Skip to main content

Senior ITC Members

Content tagged with Senior ITC Members

Not finding what you're looking for? Try using Advanced Search.
Not finding what you're looking for? Try using Advanced Search.

Fabio Pacucci

Person

Research Interests: Theoretical and observational studies of black holes, including supermassive black holes, quasars, black hole seeds, intermediate-mass black holes, and wandering black holes. I am also involved in the development of next-generation...

Liam Connor

Person

Research interests: The origin of Fast Radio Bursts and their application to cosmology; the intersection of AI and astrophysics, in particular computer vision methods for astronomical imaging and ill-posed 3D reconstruction. To advance these subjects, I...

Ashley Villar

Person

Research Interests:  Theoretical and observational studies of extragalactic transients, including core-collapse supernovae and kilonovae. Development of statistical and deep learning methodologies for wide-field surveys, such as the Vera C. Rubin...

Lisa Kewley

Person

Lisa Kewley is Director of the Center for Astrophysics | Harvard & Smithsonian. She is Director of the Smithsonian Astrophysical Observatory, Director of the Harvard College Observatory, and Professor of Astrophysics at the Harvard Department of Astronomy...

Morgan MacLeod

Person

Morgan MacLeod is a Lecturer in Astronomy whose research focuses on stellar encounters in binary systems and their imprints on the transient night sky. 

Morgan uses computational and simulation methods to trace close encounters of stars and compact objects...

Karin Öberg

Person

The Öberg Astrochemistry Lab pursues laboratory ice experiments and astronomical observations that address how astrochemically important molecules form, and how they may evolve into larger molecules associated with the origins of life.  An important...

Charlie Conroy

Person

Research Interests:  Galaxy formation and evolution, connection between galaxies and dark matter halos, stellar population modeling, stellar evolution.