activity
20082014
most citedFive-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

5.7k citations · 8.5k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2014★ 34 cited

Comparing Planck and WMAP: Maps, Spectra, and Parameters

D. Larson, J. L. Weiland, G. Hinshaw +1

We examine the consistency of WMAP9 and Planck data. We compare sky maps, power spectra, and inferred LCDM cosmological parameters. Residual dipoles are seen in the WMAP and Planck…

astro-ph.CO2014★ 427 cited

The 1% Concordance Hubble Constant

C. L. Bennett, D. Larson, J. L. Weiland +1

The determination of the Hubble constant has been a central goal in observational astrophysics for nearly 100 years. Extraordinary progress has occurred in recent years on two fron…

astro-ph.GA2010★ 447 cited

Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission

B. Gold, N. Odegard, J. L. Weiland +19

[Abridged] We present updated estimates of Galactic foreground emission using seven years of WMAP data. Using the power spectrum of differences between multi-frequency template-cle…

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-ph2008★ 5.7k cited

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

E. Komatsu, J. Dunkley, M. R. Nolta +16

(Abridged) The WMAP 5-year data strongly limit deviations from the minimal LCDM model. We constrain the physics of inflation via Gaussianity, adiabaticity, the power spectrum shape…