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The ClOVER Experiment - art. no. 70201E

Piccirillo, L; Ade, P; Audley, M D; Baines, C; Battye, R; Brown, M; Calisse, P; Challinor, A; Duncan, W D; Ferreira, P; Gear, W; Glowacka, D M; Goldie, D; Grimes, P K; Halpern, M; Haynes, V; Hilton, G C; Irwin, K D; Johnson, B; Jones, M; Lasenby, A; Leahy, P; Leech, J; Lewis, S; Maffei, B; Martinis, L; Mauskopf, P D; Melhuish, S J; North, C E; O'Dea, D; Parsley, S; Pisano, G; Reintsema, C D; Savini, G; Sudiwala, R V; Sutton, D; Taylor, A; Teleberg, G; Titterington, D; Tsaneva, V N; Tucker, C; Watson, R; Withington, S; Yassin, G; Zhang, J

In: Duncan, W D; Holland, W S; Withington, S; Zmuidzinas, J. Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astonomy IV: Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astonomy IV; 26 Jun 2008-28 Jun 2008; Marseille, FRANCE. Spie-Int Soc Optical Engineering; 2008. p. E201-E201.

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Abstract

ClOVER is a multi-frequency experiment optimised to measure the Cosmic Microwave Background (CMB) polarization, in particular the B-mode component. ClOVER comprises two instruments observing respectively at 97 GHz and 150/225 GHz. The focal plane of both instruments consists of an array of corrugated feed-horns coupled to TES detectors cooled at 100 mK. The primary science goal of ClOVER is to be sensitive to gravitational waves down to r similar to 0.03 (at 3 sigma) in two years of operations.

Bibliographic metadata

Content type:
Type of conference contribution:
Conference contribution title:
Publication date:
Conference title:
Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astonomy IV
Conference venue:
Marseille, FRANCE
Conference start date:
2008-06-26
Conference end date:
2008-06-28
Proceedings start page:
E201-E201
Proceedings pagination:
E201-E201-
Abstract:
ClOVER is a multi-frequency experiment optimised to measure the Cosmic Microwave Background (CMB) polarization, in particular the B-mode component. ClOVER comprises two instruments observing respectively at 97 GHz and 150/225 GHz. The focal plane of both instruments consists of an array of corrugated feed-horns coupled to TES detectors cooled at 100 mK. The primary science goal of ClOVER is to be sensitive to gravitational waves down to r similar to 0.03 (at 3 sigma) in two years of operations.
Digtial Object Identifier:
10.1117/12.788927
Proceedings' ISBN:
0277-786X 978-0-8194-7230-4
Proceedings' volume:
7020
Language:
english
General notes:
  • Spie, Spie Europe Piccirillo, L. Ade, P. Audley, M. D. Baines, C. Battye, R. Brown, M. Calisse, P. Challinor, A. Duncan, W. D. Ferreira, P. Gear, W. Glowacka, D. M. Goldie, D. Grimes, P. K. Halpern, M. Haynes, V. Hilton, G. C. Irwin, K. D. Johnson, B. Jones, M. Lasenby, A. Leahy, P. Leech, J. Lewis, S. Maffei, B. Martinis, L. Mauskopf, P. D. Melhuish, S. J. North, C. E. O'Dea, D. Parsley, S. Pisano, G. Reintsema, C. D. Savini, G. Sudiwala, R. V. Sutton, D. Taylor, A. Teleberg, G. Titterington, D. Tsaneva, V. N. Tucker, C. Watson, R. Withington, S. Yassin, G. Zhang, J. 20 BELLINGHAM BIR58

Record metadata

Manchester eScholar ID:
uk-ac-man-scw:2f28
Created:
7th September, 2009, 15:27:04
Last modified by:
Leahy, John
Last modified:
5th January, 2016, 22:43:12

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