Kyle Kremer joined the Carnegie Observatories in 2020 as an NSF Fellow. He develops N-body simulations of dense stellar clusters, with a particular focus upon the dynamical formation and evolution of black hole binaries within these environments. His primary current interest is in applications to gravitational wave astrophysics and high-energy transients.
Before arriving in Pasadena, Kremer was a member of CIERA at Northwestern University, where he earned his Ph.D. in Astronomy.