Biosketch

Steven M. Kahn is the Dean of Mathematical and Physical Sciences and a Professor of Physics and Astronomy at the University of California, Berkeley. Prior to taking up this current position, he was the Cassius Lamb Kirk Professor in the Natural Sciences at Stanford University (2003-2022), the I.I. Rabi Professor of Physics and Astronomy at Columbia University (1995-2003), and a Professor of Physics and Astronomy at Berkeley (1984-1995). He received his A.B. degree summa cum laude from Columbia in 1975, his Ph.D. in Physics from Berkeley in 1980, and was a Center Postdoctoral Fellow at the Harvard-Smithsonian Center for Astrophysics from 1980-82. Kahn is an experimental astrophysicist and cosmologist. He began his career working in X-ray astronomy, where he pioneered the development of high-resolution X-ray spectroscopy of cosmic sources, and the relevant atomic physics. Kahn was the U.S. Principal Investigator on the Reflection Grating Spectrometer experiment which was launched on the European Space Agency’s XMM-Newton Observatory in December 1999. With his move to Stanford in 2003, Kahn switched his attention to experimental cosmology where he played an early crucial role in the design and development of the ground-based Vera C. Rubin Observatory and served as director of the project from 2013 through 2022. Kahn is an elected Member of the National Academy of Sciences, and an elected Fellow of the American Academy of Arts and Sciences, the American Association for the Advancement of Science and the American Physical Society.

Research Interests

Kahn’s current research interests primarily center around the use of the newly constructed Vera C. Rubin Observatory for observational cosmology and time-domain astrophysics. The Rubin Observatory is a world-unique facility designed to provide deep images in six visible bands over the entire southern hemisphere of sky. Over ten years of observations, each patch of the southern sky will be observed nearly one thousand times. The resulting data base will allow us to measure everything that moves in the sky (e.g. small bodies in the solar system, stellar parallax and proper motion), everything that varies in brightness (e.g. supernovae, variable stars, active galactic nuclei), and everything in the sky down to ~ 27th magnitude (nearly 20 billion galaxies and a comparable number of stars). For precision cosmology, Rubin will provide a catalog of measured positions, colors, and shapes of galaxies out to redshifts of z > 1. The correlations among these parameters yield precision constraints on the distribution of dark matter in the universe and the nature of dark energy through detailed measurements of the cosmic expansion history as a function of time. Kahn is also interested in using the Rubin Observatory to search for and characterize very short-term transient variability of faint sources, which could be linked to gamma-ray bursts, fast radio bursts, and other explosive phenomena.

Membership Type

Member

Election Year

2025

Primary Section

Section 12: Astronomy

Secondary Section

Section 13: Physics