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Observational probes of cosmic acceleration

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In this article, the authors present extensive forecasts for constraints on the dark energy equation of state and parameterized deviations from General Relativity, achievable with Stage III and Stage IV experimental programs that incorporate supernovae, BAO, weak lensing, and cosmic microwave background data.
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This article is published in Physics Reports.The article was published on 2013-09-10 and is currently open access. It has received 1253 citations till now. The article focuses on the topics: Dark energy & Lambda-CDM model.

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Gravity at the horizon: on relativistic effects, CMB-LSS correlations and ultra-large scales in Horndeski's theory

TL;DR: In this paper, the impact of consistent modifications of gravity on the largest observable scales, focusing on relativistic effects in galaxy number counts and the cross-correlation between the matter in the galaxies, is discussed.
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Dark Energy Survey Year 1 results: the impact of galaxy neighbours on weak lensing cosmology with IM3SHAPE

TL;DR: In this paper, the authors used a suite of simulated images based on the Dark Energy Survey (DES Y1) IM3SHAPE catalogue to explore the impact of galaxy neighbours on shape measurement and shear cosmology.
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Improving initial conditions for cosmological N-body simulations

TL;DR: In this paper, the authors proposed an approach to solve the problem of energy-efficient computing in the context of cloud computing, using the FAS Division of Science, Research Computing Group at Harvard University.
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SPIDERS: the spectroscopic follow-up of X-ray-selected clusters of galaxies in SDSS-IV

TL;DR: Alfred P. Sloan Foundation, US Department of Energy Office of Science; Center for High Performance Computing at the University of Utah; Brazilian Participation Group, Carnegie Institution for Science; Carnegie Mellon University; Chilean Participation Group; French Participation Group and Harvard-Smithsonian Center for Astrophysics; Instituto de Astrofisica de Canarias; Johns Hopkins University; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo; Lawrence Berkeley National Laboratory; Leibniz Institut fur Astrophysik Potsdam (A
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The relationship between infrared, optical, and ultraviolet extinction

TL;DR: In this article, the average extinction law over the 3.5 micron to 0.125 wavelength range was derived for both diffuse and dense regions of the interstellar medium. And the validity of the law over a large wavelength interval suggests that the processes which modify the sizes and compositions of grains are stochastic in nature.
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