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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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Forecast and analysis of the cosmological redshift drift

TL;DR: The Sandage-Loeb (SL) test as discussed by the authors was used to test the viability and possible properties of the cosmological redshift drift in high-precision cosmic geometric observations, becoming an irrefutable test for cosmic acceleration.
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Photometric redshifts for the S-PLUS Survey: Is machine learning up to the task?

TL;DR: In this paper , a combination of a Bayesian Neural Network and a Mixture Density Network was used to predict the photometric redshift of the Southern Photometric Local Universe Survey (S-PLUS) dataset.
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Unraveling the nature of Gravity through our clumpy Universe

TL;DR: In this paper, the authors proposed a new probe to test the nature of gravity at various redshifts through large-scale cosmological observations, using a void catalog extracted from the Sloan Digital Sky Survey (SDSS, DR10) to trace the distribution of matter along the lines of sight.
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An Outline Picture of a Growing and Rotating Planck Universe with Emerging Dark Foam

TL;DR: It is suggested that, from the beginning of Planck scale, dark matter can be considered as a kind of cosmic foam responsible for formation of galaxies and there is no need to consider dark energy for understanding cosmic acceleration.
Posted Content

Image simulations for strong and weak gravitational lensing

TL;DR: A general overview of the generation and applications of image simulations in strong and weak gravitational lensing is presented.
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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