Fig. A.6
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Comparison of fX (left panel), IIN (middle panel), and Γ (right panel) measurements for sources within the C4 catalogue, where the zpltb model is utilised for spectral fitting (i.e., AGNs), with corresponding measurements from C2, employing a power-law model for spectral fitting. Each panel displays the mean, median difference, and scatter. Sources included in the Good-fit samples are presented.
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