Fig. 4.
Hard X-ray bolometric correction in the 2–10 keV band as a function of the bolometric luminosity for type 1 (upper panel) and type 2 (central panel) AGN. Symbols are as in the legend. Black filled triangles and open circles show the average values for type 1 and type 2 sources, respectively (directly compared in the lower panel), in bins of bolometric luminosity. The black solid and dashed lines show our best-fit relations and their extrapolations according to Eq. (2).
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