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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; Lasenby, A; Leahy, P; Leech, J; Lewis, S; Maffei, B; Martinis, L; Mauskopf, P D; Melhuish, S J; North, C E; {O'Dea}, D; Parsley, S; Pisano, G; Reintsema, C D; Savini, G; Sudiwala, R V; Sutton, D; Taylor, A; Teleberg, G; Titterington, D; Tsaneva, V N; Tucker, C; Watson, R; Withington, S; Yassin, G; Zhang, J
In: 2008. p. 35.
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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 {\textasciitilde} 0.03 (at 3??)in two years of operations.
Bibliographic metadata
- 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
- Lasenby, A
- Leahy, P
- Leech, J
- Lewis, S
- Maffei, B
- Martinis, L
- Mauskopf, P D
- Melhuish, S J
- North, C E
- {O'Dea}, D
- Parsley, S
- Pisano, G
- Reintsema, C D
- Savini, G
- Sudiwala, R V
- Sutton, D
- Taylor, A
- Teleberg, G
- Titterington, D
- Tsaneva, V N
- Tucker, C
- Watson, R
- Withington, S
- Yassin, G
- Zhang, J
- Related website http://adsabs.harvard.edu/abs/2008SPIE.7020E..35P