SPIDER: a balloon-borne CMB polarimeter for large angular scales ...
We describe SPIDER, a balloon-borne instrument to map the polarization of the millimeter-wave sky with degree angular resolution. Spider consists of six monochromatic refracting telescopes, each illuminating a focal plane of large-format antenna-coupled bolometer arrays. A total of 2,624 superconduc...
| Main Authors: | , , , |
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| Format: | Text |
| Language: | English |
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Society of Photo-Optical Instrumentation Engineers (SPIE)
2011
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| Subjects: | |
| Online Access: | https://dx.doi.org/10.14288/1.0107571 https://doi.library.ubc.ca/10.14288/1.0107571 |
| Summary: | We describe SPIDER, a balloon-borne instrument to map the polarization of the millimeter-wave sky with degree angular resolution. Spider consists of six monochromatic refracting telescopes, each illuminating a focal plane of large-format antenna-coupled bolometer arrays. A total of 2,624 superconducting transition-edge sensors are distributed among three observing bands centered at 90, 150, and 280 GHz. A cold half-wave plate at the aperture of each telescope modulates the polarization of incoming light to control systematics. SPIDER's first flight will be a 20-30-day Antarctic balloon campaign in December 2011. This flight will map ~8% of the sky to achieve unprecedented sensitivity to the polarization signature of the gravitational wave background predicted by inflationary cosmology. The SPIDER mission will also serve as a proving ground for these detector technologies in preparation for a future satellite mission. Copyright 2010 Society of Photo-Optical Instrumentation Engineers. One print or electronic ... |
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