Edge Detection, Cosmic Strings and the South Pole Telescope
We develop a method of constraining the cosmic string tension $Gμ$ which uses the Canny edge detection algorithm as a means of searching CMB temperature maps for the signature of the Kaiser-Stebbins effect. We test the potential of this method using high resolution, simulated CMB temperature maps. B...
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ftdatacite:10.48550/arxiv.0809.0865 2023-05-15T18:21:51+02:00 Edge Detection, Cosmic Strings and the South Pole Telescope Stewart, Andrew Brandenberger, Robert 2008 https://dx.doi.org/10.48550/arxiv.0809.0865 https://arxiv.org/abs/0809.0865 unknown arXiv https://dx.doi.org/10.1088/1475-7516/2009/02/009 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2008 ftdatacite https://doi.org/10.48550/arxiv.0809.0865 https://doi.org/10.1088/1475-7516/2009/02/009 2022-04-01T15:21:54Z We develop a method of constraining the cosmic string tension $Gμ$ which uses the Canny edge detection algorithm as a means of searching CMB temperature maps for the signature of the Kaiser-Stebbins effect. We test the potential of this method using high resolution, simulated CMB temperature maps. By modeling the future output from the South Pole Telescope project (including anticipated instrumental noise), we find that cosmic strings with $Gμ> 5.5\times10^{-8}$ could be detected. : 27 pages, 5 figures, reference and minor notes added, discussion of noise expanded, explanation of equation (4) expanded Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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DataCite Metadata Store (German National Library of Science and Technology) |
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ftdatacite |
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unknown |
topic |
Astrophysics astro-ph FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph FOS Physical sciences Stewart, Andrew Brandenberger, Robert Edge Detection, Cosmic Strings and the South Pole Telescope |
topic_facet |
Astrophysics astro-ph FOS Physical sciences |
description |
We develop a method of constraining the cosmic string tension $Gμ$ which uses the Canny edge detection algorithm as a means of searching CMB temperature maps for the signature of the Kaiser-Stebbins effect. We test the potential of this method using high resolution, simulated CMB temperature maps. By modeling the future output from the South Pole Telescope project (including anticipated instrumental noise), we find that cosmic strings with $Gμ> 5.5\times10^{-8}$ could be detected. : 27 pages, 5 figures, reference and minor notes added, discussion of noise expanded, explanation of equation (4) expanded |
format |
Text |
author |
Stewart, Andrew Brandenberger, Robert |
author_facet |
Stewart, Andrew Brandenberger, Robert |
author_sort |
Stewart, Andrew |
title |
Edge Detection, Cosmic Strings and the South Pole Telescope |
title_short |
Edge Detection, Cosmic Strings and the South Pole Telescope |
title_full |
Edge Detection, Cosmic Strings and the South Pole Telescope |
title_fullStr |
Edge Detection, Cosmic Strings and the South Pole Telescope |
title_full_unstemmed |
Edge Detection, Cosmic Strings and the South Pole Telescope |
title_sort |
edge detection, cosmic strings and the south pole telescope |
publisher |
arXiv |
publishDate |
2008 |
url |
https://dx.doi.org/10.48550/arxiv.0809.0865 https://arxiv.org/abs/0809.0865 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1088/1475-7516/2009/02/009 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.0809.0865 https://doi.org/10.1088/1475-7516/2009/02/009 |
_version_ |
1766201176169119744 |