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The Wilkinson Microwave Anisotropy Probe (WMAP) Source Catalog
E. L. Wright, X. Chen, N. Odegard +18
We present the list of point sources found in the WMAP 5-year maps. The technique used in the first-year and three-year analysis now finds 390 point sources, and the five-year sour…
Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Polarization
A. Kogut, J. Dunkley, C. L. Bennett +14
We present a full-sky model of polarized Galactic microwave emission based on three years of observations by the Wilkinson Microwave Anisotropy Probe (WMAP) at frequencies from 23…
Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
A. Kogut, D. N. Spergel, C. Barnes +10
The Wilkinson Microwave Anisotropy Probe (WMAP) has mapped the full sky in Stokes I, Q, and U parameters at frequencies 23, 33, 41, 61, and 94 GHz. We detect correlations between t…
The MAP satellite mission to map the CMB anisotropy
Lyman Page
The Microwave Anisotropy Probe (MAP) satellite is scheduled to launch in mid-2001. MAP's goal is to produce a map of the anisotropy in the cosmic microwave background of unpreceden…
On Observing The Cosmic Microwave Background
Lyman A. Page
The cosmic microwave background (CMB) comprises the oldest photons in the universe and is arguably our most direct cosmological observable. All precise and accurate measurements of…