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23 ta ish
Ish: Probing the Largest Scale Structure in the Universe with Polarization Map of Galaxy Clusters
First‐Year <i>Wilkinson Microwave Anisotropy Probe</i> ( <i>WMAP</i> ) Observations: Determination of Cosmological Parameters
David N. Spergel, Licia Verde, Hiranya V. Peiris +14
MaqolaOchiq kirish200366 iqtibosABIFirst‐Year <i>Wilkinson Microwave Anisotropy Probe</i> ( <i>WMAP</i> ) Observations: Preliminary Maps and Basic Results
C. L. Bennett, M. Halpern, G. Hinshaw +18
MaqolaOchiq kirish200314 iqtibosABIAll-sky analysis of polarization in the microwave background
Matías Zaldarriaga, Uroš Seljak
Maqola19974 iqtibosABIStatistics of cosmic microwave background polarization
Marc Kamionkowski, Arthur Kosowsky, Albert Stebbins
Maqola19973 iqtibosABISignificance of the largest scale CMB fluctuations in WMAP
A. de Oliveira‐Costa, Max Tegmark, Matías Zaldarriaga +1
MaqolaOchiq kirish20042 iqtibosABIWeak lensing analysis in three dimensions
P. G. Castro, Alan Heavens, T. Kitching
MaqolaOchiq kirish20052 iqtibosABI