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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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Dark energy two decades after: Observables, probes, consistency tests

TL;DR: In this review, the developments that led to the discovery of dark energy are summarized and the parametric descriptions ofdark energy and the cosmological tests that allow us to better understand its nature are discussed.
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Science with the space-based interferometer eLISA. III: probing the expansion of the universe using gravitational wave standard sirens

TL;DR: In this paper, the authors investigate the capability of various configurations of the space interferometer eLISA to probe the late-time background expansion of the universe using gravitational wave standard sirens.
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Dark Energy Survey year 1 results: Constraints on extended cosmological models from galaxy clustering and weak lensing

T. M. C. Abbott, +113 more
- 07 Jun 2019 - 
TL;DR: In this paper, the authors present constraints on extensions of the minimal cosmological models dominated by dark matter and dark energy, ΛCDM and wCDM, by using a combined analysis of galaxy clustering and weak gravitational lensing from the first-year data of the Dark Energy Survey (DES Y1) in combination with external data.
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The MICE Grand Challenge light-cone simulation – III. Galaxy lensing mocks from all-sky lensing maps

TL;DR: In this article, a new N-body lightcone simulation from the MICE Grand Challenge (MICE-GC), containing about 70 billion dark-matter particles in a (3 Gpc)^3 comoving volume, from which they built halo and galaxy catalogues using a Halo Occupation Distribution and Halo Abundance Matching technique.
References
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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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