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Three‐Year<i>Wilkinson Microwave Anisotropy Probe</i>(<i>WMAP</i>) Observations: Temperature Analysis
The Astrophysical Journal Supplement Series · 2007 · Vol. 170(2) · pp. 288–334
G. Hinshaw✉(Goddard Space Flight Center)Michael R. Nolta(University of Toronto)C. L. Bennett(Johns Hopkins University)Rachel Bean(Cornell University)Olivier Doré(University of Toronto)M. R. Greason(Science Systems and Applications (United States))M. Halpern(University of British Columbia)Robert Hill(Science Systems and Applications (United States))N. Jarosik(Princeton University)A. Kogut(Goddard Space Flight Center)Eiichiro Komatsu(The University of Texas at Austin)M. Limon(Science Systems and Applications (United States))N. Odegard(Science Systems and Applications (United States))S. S. Meyer(University of Chicago)Lyman A. Page(Princeton University)Hiranya V. Peiris(University of Chicago)David N. Spergel(Princeton University)Gregory S. Tucker(Brown University)Licia Verde(University of Pennsylvania)J. L. Weiland(Science Systems and Applications (United States))Edward J. Wollack(Goddard Space Flight Center)E. L. Wright
Abstract
1WMAP is the result of a partnership between Princeton University and NASA’s Goddard Space Flight Center. Scientific guidance is provided by the WMAP Science Team.
Radio Astronomy Observations and TechnologyCosmology and Gravitation TheoriesAstrophysics and Cosmic PhenomenaCMB cold spotCosmic microwave backgroundSkyPhysicsResidualAstrophysicsSpectral densityAnisotropyPoint sourceRemote sensing
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First‐Year <i>Wilkinson Microwave Anisotropy Probe</i> ( <i>WMAP</i> ) Observations: Implications For Inflation
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Three‐Year <i>Wilkinson Microwave Anisotropy Probe</i> ( <i>WMAP</i> ) Observations: Polarization Analysis
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