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Gary Bernstein

Researcher at University of Pennsylvania

Publications -  393
Citations -  31413

Gary Bernstein is an academic researcher from University of Pennsylvania. The author has contributed to research in topics: Weak gravitational lensing & Galaxy. The author has an hindex of 86, co-authored 364 publications receiving 27254 citations. Previous affiliations of Gary Bernstein include University of Oxford & University of Miami.

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Journal ArticleDOI

Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing

T. M. C. Abbott, +199 more
- 27 Aug 2018 - 
TL;DR: In this paper, the cosmological results from a combined analysis of galaxy clustering and weak gravitational lensing, using 1321 deg2 of griz imaging data from the first year of the Dark Energy Survey (DES Y1), were presented.
Journal ArticleDOI

The dark energy camera

B. Flaugher, +121 more
TL;DR: The Dark Energy Camera as mentioned in this paper was designed and constructed by the Dark Energy Survey Collaboration, and meets or exceeds the stringent requirements designed for the wide-field and supernova surveys for which the collaboration uses it.
Journal ArticleDOI

The Dark Energy Survey: more than dark energy - an overview

T. M. C. Abbott, +156 more
TL;DR: In this paper, the authors presented the results of the Dark Energy Survey (DES) 2013, 2014, 2015, 2016, 2017, 2018, 2019 and 2019 at the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign.
Posted Content

Report of the Dark Energy Task Force

TL;DR: In this article, the authors present an observational program to determine the dark energy properties as well as possible, based on the observation of the acceleration of the universe, along with dark matter, the observed phenomenon that most directly demonstrates that our theories of fundamental particles and gravity are either incorrect or incomplete.
Journal ArticleDOI

The Dark Energy Camera

B. Flaugher, +117 more
TL;DR: The Dark Energy Camera as discussed by the authors was designed and constructed by the Dark Energy Survey Collaboration, and meets or exceeds the stringent requirements designed for the wide-field and supernova surveys for which the collaboration uses it.