Fig. 14.

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Intrinsic absorption in AGN protocluster members. The red histogram shows the distribution of the intrinsic absorption of the eight protocluster members (including the Spiderweb) for which a robust measurement of NH has been possible. The blue dashed histogram shows the upper limits on NH obtained for six sources. The black solid line shows the distribution of NH expected in the model of Gilli et al. (2007) at the flux limit of our observations. The two Compton-thick candidates with a reflection-dominated spectrum are not included.
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