**TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters:
As part of a combined Sunyaev-Zeldovich Effect (SZE), X-ray and weak lensing survey of low redshift (z < 0.1) X-ray clusters, we present SZE images of the z = 0.059 X-ray cluster Abell 3266 at three observing frequencies (150, 220, 275 GHz) and after the spectral subtraction of primary Cosmic Mic...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.256.8371 2023-05-15T18:22:16+02:00 **TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: Percy L. Gómez Kathy A. Romer Jeff Peterson Chris Cantalupo Bill Holzapfel Chao-lin Kuo Matt Newcomb John Ruhl Jon Goldstein Eric Torbet Marcus Runyan The Pennsylvania State University CiteSeerX Archives 2003 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.8371 http://arxiv.org/pdf/astro-ph/0301024v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.8371 http://arxiv.org/pdf/astro-ph/0301024v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0301024v1.pdf text 2003 ftciteseerx 2016-01-07T19:58:53Z As part of a combined Sunyaev-Zeldovich Effect (SZE), X-ray and weak lensing survey of low redshift (z < 0.1) X-ray clusters, we present SZE images of the z = 0.059 X-ray cluster Abell 3266 at three observing frequencies (150, 220, 275 GHz) and after the spectral subtraction of primary Cosmic Microwave Background (CMB) anisotropies. These images were generated using the ACBAR bolometer array operated on the Viper telescope at the South Pole. The multi-frequency data from ACBAR should allow us to overcome one of the main obstacles facing the analysis of SZE observations of nearby clusters, i.e. contamination from primary Cosmic Microwave Background (CMB) anisotropies. 1. Text South pole Unknown South Pole |
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English |
description |
As part of a combined Sunyaev-Zeldovich Effect (SZE), X-ray and weak lensing survey of low redshift (z < 0.1) X-ray clusters, we present SZE images of the z = 0.059 X-ray cluster Abell 3266 at three observing frequencies (150, 220, 275 GHz) and after the spectral subtraction of primary Cosmic Microwave Background (CMB) anisotropies. These images were generated using the ACBAR bolometer array operated on the Viper telescope at the South Pole. The multi-frequency data from ACBAR should allow us to overcome one of the main obstacles facing the analysis of SZE observations of nearby clusters, i.e. contamination from primary Cosmic Microwave Background (CMB) anisotropies. 1. |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Percy L. Gómez Kathy A. Romer Jeff Peterson Chris Cantalupo Bill Holzapfel Chao-lin Kuo Matt Newcomb John Ruhl Jon Goldstein Eric Torbet Marcus Runyan |
spellingShingle |
Percy L. Gómez Kathy A. Romer Jeff Peterson Chris Cantalupo Bill Holzapfel Chao-lin Kuo Matt Newcomb John Ruhl Jon Goldstein Eric Torbet Marcus Runyan **TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: |
author_facet |
Percy L. Gómez Kathy A. Romer Jeff Peterson Chris Cantalupo Bill Holzapfel Chao-lin Kuo Matt Newcomb John Ruhl Jon Goldstein Eric Torbet Marcus Runyan |
author_sort |
Percy L. Gómez |
title |
**TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: |
title_short |
**TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: |
title_full |
**TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: |
title_fullStr |
**TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: |
title_full_unstemmed |
**TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** First Results From an X-ray, Weak Lensing, and Sunyaev-Zeldovich Effect Survey of Nearby Clusters: |
title_sort |
**title** asp conference series, vol. **volume**, **publication year** **editors** first results from an x-ray, weak lensing, and sunyaev-zeldovich effect survey of nearby clusters: |
publishDate |
2003 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.8371 http://arxiv.org/pdf/astro-ph/0301024v1.pdf |
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South Pole |
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South Pole |
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South pole |
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http://arxiv.org/pdf/astro-ph/0301024v1.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.8371 http://arxiv.org/pdf/astro-ph/0301024v1.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766201648110108672 |