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SPIDER: a balloon-borne large-scale CMB polarimeter. Halpern, Mark
Abstract
Spider is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Background over a large fraction of a sky at ~ 1° resolution. Six monochromatic refracting millimeter-wave telescopes with large arrays of antenna-coupled transition-edge superconducting bolometers will provide system sensitivities of 4.2 and 3.1 μKcmb√s at 100 and 150 GHz, respectively. A rotating half-wave plate will modulate the polarization sensitivity of each telescope, controlling systematics. Bolometer arrays operating at 225 GHz and 275 GHz will allow removal of polarized galactic foregrounds. In a 2-6 day first flight from Alice Springs, Australia in 2010, Spider will map 50% of the sky to a depth necessary to improve our knowledge of the reionization optical depth by a large factor. Copyright 2008 Society of Photo-Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
Item Metadata
Title |
SPIDER: a balloon-borne large-scale CMB polarimeter.
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Creator | |
Publisher |
Society of Photo-Optical Instrumentation Engineers (SPIE)
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Date Issued |
2008
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Description |
Spider is a balloon-borne experiment that will measure the polarization of the Cosmic Microwave Background over a large fraction of a sky at ~ 1° resolution. Six
monochromatic refracting millimeter-wave telescopes with large arrays of antenna-coupled transition-edge superconducting bolometers will provide system sensitivities
of 4.2 and 3.1 μKcmb√s at 100 and 150 GHz, respectively. A rotating half-wave plate will modulate the polarization sensitivity of each telescope, controlling
systematics. Bolometer arrays operating at 225 GHz and 275 GHz will allow removal of polarized galactic foregrounds. In a 2-6 day first flight from Alice Springs,
Australia in 2010, Spider will map 50% of the sky to a depth necessary to improve our knowledge of the reionization optical depth by a large factor.
Copyright 2008 Society of Photo-Optical Instrumentation Engineers.
One print or electronic copy may be made for personal use only. Systematic reproduction and distribution,
duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.
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Genre | |
Type | |
Language |
eng
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Date Available |
2011-09-14
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Provider |
Vancouver : University of British Columbia Library
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Rights |
Attribution-NonCommercial-NoDerivatives 4.0 International
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DOI |
10.14288/1.0107594
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URI | |
Affiliation | |
Citation |
Crill, Brendan P.; Ade, Peter A. R.; Battistelli, Elia S.; Benton, Steven J.; Bihary, Richard; Bock, James J.; Bond, J. Richard; Brevik, Justus A.; Bryan, Sean A.; Contaldi, Carlo R.; Dore, Olivier; Farhang, Marzieh; Fissel, Laura M.; Golwala, Sunil R.; Halpern, Mark; Hilton, Gene C.; Holmes, Warren; Hristov, Viktor V.; Irwin, Kent D.; Jones, William C; Kuo, Chao Lin; Lange, Andrew E.; Lawrie, Craig; MacTavish, Carrie J.; Martin, Taylor G.; Mason, Peter V.; Montory, Thomas E.; Netterfield, C. Barth; Pascale, Enzo; Riley, D.; Ruhl, John E.; Runyan, Marcus C.; Trangsrud, Amy R.; Tucker, Carole E.; Turner, Anthony D.; Viero, Marco P.; Wiebe, Donald V. SPIDER: a balloon-borne large-scale CMB polarimeter. Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, edited by Jacobus M. Oschmann, Jr., Mattheus W. M. de Graauw, Howard A. MacEwen Proceedings of SPIE Volume 7010, 70102P, 2008.
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Publisher DOI |
10.1117/12.787446
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Peer Review Status |
Reviewed
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Scholarly Level |
Faculty
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Copyright Holder |
Halpern, Mark
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Rights URI | |
Aggregated Source Repository |
DSpace
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Item Media
Item Citations and Data
Rights
Attribution-NonCommercial-NoDerivatives 4.0 International