.4 GHz−LHX relation (horizontal error bar). The dashed lines indicate the redshift at which the fluxes are computed.
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