The CMB Polarization Observer (CLOVER)
We describe the design and performance of a new fully-funded instrument, CLOVER, to measure the B-mode polarization of the cosmic microwave background. The instrument comprises three independent telescopes operating at 90, 150 and 220 GHz and is planned to be sited at Dome C, Antartica. Each telesco...
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ftunivromairis:oai:iris.uniroma1.it:11573/1586207 2023-11-05T03:37:12+01:00 The CMB Polarization Observer (CLOVER) Yassin, G. Ade, P. A. R. Calderon, C. Challinor, A. D. Dunlop, L. Gear, W. K. Goldie, D. J. Grainge, K. J. B. Griffin, M. J. Jones, M. E. Lasenby, A. N. Maffei, B. Mauskopf, P. D. Melhuish, S. J. Orlando, A. Piccirillo, L. Pisano, G. Taylor, A. C. Withington, S. Yassin, G. Ade, P. A. R. Calderon, C. Challinor, A. D. Dunlop, L. Gear, W. K. Goldie, D. J. Grainge, K. J. B. Griffin, M. J. Jones, M. E. Lasenby, A. N. Maffei, B. Mauskopf, P. D. Melhuish, S. J. Orlando, A. Piccirillo, L. Pisano, G. Taylor, A. C. Withington, S. 2004 http://hdl.handle.net/11573/1586207 eng eng ispartofbook:Fifteenth International Symposium on Space Terahertz Technology Fifteenth International Symposium on Space Terahertz Technology http://hdl.handle.net/11573/1586207 Cosmic Microwave Background radiation B-Modes Instrumentation Polarimetry Millimetre waves info:eu-repo/semantics/conferenceObject 2004 ftunivromairis 2023-10-11T17:14:17Z We describe the design and performance of a new fully-funded instrument, CLOVER, to measure the B-mode polarization of the cosmic microwave background. The instrument comprises three independent telescopes operating at 90, 150 and 220 GHz and is planned to be sited at Dome C, Antartica. Each telescope will fed by a focal plane array of 256 horns with background limited detectors and will measure the polarization signal over angular multipoles 20< /<1000. The unique design of the telescope and extremely low systematics should enable the B-mode signature from gravitational waves to be measured, or constrained to a lensing confusing limited tensor-to-scalar ratio r 0.005. Conference Object antartic* Sapienza Università di Roma: CINECA IRIS |
institution |
Open Polar |
collection |
Sapienza Università di Roma: CINECA IRIS |
op_collection_id |
ftunivromairis |
language |
English |
topic |
Cosmic Microwave Background radiation B-Modes Instrumentation Polarimetry Millimetre waves |
spellingShingle |
Cosmic Microwave Background radiation B-Modes Instrumentation Polarimetry Millimetre waves Yassin, G. Ade, P. A. R. Calderon, C. Challinor, A. D. Dunlop, L. Gear, W. K. Goldie, D. J. Grainge, K. J. B. Griffin, M. J. Jones, M. E. Lasenby, A. N. Maffei, B. Mauskopf, P. D. Melhuish, S. J. Orlando, A. Piccirillo, L. Pisano, G. Taylor, A. C. Withington, S. The CMB Polarization Observer (CLOVER) |
topic_facet |
Cosmic Microwave Background radiation B-Modes Instrumentation Polarimetry Millimetre waves |
description |
We describe the design and performance of a new fully-funded instrument, CLOVER, to measure the B-mode polarization of the cosmic microwave background. The instrument comprises three independent telescopes operating at 90, 150 and 220 GHz and is planned to be sited at Dome C, Antartica. Each telescope will fed by a focal plane array of 256 horns with background limited detectors and will measure the polarization signal over angular multipoles 20< /<1000. The unique design of the telescope and extremely low systematics should enable the B-mode signature from gravitational waves to be measured, or constrained to a lensing confusing limited tensor-to-scalar ratio r 0.005. |
author2 |
Yassin, G. Ade, P. A. R. Calderon, C. Challinor, A. D. Dunlop, L. Gear, W. K. Goldie, D. J. Grainge, K. J. B. Griffin, M. J. Jones, M. E. Lasenby, A. N. Maffei, B. Mauskopf, P. D. Melhuish, S. J. Orlando, A. Piccirillo, L. Pisano, G. Taylor, A. C. Withington, S. |
format |
Conference Object |
author |
Yassin, G. Ade, P. A. R. Calderon, C. Challinor, A. D. Dunlop, L. Gear, W. K. Goldie, D. J. Grainge, K. J. B. Griffin, M. J. Jones, M. E. Lasenby, A. N. Maffei, B. Mauskopf, P. D. Melhuish, S. J. Orlando, A. Piccirillo, L. Pisano, G. Taylor, A. C. Withington, S. |
author_facet |
Yassin, G. Ade, P. A. R. Calderon, C. Challinor, A. D. Dunlop, L. Gear, W. K. Goldie, D. J. Grainge, K. J. B. Griffin, M. J. Jones, M. E. Lasenby, A. N. Maffei, B. Mauskopf, P. D. Melhuish, S. J. Orlando, A. Piccirillo, L. Pisano, G. Taylor, A. C. Withington, S. |
author_sort |
Yassin, G. |
title |
The CMB Polarization Observer (CLOVER) |
title_short |
The CMB Polarization Observer (CLOVER) |
title_full |
The CMB Polarization Observer (CLOVER) |
title_fullStr |
The CMB Polarization Observer (CLOVER) |
title_full_unstemmed |
The CMB Polarization Observer (CLOVER) |
title_sort |
cmb polarization observer (clover) |
publishDate |
2004 |
url |
http://hdl.handle.net/11573/1586207 |
genre |
antartic* |
genre_facet |
antartic* |
op_relation |
ispartofbook:Fifteenth International Symposium on Space Terahertz Technology Fifteenth International Symposium on Space Terahertz Technology http://hdl.handle.net/11573/1586207 |
_version_ |
1781692778716069888 |