Fig. 11

Hard X-ray bolometric correction against 2–10 keV luminosity for 240 type-2 AGN with AGN best-fit. The 240 type-2 sample is divided into subsamples: low-r AGN sample (black data) and high-r AGN sample (yellow data). The green and orange lines represent the bolometric correction and 1σ dispersion obtained by Hopkins et al. (2007) and Marconi et al. (2004), respectively. In the de-absorbed hard X-ray luminosity range highlighted by the solid lines, we have 167 low-r and 73 high-r (in the infrared) sources.
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