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X-ray reverberation around accreting black holes, , , , and . (May 26, 2014)The X-ray coronae of the two brightest galaxies in the Coma cluster, , , , , , and . Monthly Notices of the Royal Astronomical Society, 439 (1): 1182--1192 (Jan 14, 2014)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)Gravitationally redshifted emission implying an accretion disk and massive black hole in the active galaxy MCG–6–30–15, , , , , , , , , and 2 other author(s). Nature, 375 (6533): 659--661 (June 1995)Observational Evidence of AGN Feedback. (2012)cite arxiv:1204.4114Comment: 35 pages, 17 figures, ARAA in press.The rapid evolution of AGN feedback in brightest cluster galaxies: switching from quasar-mode to radio-mode feedback, , , , , , and . (2012)cite arxiv:1211.5606Comment: 23 pages, 11 figures, 5 tables. Submitted to MNRAS.ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix cluster, , , , , , , , , and 4 other author(s). (2016)cite arxiv:1611.00017Comment: 10 pages, 5 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)