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Coronal Properties of the Seyfert 1.9 Galaxy MCG -05-23-016 Determined from Hard X-ray Spectroscopy with NuSTAR, , , , , , , , , and 8 other author(s). (Dec 18, 2014)The high-Eddington NLS1 Ark 564 has the coolest corona, , , , , , and . (Mar 28, 2017)How AGN Jets Heat the Intracluster Medium -- Insights from Hydrodynamic Simulations, and . (2016)cite arxiv:1605.01725Comment: 17 pages, 12 figures, submitted to ApJ.The Accretion Disk Wind in the Black Hole GRS 1915+105, , , , , , , , , and . (Mar 4, 2016)Powerful, Rotating Disk Winds from Stellar-mass Black Holes, , , , , , , and . (Oct 5, 2015)Accretion Disk Dynamo as the Trigger for X-Ray Binary State Transitions, , and . Astrophys. J., (Aug 14, 2015)The remarkable X-ray variability of IRAS 13224&\#45;&\#45;3809 I: the variability process, , , , , , , , , and 10 other author(s). (Mar 28, 2018)On broad iron K-alpha lines in Seyfert 1 galaxies, , , , , , , and . (1995)cite arxiv:astro-ph/9507061Comment: uuencoded compressed postscript. The preprint is also available at http://www.ast.cam.ac.uk/preprint/PrePrint.html.Disk-Wind Connection During the Heartbeats of GRS 1915+105, , , , , , , , , and 7 other author(s). (Oct 18, 2016)How AGN Jets Heat the Intracluster Medium &\#45;&\#45; Insights from Hydrodynamic Simulations, and . (Jun 21, 2016)