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A physical model for the UV/optical power spectra of AGN

, , , , and . (2022)cite arxiv:2207.04917Comment: 15 (+11 in Appendix) pages, 12 figures, accepted for publication by ApJ.

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A dynamic black hole corona in an active galaxy through X-ray reverberation mapping, , , , , , , , , and 11 other author(s). (2020)cite arxiv:2001.06454Comment: Accepted for publication. 3 figures.Black hole spin and size of the X-ray emitting region(s) in the Seyfert 1.5 galaxy ESO 362-G18, , , , , , , , , and . (Jul 4, 2014)Modeling the Optical-X-ray Accretion Lag in LMC X-3: Insights Into Black-Hole Accretion Physics, , , , , , and . (Jan 22, 2014)A physical model for the UV/optical power spectra of AGN, , , , and . (2022)cite arxiv:2207.04917Comment: 15 (+11 in Appendix) pages, 12 figures, accepted for publication by ApJ.On measuring the Hubble constant with X-ray reverberation mapping of active galactic nuclei, , , , , , , , , and 1 other author(s). (2021)cite arxiv:2110.15651Comment: Accepted for publication in MNRAS.The Quiescent Intracluster Medium in the Core of the Perseus Cluster, , , , , , , , , and 206 other author(s). (2016)cite arxiv:1607.04487Comment: 31 pages, 11 Figs, published in Nature July 8.