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We present the results from the X‐ray spectral analysis of high‐redshift active galactic nuclei (AGN) in the Chandra Deep Field South (CDFS), making use of the new 4 Ms data set and new X‐ray spectral models from Brightman & Nandra, which account for Compton scattering and the geometry of the circumnuclear material. Our goals are to ascertain to what extent the torus paradigm of local AGN is applicable...
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