An Instrument for Investigating the Large Angular Scale Polarization of the Cosmic Microwave Background

  • Keating B
  • O’Dell C
  • Gundersen J
  • et al.
18Citations
Citations of this article
11Readers
Mendeley users who have this article in their library.

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.

Cite

CITATION STYLE

APA

Keating, B. G., O’Dell, C. W., Gundersen, J. O., Piccirillo, L., Stebor, N. C., & Timbie, P. T. (2003). An Instrument for Investigating the Large Angular Scale Polarization of the Cosmic Microwave Background. The Astrophysical Journal Supplement Series, 144(1), 1–20. https://doi.org/10.1086/344522

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free