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Vinu Vikram

Researcher at Argonne National Laboratory

Publications -  128
Citations -  14683

Vinu Vikram is an academic researcher from Argonne National Laboratory. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 54, co-authored 128 publications receiving 12380 citations. Previous affiliations of Vinu Vikram include University of Pennsylvania.

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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.
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A gravitational-wave standard siren measurement of the Hubble constant

B. P. Abbott, +1322 more
- 02 Nov 2017 - 
TL;DR: A measurement of the Hubble constant is reported that combines the distance to the source inferred purely from the gravitational-wave signal with the recession velocity inferred from measurements of the redshift using the electromagnetic data.
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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.
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The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models

Philip S. Cowperthwaite, +161 more
TL;DR: In this article, the Gordon and Betty Moore Foundation (GBMF5076) and the Heising-Simons Foundation (HSPF) have contributed to the creation of the DES-Brazil Consortium.
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Dark Energy Survey Year 1 results: cosmological constraints from cosmic shear

Michael Troxel, +136 more
- 27 Aug 2018 - 
TL;DR: In this paper, a 3.5% fractional uncertainty on σ8(Ωm/0.3)0.5 = 0.782-0.33 at 68% C.L.