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Daniel Eisenstein studies cosmology and extragalactic astronomy, employing both theoretical and observational methods. His research has primarily focused on the development of the baryon acoustic oscillation method to measure the cosmic distance scale and study dark energy. He received his Ph.D. from Harvard University in 1996 and has held postdoctoral positions at the Institute for Advanced Study and the University of Chicago. He was a faculty member in astronomy at the University of Arizona for nine years before moving to his current position as professor of astronomy at Harvard University in 2010. Eisenstein has played a significant role in the Sloan Digital Sky Survey since 1998, serving as the Director of SDSS-III from 2007 to 2015, and is a member of the Dark Energy Spectroscopic Instrument collaboration, where he served as co-Spokesperson from 2014 to 2020. Additionally, he is a part of the JWST Near-Infrared Camera instrument team and actively participates in several scientific collaborations and national committees. Eisenstein's work currently focuses on the analysis of large redshift surveys, development of new statistical methods for interpreting large-scale structures, and high-performance cosmological simulations using novel codes such as Abacus. He has also been involved in significant observational programs like the JWST Advanced Deep Extragalactic Survey (JADES).
Harvard University • Cambridge, MA
Teaching and conducting research in astronomy with a focus on cosmology and extragalactic astronomy.
Administered by the Harvard Kenneth C. Griffin Graduate School of Arts and Sciences (GSAS).