Austin / Baltimore / New York / Oxford / A1C1 Lanham / Los Angeles / Providence / Miville / Mail Code / /
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Cepheid / Adnet Systems Inc. / PAB Astrophysics Laboratory / Thomson / Komatsu / /
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Canada / Columbia / United Kingdom / /
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pence / PAB / / /
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Diplomatic Relations / /
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Princeton University / University of British Columbia / University of Chicago / Jadwin Hall / Peyton Hall / University of Oxford / Brown University / University of Toronto / Canadian Institute / Johns Hopkins University / /
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non power-law indices / scale-invariant power law fluctuations / data processing / software implementation / power-law models / lower energy distribution / dark energy equation / power law distribution / /
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Aix / /
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UCLA / Space Flight Center / The Johns Hopkins University / University of Toronto / Toronto / Brown University / NASA’s Goddard Space Flight Center / University of Chicago / Chicago / Princeton University / University of British Columbia / Vancouver / Canadian Institute for Theoretical Astrophysics / University of Oxford / National Aeronautics and Space Administration / Princeton Center for Theoretical Physics / /
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Ai / /
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Gibbs / /
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Texas / New Jersey / Maryland / Illinois / British Columbia / New York / Rhode Island / California / /
Submitted to the Astrophysical Journal Supplement Series Five-Year Wilkinson Microwave Anisotropy Probe (WMAP1 ) Observations: Likelihoods and Parameters from the WMAP data J. Dunkley2,3,4 , E. Komatsu5 , M. R. Nolta6 ,