The Princeton IQU Experiment ( PIQUE) and the Cosmic Anisotropy Polarization Mapper ( CAPMAP) are experiments designed to measure the polarization of the cosmic microwave background ( CMB) on sub- degree scales in an area within 1 degrees of the North Celestial Pole using heterodyne correlation polarimeters and off- axis telescopes located in central New Jersey. PIQUE produced the tightest limit on the CMB polarization prior to its detection by DASI, while CAPMAP has recently detected polarization at l similar to 1000. The experimental methods and instrumentation for these two projects are described in detail with emphasis on the particular challenges involved in measuring the tiny polarized component of the CMB.
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Univ Arizona, Dept Phys, Program Appl Math, Tucson, AZ 85721 USA
Univ Arizona, Dept Astron, Tucson, AZ 85721 USAUniv Arizona, Dept Phys, Program Appl Math, Tucson, AZ 85721 USA
Melia, F.
Lopez-Corredoira, M.
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Inst Astrofis Canarias, Tenerife 38205, Spain
Univ La Laguna, Dept Astrofis, E-38206 Tenerife, SpainUniv Arizona, Dept Phys, Program Appl Math, Tucson, AZ 85721 USA
机构:
Univ Arizona, Dept Phys, Program Appl Math, Tucson, AZ 85721 USA
Univ Arizona, Dept Astron, Tucson, AZ 85721 USAUniv Arizona, Dept Phys, Program Appl Math, Tucson, AZ 85721 USA
Melia, F.
Lopez-Corredoira, M.
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h-index: 0
机构:
Inst Astrofis Canarias, Tenerife 38205, Spain
Univ La Laguna, Dept Astrofis, E-38206 Tenerife, SpainUniv Arizona, Dept Phys, Program Appl Math, Tucson, AZ 85721 USA