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Fig. 3


X-ray luminosity distribution in the 2–10 keV energy band for the FERO sample. This sample has been split into Seyfert galaxies (Sy; 82 sources), quasars (QSO; 67 sources), narrow line (NL; 30 sources) and broad line (BL; 60 sources). The shaded area corresponds to the luminosity of those sources within the flux-limited sample for which a significant relativistic broad Fe Kα line detection has been found. The numbers shown on the right in each panel are the median values of the correspondent distribution, also marked by the vertical dashed line.

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