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M. S. S. Gill

Researcher at Stanford University

Publications -  138
Citations -  9476

M. S. S. Gill is an academic researcher from Stanford University. The author has contributed to research in topics: Galaxy & LIGO. The author has an hindex of 35, co-authored 138 publications receiving 8165 citations. Previous affiliations of M. S. S. Gill include Ohio State University & Max Planck Society.

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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 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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The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

Philip S. Cowperthwaite, +99 more
TL;DR: In this article, the spectral energy distribution (SED) of the binary neutron star merger GW170817 was inferred from the optical and NIR spectrograms of the first electromagnetic counterpart to a gravitational wave source from Advanced LIGO/Virgo.
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Observation of a broad structure in the pi(+)pi(-)J/psi mass spectrum around 4.26 GeV/c(2)

Bernard Aubert, +634 more
TL;DR: Fits to the mass spectrum indicate that a broad resonance with a mass of about 4.26 GeV/c2 is required to describe the observed structure, and the presence of additional narrow resonances cannot be excluded.