Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiments
The characterisation of CMB polarisation is one of the next challenge in observationnal cosmology. This is especially true for the so-called B-modes that are at least 3 order of magnitude lower than CMB temperature fluctuations. A precise measurement of the angular power spectrum of these B-modes wi...
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ftdatacite:10.48550/arxiv.astro-ph/0412590 2023-05-15T13:57:28+02:00 Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiments Piat, M. Rosset, C. BRAIN, the Collaboration, CLOVER 2004 https://dx.doi.org/10.48550/arxiv.astro-ph/0412590 https://arxiv.org/abs/astro-ph/0412590 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2004 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0412590 2022-04-01T16:21:00Z The characterisation of CMB polarisation is one of the next challenge in observationnal cosmology. This is especially true for the so-called B-modes that are at least 3 order 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. In this talk, I will 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. : SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004 Text Antarc* Antarctica DataCite Metadata Store (German National Library of Science and Technology) |
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Astrophysics astro-ph FOS Physical sciences |
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Astrophysics astro-ph FOS Physical sciences Piat, M. Rosset, C. BRAIN, the Collaboration, CLOVER Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiments |
topic_facet |
Astrophysics astro-ph FOS Physical sciences |
description |
The characterisation of CMB polarisation is one of the next challenge in observationnal cosmology. This is especially true for the so-called B-modes that are at least 3 order 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. In this talk, I will 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. : SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004 |
format |
Text |
author |
Piat, M. Rosset, C. BRAIN, the Collaboration, CLOVER |
author_facet |
Piat, M. Rosset, C. BRAIN, the Collaboration, CLOVER |
author_sort |
Piat, M. |
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 |
publisher |
arXiv |
publishDate |
2004 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0412590 https://arxiv.org/abs/astro-ph/0412590 |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.astro-ph/0412590 |
_version_ |
1766265141101330432 |