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.
- Zhang, Jin
DOIAbstract
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
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