Rest-frame X-ray spectra of the four Type 2 AGN with most counts (i.e., above 140 counts; CID339 a), CID110 b), CID522 c), and CID456 d)), characterized by increasing absorption from top to bottom, and stacked X-ray spectrum of the 19 Type 2 AGN with limited photon statistics (panel e)), showing an emission line at an energy consistent with iron Kα. An emission line is also apparent in CID339. X-ray spectra are arbitrarily scaled for visual clarity.