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CLOVER Experiment

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Title: CLOVER Experiment
Author: Halpern, Mark
Issue Date: 2008
Publicly Available in cIRcle 2011-09-13
Publisher Society of Photo-Optical Instrumentation Engineers
Citation: Piccirillo, Lucio; Ade, Peter A. R.; Audley, Michael D.; Baines, Colin; Battye, Richard A.; Brown, Michael; Calisse, Paolo; Challinor, Anthony; Duncan, William D.; Ferreira, Pedro G.; Gear, Walter K.; Glowacka, Dorota M.; Goldie, David J.; Grimes, Paul K.; Halpern, Mark; Haynes, Victor; Hilton, Gene C.; Irwin, Kent D.; Johnson, Bradley; Jones, Michael; Lasenby, Anthony N.; Leahy, J. Patrick; Leech, Jaimie; Lewis, S.; Maffei, Bruno; Martinis, Lorenzo; Mauskopf, Philip D.; Melhuish, Simon J.; North, Chris E.; O'Dea, Daniel T.; , Parsley, Stephen M.; Pisano, Giampaolo; Reintsema, Carl D.; Savini, Giorgio; Sudiwala, Rashmi V.; Sutton, David; Taylor, Angela: Teleberg, Gustav; Titterington, David J.; Tsaneva, Vassilka N.; Tucker, Carole E.; Watson, Robert A.; Withington, Stafford; Yassin, Ghassan; Zhang, Jin. CLOVER experiment. Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV, edited by William D. Duncan, Wayne S. Holland, Withington, Stafford; Jonas Zmuidzinas, Proceedings of SPIE Volume 7020, 70201E, 2008. http://dx.doi.org/10.1117/12.788927
Abstract: ClOVER is a multi-frequency experiment optimised to measurethe Cosmic Microwave Background (CMB) polarization, inparticular 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 ofcorrugated feed-horns coupled to TES detectors cooled at 100mK. The primary science goal of ClOVER is to be sensitive togravitational waves down to r ~ 0.03 (at 3σ)in two years of operations. 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.
Affiliation: Science, Faculty ofPhysics and Astronomy, Department of
URI: http://hdl.handle.net/2429/37298
Peer Review Status: Reviewed
Scholarly Level: Faculty

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