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The CℓOVER experiment

Piccirillo, L., Ade, Peter A. R. ORCID:, Audley, M. D., Baines, C., Battye, R., Brown, M., Calisse, Paolo Gherardo, Challinor, A., Duncan, W. D., Ferreira, P., Gear, Walter Kieran ORCID:, 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 ORCID:, Melhuish, S. J., North, Christopher E., O'Dea, D., Parsley, Stephen M., Pisano, G., Reintsema, C. D., Savini, Giorgio, Sudiwala, Rashmikant V. ORCID:, Sutton, D., Taylor, A., Teleberg, Gustav, Titterington, D., Tsaneva, V. N., Tucker, Carole Elizabeth ORCID:, 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 (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: 07 Feb 2023 16:27

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