Explore the gravitational-wave signatures produced by supermassive black holes in this research seminar presented by Gabriela Sato-Polito from the Institute for Advanced Study. Delve into the theoretical and observational aspects of how these massive cosmic objects generate detectable gravitational waves, examining the unique characteristics and patterns that distinguish supermassive black hole signatures from other gravitational wave sources. Learn about current detection methods, data analysis techniques, and the implications of these discoveries for our understanding of black hole physics and cosmology. Gain insights into the latest research developments in gravitational wave astronomy and how supermassive black holes contribute to the gravitational wave spectrum observed by current and future detectors.