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A reassessment of the evidence of the Integrated Sachs-Wolfe effect through the WMAP-NVSS correlation

Author
RACCANELLI, A1 ; BONALDI, A1 2 ; NEGRELLO, M3 ; MATARRESE, S4 ; TORMEN, G1 ; DE ZOTTI, G2 5
[1] Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
[2] INAF, Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy
[3] The Open University, Walton Hall, Milton Keynes MK7 6AA, United Kingdom
[4] Dipartimento di Fisica 'Galileo Galilei', Università di Padova, and INFN Sezione di Padova, via F. Marzolo, 8, 35131 Padova, Italy
[5] SISSA, Via Beirut 4, 34014 Trieste, Italy
Source

Monthly Notices of the Royal Astronomical Society. 2008, Vol 386, Num 4, pp 2161-2166, 6 p ; ref : 1/2 p

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Blackwell Science, Oxford
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
cosmic microwave background cosmological parameters cosmology: observations radio continuum: galaxies
Keyword (fr)
Anisotropie Continuum Corrélation angulaire Corrélation croisée Cosmologie Déplacement vers le rouge Effet Sachs Wolfe Etude ciel Fonction corrélation Matière sombre froide Modèle Paramètre cosmologique Radiogalaxies Radiosource cosmique Rayonnement fond cosmique Répartition spatiale Satellite WMAP Spectre puissance
Keyword (en)
Anisotropy Continuum Angular correlation Cross correlations Cosmology Red shift Sachs Wolfe effect Sky surveys Correlation functions Cold dark matter Models Cosmological parameter Radio galaxies Cosmic radio sources Cosmic background radiation Spatial distribution WMAP satellite Power spectra
Keyword (es)
Continuo Efecto Sachs Wolfe Materia oscura fría Modelo Parámetro cosmológico Satélite WMAP
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20358890

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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