Fig. A.4.
Difference of the AGN fraction values estimated by fitting the mock catalogue from the true values. We present the results when the X-ray flux has been included in the SED (shaded histograms) and without including the X-ray flux (green histograms). The results are split into X-ray luminosity bins. X-CIGALE can successfully recover the AGN fractions, regardless of whether the X-ray flux is included in the SED fitting or not, at all X-ray luminosities.
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