PRECISE MEASUREMENT OF CMB POLARISATION FROM DOME-C: THE BRAIN AND CLOVER EXPERIMENTS

collaboration 2 Abstract. The characterisation of CMB polarisation is one of the next challenges in observational cosmology. This is especially true for the so-called B-modes that are at least 3 orders of magnitude lower than CMB temperature fluctuations. A precise measurement of the angular power s...

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Main Authors: F. Combes, D. Barret, T. Contini, F. Meynadier, L. Pagani (eds
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2004
Subjects:
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.316.6830
http://arxiv.org/pdf/astro-ph/0412590v1.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.316.6830 2023-05-15T14:00:10+02:00 PRECISE MEASUREMENT OF CMB POLARISATION FROM DOME-C: THE BRAIN AND CLOVER EXPERIMENTS F. Combes D. Barret T. Contini F. Meynadier L. Pagani (eds The Pennsylvania State University CiteSeerX Archives 2004 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.316.6830 http://arxiv.org/pdf/astro-ph/0412590v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.316.6830 http://arxiv.org/pdf/astro-ph/0412590v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0412590v1.pdf text 2004 ftciteseerx 2016-09-04T00:08:16Z collaboration 2 Abstract. The characterisation of CMB polarisation is one of the next challenges in observational cosmology. This is especially true for the so-called B-modes that are at least 3 orders of magnitude lower than CMB temperature fluctuations. A precise measurement of the angular power spectrum of these B-modes will give important constraints on inflation parameters. We describe two complementary experiments, BRAIN and CLOVER, dedicated to CMB polarisation measurement. These experiments are proposed to be installed in Dome-C, Antarctica, to take advantage of the extreme dryness of the atmosphere and to allow long integration time. 1 Text Antarc* Antarctica Unknown
institution Open Polar
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op_collection_id ftciteseerx
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description collaboration 2 Abstract. The characterisation of CMB polarisation is one of the next challenges in observational cosmology. This is especially true for the so-called B-modes that are at least 3 orders of magnitude lower than CMB temperature fluctuations. A precise measurement of the angular power spectrum of these B-modes will give important constraints on inflation parameters. We describe two complementary experiments, BRAIN and CLOVER, dedicated to CMB polarisation measurement. These experiments are proposed to be installed in Dome-C, Antarctica, to take advantage of the extreme dryness of the atmosphere and to allow long integration time. 1
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author F. Combes
D. Barret
T. Contini
F. Meynadier
L. Pagani (eds
spellingShingle F. Combes
D. Barret
T. Contini
F. Meynadier
L. Pagani (eds
PRECISE MEASUREMENT OF CMB POLARISATION FROM DOME-C: THE BRAIN AND CLOVER EXPERIMENTS
author_facet F. Combes
D. Barret
T. Contini
F. Meynadier
L. Pagani (eds
author_sort F. Combes
title PRECISE MEASUREMENT OF CMB POLARISATION FROM DOME-C: THE BRAIN AND CLOVER EXPERIMENTS
title_short PRECISE MEASUREMENT OF CMB POLARISATION FROM DOME-C: THE BRAIN AND CLOVER EXPERIMENTS
title_full PRECISE MEASUREMENT OF CMB POLARISATION FROM DOME-C: THE BRAIN AND CLOVER EXPERIMENTS
title_fullStr PRECISE MEASUREMENT OF CMB POLARISATION FROM DOME-C: THE BRAIN AND CLOVER EXPERIMENTS
title_full_unstemmed PRECISE MEASUREMENT OF CMB POLARISATION FROM DOME-C: THE BRAIN AND CLOVER EXPERIMENTS
title_sort precise measurement of cmb polarisation from dome-c: the brain and clover experiments
publishDate 2004
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.316.6830
http://arxiv.org/pdf/astro-ph/0412590v1.pdf
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Antarctica
genre_facet Antarc*
Antarctica
op_source http://arxiv.org/pdf/astro-ph/0412590v1.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.316.6830
http://arxiv.org/pdf/astro-ph/0412590v1.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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