Charles Baltay

Charles Baltay

Eugene Higgins Professor Emeritus of Physics
Physics

Biographical Sketch: 

Charles Baltay is the Eugene Higgins Professor Emeritus of Physics and Astronomy. Prof. Baltay explores fundamental issues in particle physics, astrophysics, and cosmology, with a particular focus on the nature of dark energy. 

Baltay joined the faculty of Yale in 1988 and served as chair of the Department of Physics from 1995 to 2001. Previously, Baltay performed research as a professor at Columbia University in elementary particle physics and served as director of Nevis Laboratories of Columbia University from 1979 to 1985. 

He also served as co-spokesman of the Stanford Linear Detector (SLD) project at the SLAC Linear Accelerator from 1983 to 2003. 

In collaboration with the Perlmutter group at Berkeley, Professor Baltay is involved in the NASA Nancy Grace Roman space mission, having served as co-chair of the Science Working Group commissioned to develop the Roman mission concept. 

Baltay received his Ph.D. in physics from Yale University.  

Research: 

Charlie Baltay explores fundamental issues in particle physics, astrophysics, and cosmology. His research focuses on the nature of dark energy, a mysterious component that makes up three quarters of our universe that we know essentially nothing about. The Baltay group investigates dark energy via the study of distant supernova explosion events both from ground-based telescopes in the Andes Mountains in Chile (La Silla-QUEST and La Silla Schmidt Southern Survey) and from the Nancy Grace Roman Space Telescope (formerly known as WFIRST). 

Education: 

Ph.D., Yale University, 1963

Selected Publications: 

Contact Info

charles.baltay@yale.edu

+1 (203) 432-3386

WL 213

Research Website

Research Areas: Astrophysics & Cosmology

Research Type: Experimental

Experiments

CV

Experiments

DESI

Baltay

Science goal: Measure the effects of dark energy on the expansion of the Universe

WL involvement: The Yale Fiberview Camera—designed, built, and installed by the Baltay group at Wright Lab—is an integral part of the efficiency and precision of DESI.

DESI

La Silla-QUEST/La Silla Schmidt Southern Survey

Baltay

Science goal: Study the expansion of the Universe and dark energy.

WL involvement: The Baltay group’s work has improved the precision of the Hubble constant measurement using supernovae and variable stars as calibration standards, such that it is now better than the unexplained discrepancies. 

La Silla-QUEST

Roman Space Telescope

Baltay

Science goal: Study the nature of the  mysterious acceleration of the expansion of the Universe and dark energy.

WL involvement: Baltay and his collaborator Saul Perlmutter (U.C. Berkeley) have advised NASA for many years on the design and use of the Roman Space Telescope for a supernova survey. The telescope is expected to launch in 2026.

Roman Space Telescope

News