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

Author
COLE, Shaun1 ; PERCIVAL, Will J2 ; COLLESS, Matthew5 ; COLLINS, Chris7 ; COUCH, Warrick8 ; CROSS, Nicholas J. G2 4 ; DALTON, Gavin10 9 ; EKE, Vincent R1 ; DE PROPRIS, Roberto11 ; DRIVER, Simon P12 ; EFSTATHIOU, George13 ; ELLIS, Richard S14 ; PEACOCK, John A2 ; GLAZEBROOK, Karl4 ; JACKSON, Carole15 ; JENKINS, Adrian1 ; LAHAV, Ofer16 ; LEWIS, Ian9 ; LUMSDEN, Stuart17 ; MADDOX, Steve18 ; MADGWICK, Darren13 ; PETERSON, Bruce A12 ; SUTHERLAND, Will13 ; NORBERG, Peder3 ; TAYLOR, Keith14 ; BAUGH, Carlton M1 ; FRENK, Carlos S1 ; BALDRY, Ivan4 ; BLAND-HAWTHORN, Joss5 ; BRIDGES, Terry6 ; CANNON, Russell5
[1] Department of Physics, University of Durham, Science Laboratories, South Road, Durham DH1 3LE, United Kingdom
[2] Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, United Kingdom
[3] Institut für Astronomie, Departement Physik, ETH Zurich, HPF G3.1, Zurich 8093, Switzerland
[4] Department of Physics & Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218-2686, United States
[5] Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia
[6] Department of Physics, Queen's University, Kingston, ON K7L 3N6, Canada
[7] Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead L14 ILD, United Kingdom
[8] School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
[9] Department of Physics, Keble Road, Oxford OX1 3RH, United Kingdom
[10] Rutherford Appleton Laboratory, Chiltern, Didcot OX11 OQX, United Kingdom
[11] H.H. Wills Physics Laboratory, University of Bristol, Royal Fort, Tyndall Avenue, Bristol BS8 1TL, United Kingdom
[12] Research School of Astronomy & Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia
[13] Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 OHA, United Kingdom
[14] Department of Astronomy, California Institute of Technology, Pasadena, CA 91125, United States
[15] Australia Telescope National Facility, PO Box 76, Epping NSW 1710, Australia
[16] Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
[17] Department of Physics & Astronomy E C Stoner Building, Leeds LS2 9JT, United Kingdom
[18] School of Physics and Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD, United Kingdom
The 2dFGRS Team
Source

Monthly Notices of the Royal Astronomical Society. 2005, Vol 362, Num 2, pp 505-534, 30 p ; ref : 89 ref

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
cosmological parameters large-scale structure of Universe
Keyword (fr)
Analyse spectre Baryon Correction Cosmologie Couleur Déplacement vers le rouge Fonction sélection Galaxies Masse neutrino Masse particule élémentaire Matière sombre froide Matrice covariance Modèle cosmologique Modèle hybride Paramètre cosmologique Rayonnement fond cosmique Spectre masse Spectre puissance Structure grande échelle Satellite WMAP
Keyword (en)
Spectrum analysis Baryons Corrections Cosmology Color Red shift Selection function Galaxies Neutrino mass Elementary particle mass Cold dark matter Covariance matrices Cosmological models Hybrid model Cosmological parameter Cosmic background radiation Mass spectra Power spectra Large-scale structure WMAP satellite
Keyword (es)
Análisis espectro Función selección Materia oscura fría Modelo híbrido Parámetro cosmológico Satélite WMAP
Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
17065043

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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