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Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

http://www.wikidata.org/entity/Q27442307

about

Cosmological tests of general relativity with future tomographic surveys.Theoretical estimates of integrated Sachs–Wolfe effect detection through the Australian Square Kilometre Array Pathfinder’s Evolutionary Map of the Universe (ASKAP- EMU) survey, with confusion, position uncertainty, shot noise, and signal-to-nois Evidence against a supervoid causing the CMB Cold Spot Neutrino lumps and the cosmic microwave background Planck 2013 results. XIX. The integrated Sachs-Wolfe effect Phantomlike behavior in a brane-world model with curvature effects Cross-correlation of cosmic far-infrared background anisotropies with large scale structures Does cosmological structure formation require dark energy?Cosmological constraints on dark energy The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae Measurement of CIB power spectra over large sky areas fromPlanckHFI maps CMB lensing tomography with the DES Science Verification galaxies Improved primordial non-Gaussianity constraints from measurements of galaxy clustering and the integrated Sachs-Wolfe effect The significance of the integrated Sachs-Wolfe effect revisited Detecting the integrated Sachs-Wolfe effect with high-redshift 21-cm surveys Cosmological measurements with forthcoming radio continuum surveys An optimal estimator for the CMB-LSS angular power spectrum and its application to WMAP and NVSS data Constraints on the early and late integrated Sachs-Wolfe effects from the Planck 2015 cosmic microwave background anisotropies in the angular power spectra A comparison of structure formation in minimally and non-minimally coupled quintessence models

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Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

http://www.wikidata.org/entity/Q27442307

description

2008 nî lūn-bûn

@nan

2008 թուականի Յունիսին հրատարակուած գիտական յօդուած

@hyw

2008 թվականի հունիսին հրատարակված գիտական հոդված

@hy

2008年の論文

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2008年論文

@yue

2008年論文

@zh-hant

2008年論文

@zh-hk

2008年論文

@zh-mo

2008年論文

@zh-tw

2008年论文

@wuu

name

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@ast

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@en

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@nl

type

label

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@ast

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@en

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@nl

prefLabel

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@ast

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@en

Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@nl

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P356

PHYSREVD.77.123520

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Physical Review D

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Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications

@en

P2093

Adam D. Myers

http://www.w3.org/2001/XMLSchema#string

Gordon T. Richards

http://www.w3.org/2001/XMLSchema#string

Robert G. Crittenden

http://www.w3.org/2001/XMLSchema#string

Ryan Scranton

http://www.w3.org/2001/XMLSchema#string

Stephen P. Boughn

http://www.w3.org/2001/XMLSchema#string

Tommaso Giannantonio

http://www.w3.org/2001/XMLSchema#string

P2860

Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds

Looking for a Cosmological Constant with the Rees-Sciama Effect

A Line-of-Sight Integration Approach to Cosmic Microwave Background Anisotropies

A correlation between the cosmic microwave background and large-scale structure in the Universe.

Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant

Perturbations of a Cosmological Model and Angular Variations of the Microwave Background

The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications

Three‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Temperature Analysis

The Supernova Legacy Survey: measurement of $\Omega_{\mathsf{M}}$, $\Omega_\mathsf{\Lambda}$ and w from the first year data set

The Shape of the Sloan Digital Sky Survey Data Release 5 Galaxy Power Spectrum

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scholarly article

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10.1103/PHYSREVD.77.123520

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12

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77

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Robert C. Nichol

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2008-06-13T00:00:00Z

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0801.4380

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