POWER ASYMMETRY IN COSMIC MICROWAVE BACKGROUND FLUCTUATIONS FROM FULL SKY TO SUB-DEGREE SCALES: IS THE UNIVERSE ISOTROPIC?
- Author
- HANSEN, F. K1 2 ; BANDAY, A. J3 4 ; GORSKI, K. M5 6 7 ; ERIKSEN, H. K1 2 ; LILJE, P. B1 2
[1] Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindem, 0315 Oslo, Norway
[2] Centre of Mathematics for Applications, University of Oslo, P.O. Box 1053 Blindem, 0316 Oslo, Norway
[3] Max-Planck-Institut fiir Astrophysik, Karl Schwarzschild-Str. 1, Postfach 1317, 85741 Garching bei München, Germany
[4] Centre d'Etude Spatiale des Rayonnements, 9 av du Colonel Roche, BP 44346, 31028 Toulouse, France
[5] Jet Propulsion Laboratory, M/S 169/327, 4800 Oak Grove Drive, Pasadena, CA 91109, United States
[6] Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
[7] California Institute of Technology, Pasadena, CA 91125, United States - Source
The Astrophysical journal. 2009, Vol 704, Num 2, pp 1448-1458, 11 p ; 1 ; ref : 1/2 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- IOP, Bristol
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- cosmic microwave background cosmology: observations methods: data analysis methods: statistical
- Keyword (fr)
- Analyse donnée Asymétrie Cosmologie Fluctuation Méthode statistique Rayonnement fond cosmique Univers isotrope
- Keyword (en)
- Data analysis Asymmetry Cosmology Fluctuations Statistical method Cosmic background radiation Isotropic universe
- Keyword (es)
- Método estadístico Universo isótropo
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 22144110
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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DOI
10.1088/0004-637X/704/2/1448 
https://dx.doi.org/10.1088/0004-637X/704/2/1448
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