An instrument for investigating the large angular scale polarization of the cosmic microwave background

Brian G. Keating, Christopher W. O'Dell, Joshua O. Gundersen, Lucio Piccirillo, Nate C. Stebor, Peter T. Timbie

    Research output: Contribution to journalArticlepeer-review

    Abstract

    We describe the design and performance of a microwave polarimeter used to make precision measurements of polarized astrophysical radiation in three microwave frequency bands spanning 26-36 GHz. The instrument uses cooled HEMT amplifiers in a correlation polarimeter configuration to achieve high sensitivity and long-term stability. The instrument demonstrates long-term stability and has produced the most restrictive upper limits to date on the large angular scale polarization of the 2.7 K cosmic microwave background radiation.
    Original languageEnglish
    Pages (from-to)1-20
    Number of pages19
    JournalASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
    Volume144
    Issue number1
    DOIs
    Publication statusPublished - Jan 2003

    Keywords

    • Cosmic microwave background
    • Cosmology: observations
    • Instrumentation: polarimeters
    • Radio continuum: general

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