We present a new, fully-funded ground-based instrument designed to measure the B-mode polarization of the Cosmic Microwave Background (CMB). The concept is based on three independent sub-systems operating at 90, 150 and 220 GHz, each comprising a telescope and a focal plane of horn-coupled background-limited bolometers. This highly-sensitive experiment, planned to be based at Dome C station in Antarctica, is optimised to produce very low systematic effects. It will allow the detection of the CMB polarization over angular multipoles 20 < l < 1000 accurately enough to measure the B-mode signature from gravitational waves to a lensing-confusion-limited tensor-to-scalar ratio r ∼ 0.005. © EAS, EDP Sciences 2005.

CLOVER: The CMB polarization observer / Maffei, B.; Ade, P. A. R.; Calderon, C.; Challinor, A. D.; De Bernardis, P.; Dunlop, L.; Gear, W. K.; Giraud-Heraud, Y.; Goldie, D. J.; Grainge, K. J. B.; Isaak, K. G.; Johnson, B.; Jones, M. E.; Lasenby, A. N.; Mauskopf, P. D.; Melhuish, S. J.; Orlando, A.; Piccirillo, L.; Pisano, G.; Taylor, A. C.; Withington, S.; Yassin, G.. - 14:(2005), pp. 251-256. (Intervento presentato al convegno Dome C Astronomy and Astrophysics Meeting tenutosi a Toulouse, fra) [10.1051/eas:2005039].

CLOVER: The CMB polarization observer

De Bernardis P.;Pisano G.;
2005

Abstract

We present a new, fully-funded ground-based instrument designed to measure the B-mode polarization of the Cosmic Microwave Background (CMB). The concept is based on three independent sub-systems operating at 90, 150 and 220 GHz, each comprising a telescope and a focal plane of horn-coupled background-limited bolometers. This highly-sensitive experiment, planned to be based at Dome C station in Antarctica, is optimised to produce very low systematic effects. It will allow the detection of the CMB polarization over angular multipoles 20 < l < 1000 accurately enough to measure the B-mode signature from gravitational waves to a lensing-confusion-limited tensor-to-scalar ratio r ∼ 0.005. © EAS, EDP Sciences 2005.
2005
Dome C Astronomy and Astrophysics Meeting
Cosmic Microwave Background radiation, B-Modes, Instrumentation, Polarimetry, Millimetre waves, Microwave receivers, Polarization
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
CLOVER: The CMB polarization observer / Maffei, B.; Ade, P. A. R.; Calderon, C.; Challinor, A. D.; De Bernardis, P.; Dunlop, L.; Gear, W. K.; Giraud-Heraud, Y.; Goldie, D. J.; Grainge, K. J. B.; Isaak, K. G.; Johnson, B.; Jones, M. E.; Lasenby, A. N.; Mauskopf, P. D.; Melhuish, S. J.; Orlando, A.; Piccirillo, L.; Pisano, G.; Taylor, A. C.; Withington, S.; Yassin, G.. - 14:(2005), pp. 251-256. (Intervento presentato al convegno Dome C Astronomy and Astrophysics Meeting tenutosi a Toulouse, fra) [10.1051/eas:2005039].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1585918
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