Paper
28 September 2004 Measuring the cosmic microwave background polarization with the QUaD experiment
Melanie Bowden, Andy N. Taylor, Ken M. Ganga, Peter A.R. Ade, James J. Bock, Gary A. Cahill, John E. Carlstrom, Sarah E. Church, Walter K. Gear, James R. Hinderks, Wayne Hu, Brian G. Keating, John Kovac, Andrew E. Lange, Erik M. Leitch, Bruno Maffei, Olivier Mallie, Simon J. Melhuish, John Anthony Murphy, Giampaolo Pisano, Lucio Piccirillo, Clem Pryke, Ben A. Rusholme, Creidhe M. O'Sullivan, Keith L. Thompson, Michael Zemcov
Author Affiliations +
Abstract
We look at anticipated science results achievable with QUaD, a ground-based experiment to measure the polarization of the CMB from the South Pole, and describe the features that will enable it to measure this weak polarized signal. We show that QUaD can make a high resolution measurement of the polarization signals on small angular scales. This will lead to tighter constraints on the key cosmological parameters and could also put new limits on the inflationary model.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Melanie Bowden, Andy N. Taylor, Ken M. Ganga, Peter A.R. Ade, James J. Bock, Gary A. Cahill, John E. Carlstrom, Sarah E. Church, Walter K. Gear, James R. Hinderks, Wayne Hu, Brian G. Keating, John Kovac, Andrew E. Lange, Erik M. Leitch, Bruno Maffei, Olivier Mallie, Simon J. Melhuish, John Anthony Murphy, Giampaolo Pisano, Lucio Piccirillo, Clem Pryke, Ben A. Rusholme, Creidhe M. O'Sullivan, Keith L. Thompson, and Michael Zemcov "Measuring the cosmic microwave background polarization with the QUaD experiment", Proc. SPIE 5489, Ground-based Telescopes, (28 September 2004); https://doi.org/10.1117/12.551110
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Cited by 5 scholarly publications.
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KEYWORDS
Polarization

Photons

Anisotropy

Contamination

Electrons

Acoustics

Microwave radiation

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