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SPIDER: a balloon-borne large-scale CMB polarimeter

Crill, B. P., Ade, Peter A. R., Battistelli, E. S., Benton, S., Bihary, R., Bock, J. J., Bond, J. R., Brevik, J., Bryan, S., Contaldi, C. R., Dore, O., Farhang, M., Fissel, L., Golwala, S. R., Halpern, M., Hilton, G., Holmes, W., Hristov, V. V., Irwin, K., Jones, W. C., Kuo, C. L., Lange, A. E., Lawrie, C., MacTavish, C. J., Martin, T. G., Mason, P., Montroy, T. E., Netterfield, C. B., Pascale, Enzo, Riley, D., Ruhl, J. E., Runyan, M. C., Trangsrud, A., Tucker, Carole Elizabeth, Turner, A., Viero, M. and Wiebe, D. 2008. SPIDER: a balloon-borne large-scale CMB polarimeter. Presented at: Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, Marseille, France, 23 June 2008. Space telescopes and instrumentation 2008: optical, infrared, and millimeter : 23-28 June 2008, Marseille, France. Proceedings of SPIE , vol. 7010. Bellingham, WA: SPIE, 70102P. 10.1117/12.787446

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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.

Item Type: Conference or Workshop Item (Paper)
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Publisher: SPIE
ISBN: 0819472204
ISSN: 0277-786X
Last Modified: 04 Jun 2017 04:08

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