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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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 |
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English |
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 |
genre |
Antarc* 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. |
_version_ |
1766269154403287040 |