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Observational probes of cosmic acceleration

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TLDR
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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The mass function dependence on the dynamical state of dark matter haloes

TL;DR: In this paper, a generalized mass function framework was proposed to account for the dynamical state of the dark matter haloes in the galaxy clusters using the MultiDark suite of simulations and the high-mass objects M > 2.
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Observational constraints to a unified cosmological model

TL;DR: In this article, a phenomenological unified model (UM) for dark matter and dark energy based on an equation of state parameter w that scales with the arctan of the redshift was proposed.
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Palatini formulation of the conformally invariant $$f\left( R,L_m\right) $$ gravity theory

TL;DR: In this article , the authors investigated the field equations of the conformally invariant models of gravity with curvature-matter coupling, constructed in Weyl geometry, using the Palatini formalism.
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Cosmological tests of the osculating Barthel–Kropina dark energy model

TL;DR: In this article , the authors further investigate the dark energy model based on the Finsler geometry inspired osculating Barthel-Kropina cosmology and compare it with the standard $$\Lambda model.
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Evolution of the Dark Matter Distribution with 3-D Weak Lensing

TL;DR: In this paper, the authors present a direct detection of the growth of large-scale structure, using weak gravitational lensing and photometric redshift data from the COMBO-17 survey.
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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