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A Large Population of Obscured AGN in Disguise as Low Luminosity AGN in Chandra Deep Field South

, , , , , and . (2020)cite arxiv:2002.00955Comment: 23 pages, 16 figures, submitted to the Astrophysical Journal, first round of revision completed.

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Radio Loud AGNs are Mergers, , , and . (May 27, 2015)A Large Population of Obscured AGN in Disguise as Low Luminosity AGN in Chandra Deep Field South, , , , , and . (2020)cite arxiv:2002.00955Comment: 23 pages, 16 figures, submitted to the Astrophysical Journal, first round of revision completed.The X-ray properties of $z>6$ quasars: no evident evolution of accretion physics in the first Gyr of the Universe, , , , , , , , , and 3 other author(s). (2019)cite arxiv:1908.09849Comment: 15 pages. 10 figures. 7 tables. Accepted for publication in A&A.X-ray spectroscopy of the z=6.4 quasar J1148+5251, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1702.07349Comment: 9 pages, 3 figures, 1 table, MNRAS in press.The most luminous blue quasars at 3.0<z<3.3. II. CIV/X-ray emission and accretion disc physics, , , , , , , , , and 5 other author(s). (2021)cite arxiv:2107.02806Comment: 22 pages, 15 figures (with 3 more figures in the Appendix), abstract abridged. Accepted for publication in A&A.