Measuring the cosmic microwave background polarization with the QUaD experiment

M. Bowden, A. N. Taylor, K. M. Ganga, P. A R Ade, J. J. Bock, G. Cahill, J. E. Carlstrom, S. E. Church, W. K. Gear, J. R. Hinderks, W. Hu, B. Keating, J. Kovac, A. E. Lange, E. M. Leitch, B. Maffei, O. Mallie, S. J. Melhuish, J. A. Murphy, G. PisanoL. Piccirillo, C. Pryke, B. A. Rusholme, C. O'Sullivan, K. Thompson, M. Zemcov

    Research output: Contribution to journalArticlepeer-review

    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.
    Original languageEnglish
    Pages (from-to)84-94
    Number of pages10
    JournalProceedings of SPIE - The International Society for Optical Engineering
    Volume5489
    Issue number1
    DOIs
    Publication statusPublished - 2004

    Keywords

    • Cosmic microwave background
    • Cosmology
    • Polarization
    • Sub-mm telescope

    Fingerprint

    Dive into the research topics of 'Measuring the cosmic microwave background polarization with the QUaD experiment'. Together they form a unique fingerprint.

    Cite this