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A model of diffuse Galactic radio emission from 10 MHz to 100 GHz
Understanding diffuse Galactic radio emission is interesting both in its own right and for minimizing foreground contamination of cosmological measurements. cosmic microwave background experimentsExpand
Foregrounds and Forecasts for the Cosmic Microwave Background
One of the main challenges facing upcoming cosmic microwave background (CMB) experiments will be to distinguish the cosmological signal from foreground contamination. We present a comprehensiveExpand
High resolution foreground cleaned CMB map from WMAP
We perform an independent foreground analysis of the Wilkinson Microwave Anisotropy Probe (WMAP) maps to produce a cleaned cosmic microwave background (CMB) map (available online) useful forExpand
Significance of the largest scale CMB fluctuations in WMAP
We investigate anomalies reported in the Cosmic Microwave Background maps from the Wilkinson Microwave Anisotropy Probe (WMAP) satellite on very large angular scales and discuss possibleExpand
Properties of Galactic Cirrus Clouds Observed by BOOMERANG
The physical properties of galactic cirrus emission are not well characterized. BOOMERANG is a balloon-borne experiment designed to study the cosmic microwave background at high angular resolution inExpand
A Measurement of the CMB EE Spectrum from the 2003 Flight of BOOMERANG
We report measurements of the CMB polarization power spectra from the 2003 January Antarctic flight of BOOMERANG. The primary results come from 6 days of observation of a patch covering 0.22% of theExpand
A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERANG
We report on observations of the cosmic microwave background (CMB) obtained during the 2003 January flight of BOOMERANG. These results are derived from 195 hr of observation with four 145 GHzExpand
A Measurement of the Polarization-Temperature Angular Cross-Power Spectrum of the Cosmic Microwave Background from the 2003 Flight of BOOMERANG
We present a measurement of the polarization-temperature angular cross power spectra, langTErang and langTBrang, of the cosmic microwave background. The result is based on ~200 hr of data from eightExpand
A 189 MHz, 2400 deg2 Polarization Survey with the Murchison Widefield Array 32-element Prototype
We present a Stokes I , Q and U survey at 189 MHz with the Murchison Widefield Array 32 element prototype covering 2400 deg 2 . The survey has a 15.6 arcmin angular resolution and achieves a noiseExpand
The Cosmic Microwave Background and Its Polarization
The DASI discovery of CMB polarization, confirmed by WMAP, has opened a new chapter in cosmology. Most of the useful information about inflationary gravitational waves and reionization is on largeExpand
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