Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiment

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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Main Author: Piat, M
Language:English
Published: 2004
Subjects:
Online Access:http://cds.cern.ch/record/812560
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spelling ftcern:oai:cds.cern.ch:812560 2023-05-15T14:03:11+02:00 Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiment Piat, M 2004-12-22 http://cds.cern.ch/record/812560 eng eng http://cds.cern.ch/record/812560 astro-ph/0412590 oai:cds.cern.ch:812560 Astrophysics and Astronomy 2004 ftcern 2018-07-28T07:06:56Z 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. Other/Unknown Material Antarc* Antarctica CERN Document Server (CDS)
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id ftcern
language English
topic Astrophysics and Astronomy
spellingShingle Astrophysics and Astronomy
Piat, M
Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiment
topic_facet Astrophysics and Astronomy
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.
author Piat, M
author_facet Piat, M
author_sort Piat, M
title Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiment
title_short Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiment
title_full Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiment
title_fullStr Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiment
title_full_unstemmed Precise measurement of CMB polarisation from Dome-C: the BRAIN and CLOVER experiment
title_sort precise measurement of cmb polarisation from dome-c: the brain and clover experiment
publishDate 2004
url http://cds.cern.ch/record/812560
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation http://cds.cern.ch/record/812560
astro-ph/0412590
oai:cds.cern.ch:812560
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