Figure 15
NHand obscured fraction versus 2–10 keV luminosity for all sources. Obscured fraction is calculated in equal logarithmic luminosity bins, as the number of sources with NH > 1022 cm−2 divided by the total number of sources in that bin, where more than one source exists per bin.

NHand obscured fraction versus 2–10 keV luminosity for all sources. Obscured fraction is calculated in equal logarithmic luminosity bins, as the number of sources with NH > 1022 cm−2 divided by the total number of sources in that bin, where more than one source exists per bin.

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