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Modulation of cosmic microwave background polarization with a warm rapidly rotating half-wave plate on the Atacama B-Mode Search instrument.
Kusaka, A; Essinger-Hileman, T; Appel, J W; Gallardo, P; Irwin, K D; Jarosik, N; Nolta, M R; Page, L A; Parker, L P; Raghunathan, S; Sievers, J L; Simon, S M; Staggs, S T; Visnjic, K.
Affiliation
  • Kusaka A; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
  • Essinger-Hileman T; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
  • Appel JW; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
  • Gallardo P; Department of Physics, Cornell University, Ithaca, New York 14853, USA.
  • Irwin KD; National Institute of Standards and Technology, 325 Broadway MC 817.03, Boulder, Colorado 80305, USA and Department of Physics, Stanford University, Stanford, California 94305, USA.
  • Jarosik N; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
  • Nolta MR; The Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario M5S 3H8, Canada.
  • Page LA; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
  • Parker LP; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
  • Raghunathan S; Department of Astronomy, Universidad de Chile, Santiago, Chile.
  • Sievers JL; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
  • Simon SM; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
  • Staggs ST; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
  • Visnjic K; Department of Physics, Princeton University, Princeton, New Jersey 08544, USA.
Rev Sci Instrum ; 85(2): 024501, 2014 Feb.
Article in En | MEDLINE | ID: mdl-24593374
ABSTRACT
We evaluate the modulation of cosmic microwave background polarization using a rapidly rotating, half-wave plate (HWP) on the Atacama B-Mode Search. After demodulating the time-ordered-data (TOD), we find a significant reduction of atmospheric fluctuations. The demodulated TOD is stable on time scales of 500-1000 s, corresponding to frequencies of 1-2 mHz. This facilitates recovery of cosmological information at large angular scales, which are typically available only from balloon-borne or satellite experiments. This technique also achieves a sensitive measurement of celestial polarization without differencing the TOD of paired detectors sensitive to two orthogonal linear polarizations. This is the first demonstration of the ability to remove atmospheric contamination at these levels from a ground-based platform using a rapidly rotating HWP.

Full text: 1 Database: MEDLINE Language: En Journal: Rev Sci Instrum Year: 2014 Type: Article Affiliation country: United States

Full text: 1 Database: MEDLINE Language: En Journal: Rev Sci Instrum Year: 2014 Type: Article Affiliation country: United States