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About

Mike Eracleous is a leading astrophysicist renowned for his transformative work on supermassive black holes and their active galactic nuclei (AGN). His research primarily focuses on understanding the physics of accretion flows, the dynamics of binary black hole systems, and the evolution of quasars across cosmic time. A major contribution is his pioneering use of double-peaked emission lines to probe the structure and kinematics of accretion disks in AGN, providing direct observational evidence for disk dynamics. Eracleous has also been instrumental in large-scale spectroscopic surveys, notably as a key contributor to the Sloan Digital Sky Survey V (SDSS-V), which is conducting the first all-sky, multiepoch optical-to-infrared spectroscopic mapping. His work has garnered over 25,000 citations, reflecting its profound impact on the field. Among his notable achievements, he has led efforts to identify candidate supermassive black hole binaries, advancing our understanding of galaxy mergers and gravitational wave sources. His research continues to shape the study of black hole growth and feedback in the universe.