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The CℓOVER experiment

Piccirillo, L., Ade, Peter A. R., Audley, M. D., Baines, C., Battye, R., Brown, M., Calisse, Paolo Gherardo, Challinor, A., Duncan, W. D., Ferreira, P., Gear, Walter Kieran, 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, Philip Daniel, Melhuish, S. J., North, Christopher E., O'Dea, D., Parsley, Stephen M., Pisano, G., Reintsema, C. D., Savini, Giorgio, Sudiwala, Rashmikant V., Sutton, D., Taylor, A., Teleberg, Gustav, Titterington, D., Tsaneva, V. N., Tucker, Carole Elizabeth, Watson, R., Withington, S., Yassin, G. and Zhang, Jin 2008. The CℓOVER experiment. Presented at: Millimeter and submillimeter detectors and instrumentation for astronomy IV, Marseille, France, 26-28 June 2008. Published in: Duncan, W. D., Holland, W. S., Withington, S. and Zmuidzinas, S. eds. Millimeter and submillimeter detectors and instrumentation for astronomy IV : 26-28 June 2008, Marseille, France. Proceedings of SPIE , vol. 7020. Bellingham, WA: SPIE, 70201E. 10.1117/12.788927

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CℓOVER is a multi-frequency experiment optimised to measurethe Cosmic Microwave Background (CMB) polarization, inparticular the B-mode component. CℓOVER comprises twoinstruments 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.

Item Type: Conference or Workshop Item (Paper)
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Publisher: SPIE
ISBN: 9780819472304
ISSN: 0277-786X
Last Modified: 31 Jan 2020 08:53

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