Noah Wolfe
NW22-261
Noah works with Salvatore Vitale and is interested in understanding extreme astrophysical laboratories through their gravitational-wave signals with Bayesian parameter estimation techniques. Previously, he developed a new sampling technique to study deviations from general relativity in gravitational wave signals from black hole mergers. Noah has also investigated how well we could characterize sub-solar mass black hole mergers with current and next-generation detectors. Currently, he is developing tools to enable forecasts of astrophysical population inference with next-generation gravitational wave detectors. Noah graduated from North Carolina State University in 2022, where he modeled gravitational-wave signals from core-collapse supernovae.