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On the hunt for ultramassive black holes in brightest cluster galaxies, , , and . (2012)cite arxiv:1204.5759Comment: 9 pages, 3 figures, accepted for publication in MNRAS.Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ~100pc scales, , , , , , , , , and 2 other author(s). (2015)cite arxiv:1503.07873Comment: 26 pages, 11 figures. Accepted for publication in MNRAS.Does absorption against AGN reveal supermassive black hole accretion?, , , , , , , , , and . (2022)cite arxiv:2210.14922Comment: Submitted to MNRAS.Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales, , , , , , , , , and 10 other author(s). (2015)cite arxiv:1508.05941Comment: 20 pages, 12 figures. Accepted for publication in ApJ.A Ten Billion Solar Mass Outflow of Molecular Gas Launched by Radio Bubbles in the Abell 1835 Brightest Cluster Galaxy, , , , , , , , , and 10 other author(s). (2013)cite arxiv:1309.0013Comment: Five Figures, submitted to ApJ.The DESI Survey Validation: Results from Visual Inspection of the Quasar Survey Spectra, , , , , , , , , and 62 other author(s). (2022)cite arxiv:2208.08517Comment: AJ, submitted, 26 pages, 15 figures, 9 tables, one of a suite of 8 papers detailing targeting for DESI.Observational limits on the gas mass of a z=4.9 galaxy, , , , , , , , and . (2012)cite arxiv:1210.0899Comment: 14 pages, 4 figures, published in ApJL.Close entrainment of massive molecular gas flows by radio bubbles in the central galaxy of Abell 1795, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1708.08935Comment: 14 pages, 9 figures, accepted to MNRAS.A Mechanism for Stimulated AGN Feedback in Massive Galaxies, , , , , , and . (2016)cite arxiv:1604.04629Comment: Submitted to Ap.J.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.