Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps
Clusters of galaxies produce negative features at wavelengths $\lambda > 1.25$ mm in CMB maps, by means of the thermal SZ effect, while point radio sources produce positive peaks. This fact implies that a distribution of unresolved SZ clusters could be detected using the negative asymmetry introd...
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ftcern:oai:cds.cern.ch:592327 2023-05-15T18:22:24+02:00 Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps Rubiño-Martín, J A Sunyaev, R A 2002-11-19 http://cds.cern.ch/record/592327 eng eng http://cds.cern.ch/record/592327 astro-ph/0211430 oai:cds.cern.ch:592327 Astrophysics and Astronomy 2002 ftcern 2018-07-28T05:46:19Z Clusters of galaxies produce negative features at wavelengths $\lambda > 1.25$ mm in CMB maps, by means of the thermal SZ effect, while point radio sources produce positive peaks. This fact implies that a distribution of unresolved SZ clusters could be detected using the negative asymmetry introduced in the odd-moments of the brightness map (skewness and higher), or in the probability distribution function (PDF) for the fluctuations. This property provides a consistency check to the recent detections from CBI and BIMA experiments of an excess of power at small angular scales, in order to confirm that they are produced by a distribution of unresolved SZ clusters. However it will require at least 1.5 - 2 times more observing time than detection of corresponding power signal. This approach could also be used with the data of the planned SZ experiments (e.g. AMI, AMIBA, APEX, 8 m South Pole telescope). Other/Unknown Material South pole CERN Document Server (CDS) Lambda ENVELOPE(-62.983,-62.983,-64.300,-64.300) South Pole |
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CERN Document Server (CDS) |
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English |
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Astrophysics and Astronomy |
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Astrophysics and Astronomy Rubiño-Martín, J A Sunyaev, R A Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps |
topic_facet |
Astrophysics and Astronomy |
description |
Clusters of galaxies produce negative features at wavelengths $\lambda > 1.25$ mm in CMB maps, by means of the thermal SZ effect, while point radio sources produce positive peaks. This fact implies that a distribution of unresolved SZ clusters could be detected using the negative asymmetry introduced in the odd-moments of the brightness map (skewness and higher), or in the probability distribution function (PDF) for the fluctuations. This property provides a consistency check to the recent detections from CBI and BIMA experiments of an excess of power at small angular scales, in order to confirm that they are produced by a distribution of unresolved SZ clusters. However it will require at least 1.5 - 2 times more observing time than detection of corresponding power signal. This approach could also be used with the data of the planned SZ experiments (e.g. AMI, AMIBA, APEX, 8 m South Pole telescope). |
author |
Rubiño-Martín, J A Sunyaev, R A |
author_facet |
Rubiño-Martín, J A Sunyaev, R A |
author_sort |
Rubiño-Martín, J A |
title |
Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps |
title_short |
Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps |
title_full |
Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps |
title_fullStr |
Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps |
title_full_unstemmed |
Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps |
title_sort |
discriminating between unresolved point sources and "negative" sz clusters in cmb maps |
publishDate |
2002 |
url |
http://cds.cern.ch/record/592327 |
long_lat |
ENVELOPE(-62.983,-62.983,-64.300,-64.300) |
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Lambda South Pole |
geographic_facet |
Lambda South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
http://cds.cern.ch/record/592327 astro-ph/0211430 oai:cds.cern.ch:592327 |
_version_ |
1766201811069304832 |