Uncorrelated universe: Statistical anisotropy and the vanishing angular correlation function in WMAP years 1–3 - Wikidata - wikimedia - TriplyDB

Uncorrelated universe: Statistical anisotropy and the vanishing angular correlation function in WMAP years 1–3

Uncorrelated universe: Statistical anisotropy and the vanishing angular correlation function in WMAP years 1–3

http://www.wikidata.org/entity/Q56815031

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Large-Angle Anomalies in the CMB Cosmology and Fundamental Physics with the Euclid Satellite.Signature of local motion in the microwave sky.Porosity criterion for hyperbolic voids and the cosmic microwave background Low power on large scales in just-enough inflation models Kolmogorov stochasticity parameter measuring the randomness in the cosmic microwave background Probing the anisotropic local Universe and beyond with SNe Ia data Planck 2015 results. XVI. Isotropy and statistics of the CMB Cuscuton cosmology: Dark energy meets modified gravity Search for Non-Gaussianities in the WMAP Data with the Scaling Index Method Symmetry and Antisymmetry of the CMB Anisotropy Pattern Complete statistical analysis for the quadrupole amplitude in an ellipsoidal universe Recent results and perspectives on cosmology and fundamental physics from microwave surveys

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Uncorrelated universe: Statistical anisotropy and the vanishing angular correlation function in WMAP years 1–3

http://www.wikidata.org/entity/Q56815031

description

im Januar 2007 veröffentlichter wissenschaftlicher Artikel

@de

wetenschappelijk artikel

@nl

наукова стаття, опублікована в січні 2007

@uk

name

Uncorrelated universe: Statist ...... ion function in WMAP years 1–3

@en

Uncorrelated universe: Statist ...... ion function in WMAP years 1–3

@nl

type

label

Uncorrelated universe: Statist ...... ion function in WMAP years 1–3

@en

Uncorrelated universe: Statist ...... ion function in WMAP years 1–3

@nl

prefLabel

Uncorrelated universe: Statist ...... ion function in WMAP years 1–3

@en

Uncorrelated universe: Statist ...... ion function in WMAP years 1–3

@nl

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PHYSREVD.75.023507

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Physical Review D

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Uncorrelated universe: Statist ...... ion function in WMAP years 1–3

@en

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Craig J. Copi

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

Dominik J. Schwarz

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

Dragan Huterer

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

Glenn D. Starkman

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

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High resolution foreground cleaned CMB map from WMAP

First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters

Significance of the largest scale CMB fluctuations in WMAP

Assessing the effects of foregrounds and sky removal in WMAP

Is the low-l microwave background cosmic?

CMB multipole measurements in the presence of foregrounds

Examination of Evidence for a Preferred Axis in the Cosmic Radiation Anisotropy

Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background

First‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Preliminary Maps and Basic Results

Low-order multipole maps of cosmic microwave background anisotropy derived fromWMAP

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scholarly article

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10.1103/PHYSREVD.75.023507

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

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2

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75

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2007-01-08T00:00:00Z

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astro-ph/0605135

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