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 ∼ 0.03 (at 3σ) in two years of operations.
The Cℓover experiment / 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., et al.. - 7020:(2008). (Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV Marseille, fra ) [10.1117/12.788927].
The Cℓover experiment
Pisano G.;
2008
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 ∼ 0.03 (at 3σ) in two years of operations.| File | Dimensione | Formato | |
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