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20032026
most citedFive-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results

1.8k citations · 5.2k across the 61 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 125 cited

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Bayesian Estimation of CMB Polarization Maps

J. Dunkley, D. N. Spergel, E. Komatsu +17

We describe a sampling method to estimate the polarized CMB signal from observed maps of the sky. We use a Metropolis-within-Gibbs algorithm to estimate the polarized CMB map, cont…

astro-ph2008★ 1.8k cited

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results

G. Hinshaw, J. L. Weiland, R. S. Hill +18

We present new full-sky temperature and polarization maps in five frequency bands from 23 to 94 GHz, based on data from the first five years of the WMAP sky survey. The five-year m…

astro-ph2004★ 66 cited

The Temperature of the CMB at 10 GHz

D. J. Fixsen, A. Kogut, S. Levin +5

We report the results of an effort to measure the low frequency portion of the spectrum of the Cosmic Microwave Background Radiation (CMB), using a balloon-borne instrument called…

astro-ph2003★ 170 cited

First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors Limits

G. Hinshaw, C. Barnes, C. L. Bennett +14

We describe the calibration and data processing methods used to generate full-sky maps of the cosmic microwave background (CMB) from the first year of Wilkinson Microwave Anisotrop…

astro-ph2003★ 1.2k cited

First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation

H. V. Peiris, E. Komatsu, L. Verde +12

We confront predictions of inflationary scenarios with the WMAP data, in combination with complementary small-scale CMB measurements and large-scale structure data. The WMAP detect…

astro-ph2003★ 304 cited

First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks

L. Page, M. R. Nolta, C. Barnes +12

The CMB has distinct peaks in both its temperature angular power spectrum (TT) and temperature-polarization cross-power spectrum (TE). From the WMAP data we find the first peak in…