Imaging the Sunyaev Zel’dovich Effect using ACBAR on Viper
During 2001 and 2002, observations of several X-ray bright clusters of galaxies were conducted using the ACBAR Bolometer Array on the South Pole Viper telescope. A multifrequency analysis of these clusters is currently underway. This multi-frequency analysis includes 150, 220 and 275 GHz data from A...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.257.90 2023-05-15T18:22:12+02:00 Imaging the Sunyaev Zel’dovich Effect using ACBAR on Viper A. Oemler (pasadena A. K. Romer P. L. Gomez The Acbar Collaboration The Pennsylvania State University CiteSeerX Archives 2003 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.257.90 http://arxiv.org/pdf/astro-ph/0311261v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.257.90 http://arxiv.org/pdf/astro-ph/0311261v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0311261v1.pdf text 2003 ftciteseerx 2016-01-07T20:01:49Z During 2001 and 2002, observations of several X-ray bright clusters of galaxies were conducted using the ACBAR Bolometer Array on the South Pole Viper telescope. A multifrequency analysis of these clusters is currently underway. This multi-frequency analysis includes 150, 220 and 275 GHz data from ACBAR, X-ray imaging and spectroscopy from Chandra and XMM-Newton, and weak lensing data from the CTIO 4m Blanco telescope. We describe here how ACBAR can be used to create fully sampled cluster images and present such images for four of the clusters in our sample; Abell 3266, Abell 3827, Abell S1063 and 1E0657-56. In these images, the Sunyaev-Zel’dovich Effect is clearly detected. Text South pole Unknown Blanco ENVELOPE(-55.233,-55.233,-61.250,-61.250) South Pole |
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ftciteseerx |
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English |
description |
During 2001 and 2002, observations of several X-ray bright clusters of galaxies were conducted using the ACBAR Bolometer Array on the South Pole Viper telescope. A multifrequency analysis of these clusters is currently underway. This multi-frequency analysis includes 150, 220 and 275 GHz data from ACBAR, X-ray imaging and spectroscopy from Chandra and XMM-Newton, and weak lensing data from the CTIO 4m Blanco telescope. We describe here how ACBAR can be used to create fully sampled cluster images and present such images for four of the clusters in our sample; Abell 3266, Abell 3827, Abell S1063 and 1E0657-56. In these images, the Sunyaev-Zel’dovich Effect is clearly detected. |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
A. Oemler (pasadena A. K. Romer P. L. Gomez The Acbar Collaboration |
spellingShingle |
A. Oemler (pasadena A. K. Romer P. L. Gomez The Acbar Collaboration Imaging the Sunyaev Zel’dovich Effect using ACBAR on Viper |
author_facet |
A. Oemler (pasadena A. K. Romer P. L. Gomez The Acbar Collaboration |
author_sort |
A. Oemler (pasadena |
title |
Imaging the Sunyaev Zel’dovich Effect using ACBAR on Viper |
title_short |
Imaging the Sunyaev Zel’dovich Effect using ACBAR on Viper |
title_full |
Imaging the Sunyaev Zel’dovich Effect using ACBAR on Viper |
title_fullStr |
Imaging the Sunyaev Zel’dovich Effect using ACBAR on Viper |
title_full_unstemmed |
Imaging the Sunyaev Zel’dovich Effect using ACBAR on Viper |
title_sort |
imaging the sunyaev zel’dovich effect using acbar on viper |
publishDate |
2003 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.257.90 http://arxiv.org/pdf/astro-ph/0311261v1.pdf |
long_lat |
ENVELOPE(-55.233,-55.233,-61.250,-61.250) |
geographic |
Blanco South Pole |
geographic_facet |
Blanco South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
http://arxiv.org/pdf/astro-ph/0311261v1.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.257.90 http://arxiv.org/pdf/astro-ph/0311261v1.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766201578272849920 |