Paper
15 July 2010 Q/U Imaging Experiment (QUIET): a ground-based probe of cosmic microwave background polarization
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Abstract
QUIET is an experimental program to measure the polarization of the Cosmic Microwave Background (CMB) radiation from the ground. Previous CMB polarization data have been used to constrain the cosmological parameters that model the history of our universe. The exciting target for current and future experiments is detecting and measuring the faint polarization signals caused by gravity waves from the inflationary epoch which occurred < 10-30 s after the Big Bang. QUIET has finished an observing season at 44 GHz (Q-Band); observing at 95 GHz (W-Band) is ongoing. The instrument incorporates several technologies and approaches novel to CMB experiments. We describe the observing strategy, optics design, detector technology, and data acquisition. These systems combine to produce a polarization sensitivity of 64 (57) μK for a 1 s exposure of the Phase I Q (W) Band array. We describe the QUIET Phase I instrument and explain how systematic errors are reduced and quantified.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Immanuel Buder "Q/U Imaging Experiment (QUIET): a ground-based probe of cosmic microwave background polarization", Proc. SPIE 7741, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V, 77411D (15 July 2010); https://doi.org/10.1117/12.857882
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Cited by 15 scholarly publications.
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KEYWORDS
Polarization

Sensors

Modulation

Calibration

Phase shift keying

Telescopes

Microwave radiation

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