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C. B. D'Andrea

Researcher at University of Pennsylvania

Publications -  183
Citations -  17093

C. B. D'Andrea is an academic researcher from University of Pennsylvania. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 59, co-authored 179 publications receiving 14358 citations. Previous affiliations of C. B. D'Andrea include University of Southampton & Carnegie Institution for Science.

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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.
Journal ArticleDOI

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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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.