Stacy McGaugh

Stacy McGaugh is an American astronomer and astrophysicist known for his research into galaxies, cosmology, and the mass discrepancy problem, offering valuable insights into phenomena like dark matter and modified gravity. After completing his Ph.D. in Astronomy from the University of Michigan in 1992, Stacy McGaugh embarked on a distinguished career marked by groundbreaking research in galaxies and cosmology. He held extensive research fellowships, including positions at the Institute of Astronomy at the University of Cambridge, the Department of Terrestrial Magnetism of the Carnegie Institution of Washington, and Rutgers University.

At Case Western Reserve, McGaugh’s research continued to focus on galaxies, cosmology, and the mass discrepancy problem, with a primary interest in low surface brightness galaxies due to their insights into galaxy formation and evolution. A notable achievement includes his 2016 collaboration with Lelli and Schombert, which reported a significant correlation between a radial acceleration relation (RAR) in galactic rotation curves and the baryonic Tully-Fisher relation’s predictions. This finding has implications for both the ?CDM paradigm and alternative gravity theories. Recognized for his profound impact, McGaugh is consistently ranked in the top 2% of impactful authors across all sciences by Stanford-Elsevier, and was honored as a Distinguished Alumnus of the Astronomy Department, University of Michigan in 2013.