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19942023
most citedSeven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

8.8k citations · 30.3k across the 60 of their papers we have counts for

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astro-ph2008★ 104 cited

A catalog of mid-infrared sources in the Extended Groth Strip

P. Barmby, J. -S. Huang, M. L. N. Ashby +3

The Extended Groth Strip (EGS) is one of the premier fields for extragalactic deep surveys. Deep observations of the EGS with the Infrared Array Camera (IRAC) on the Spitzer Space…

astro-ph2008★ 203 cited

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

B. Gold, C. L. Bennett, R. S. Hill +15

We present a new estimate of foreground emission in the WMAP data, using a Markov chain Monte Carlo (MCMC) method. The new technique delivers maps of each foreground component for…

astro-ph2008★ 352 cited

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra

M. R. Nolta, J. Dunkley, R. S. Hill +17

We present the temperature and polarization angular power spectra of the cosmic microwave background (CMB) derived from the first 5 years of WMAP data. The 5-year temperature (TT)…

astro-ph2008★ 1.7k cited

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data

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

This paper focuses on cosmological constraints derived from analysis of WMAP data alone. A simple LCDM cosmological model fits the five-year WMAP temperature and polarization data.…

astro-ph2008★ 115 cited

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP)Observations: Beam Maps and Window Functions

R. S. Hill, J. L. Weiland, N. Odegard +15

Cosmology and other scientific results from the WMAP mission require an accurate knowledge of the beam patterns in flight. While the degree of beam knowledge for the WMAP one-year…

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…