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The X-ray properties of $z>6$ quasars: no evident evolution of accretion physics in the first Gyr of the Universe

F. Vito, W. Brandt, F. Bauer, F. Calura, R. Gilli, B. Luo, O. Shemmer, C. Vignali, G. Zamorani, M. Brusa, F. Civano, A. Comastri, и R. Nanni. (2019)cite arxiv:1908.09849Comment: 15 pages. 10 figures. 7 tables. Accepted for publication in A&A.

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Can X-ray Observations Improve Optical-UV-based Accretion-Rate Estimates for Quasars?A. Marlar, O. Shemmer, M. Brotherton, G. Richards, и C. Dix. (2022)cite arxiv:2203.16671Comment: 13 pages (aastex62), 4 figures. Accepted for publication in ApJ.The X-ray properties of $z>6$ quasars: no evident evolution of accretion physics in the first Gyr of the UniverseF. Vito, W. Brandt, F. Bauer, F. Calura, R. Gilli, B. Luo, O. Shemmer, C. Vignali, G. Zamorani, M. Brusa и 3 other автор(ы). (2019)cite arxiv:1908.09849Comment: 15 pages. 10 figures. 7 tables. Accepted for publication in A&A.Extreme star formation in the host galaxies of the fastest growing super-massive black holes at z=4.8R. Mor, H. Netzer, B. Trakhtenbrot, O. Shemmer, и P. Lira. (2012)cite arxiv:1203.1613Comment: 5 pages, 4 figures, accepted for publication in ApJL.A Novel Test of Quasar OrientationG. Richards, R. Plotkin, P. Hewett, A. Rankine, A. Rivera, Y. Shen, и O. Shemmer. (2021)cite arxiv:2106.02633Comment: 7 pages, 2 figures, accepted for publication in ApJL.Placing High-Redshift Quasars in Perspective: a Catalog of Spectroscopic Properties from the Gemini Near Infrared Spectrograph -- Distant Quasar SurveyB. Matthews, O. Shemmer, C. Dix, M. Brotherton, A. Myers, I. Andruchow, W. Brandt, G. Ferrero, S. Gallagher, R. Green и 8 other автор(ы). (2020)cite arxiv:2011.10895Comment: 20 pages, 7 figures, accepted for publication in ApJS; catalog data can be obtained at http://physics.uwyo.edu/agn/GNIRS-DQS/spectra.html.The Lack of Torus Emission from BL Lacertae Objects: An Infrared View of Unification with WISER. Plotkin, S. Anderson, W. Brandt, S. Markoff, O. Shemmer, и J. Wu. (2011)cite arxiv:1112.5162Comment: 6 Pages, 3 Figures, accepted for publication in ApJ Letters.

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