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Fig. 5.

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Distributions of λsBHAR for obscured and unobscured AGN. The top panel presents the distributions using an NH threshold of 1023 cm−2 for the source classification. The bottom panel presents the results using NH = 1022 cm−2 to characterise sources. In both cases, the errors of the NH measurements have been taken into account (see text for more details). Distributions are also weighted based on the redshift and LX of the sources.

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