The White Mountain Polarimeter Telescope and an Upper Limit on Cosmic Microwave Background Polarization

  • Levy A
  • Leonardi R
  • Ansmann M
  • et al.
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Abstract

The White Mountain Polarimeter (WMPol) is a dedicated ground-based microwave telescope and receiver system for observing polarization of the Cosmic Microwave Background. WMPol is located at an altitude of 3880 meters on a plateau in the White Mountains of Eastern California, USA, at the Barcroft Facility of the University of California White Mountain Research Station. Presented here is a description of the instrument and the data collected during April through October 2004. We set an upper limit on $E$-mode polarization of 14 $\mu\mathrm{K}$ (95% confidence limit) in the multipole range $170

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Levy, A. R., Leonardi, R., Ansmann, M., Bersanelli, M., Childers, J., Cole, T. D., … Wuensche, C. A. (2008). The White Mountain Polarimeter Telescope and an Upper Limit on Cosmic Microwave Background Polarization. The Astrophysical Journal Supplement Series, 177(2), 419–430. https://doi.org/10.1086/588784

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