Correlation of the South Pole 94 data with 100microns and 408 MHz maps

We present a correlation between the ACME/SP94 CMB anisotropy data at 25 to 45 GHz with the IRAS/DIRBE data and the Haslam 408 MHz data. We find a marginal correlation between the dust and the Q-band CMB data but none between the CMB data and the Haslam map. While the amplitude of the correlation wi...

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Main Authors: Hamilton, J. -Ch., Ganga, K. M.
Format: Text
Language:unknown
Published: arXiv 2001
Subjects:
Astrophysics astro-ph
FOS Physical sciences
South Pole
South pole
Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0101131
https://arxiv.org/abs/astro-ph/0101131
id ftdatacite:10.48550/arxiv.astro-ph/0101131
record_format openpolar
spelling ftdatacite:10.48550/arxiv.astro-ph/0101131 2023-05-15T18:22:07+02:00 Correlation of the South Pole 94 data with 100microns and 408 MHz maps Hamilton, J. -Ch. Ganga, K. M. 2001 https://dx.doi.org/10.48550/arxiv.astro-ph/0101131 https://arxiv.org/abs/astro-ph/0101131 unknown arXiv https://dx.doi.org/10.1051/0004-6361:20010061 Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2001 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0101131 https://doi.org/10.1051/0004-6361:20010061 2022-04-01T17:04:18Z We present a correlation between the ACME/SP94 CMB anisotropy data at 25 to 45 GHz with the IRAS/DIRBE data and the Haslam 408 MHz data. We find a marginal correlation between the dust and the Q-band CMB data but none between the CMB data and the Haslam map. While the amplitude of the correlation with the dust is larger than that expected from naive models of dust emission it does not dominate the sky emission. : 6 pages, 4 figures. Accepted for publication in Astronomy and Astrophysics Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
Hamilton, J. -Ch.
Ganga, K. M.
Correlation of the South Pole 94 data with 100microns and 408 MHz maps
topic_facet Astrophysics astro-ph
FOS Physical sciences
description We present a correlation between the ACME/SP94 CMB anisotropy data at 25 to 45 GHz with the IRAS/DIRBE data and the Haslam 408 MHz data. We find a marginal correlation between the dust and the Q-band CMB data but none between the CMB data and the Haslam map. While the amplitude of the correlation with the dust is larger than that expected from naive models of dust emission it does not dominate the sky emission. : 6 pages, 4 figures. Accepted for publication in Astronomy and Astrophysics
format Text
author Hamilton, J. -Ch.
Ganga, K. M.
author_facet Hamilton, J. -Ch.
Ganga, K. M.
author_sort Hamilton, J. -Ch.
title Correlation of the South Pole 94 data with 100microns and 408 MHz maps
title_short Correlation of the South Pole 94 data with 100microns and 408 MHz maps
title_full Correlation of the South Pole 94 data with 100microns and 408 MHz maps
title_fullStr Correlation of the South Pole 94 data with 100microns and 408 MHz maps
title_full_unstemmed Correlation of the South Pole 94 data with 100microns and 408 MHz maps
title_sort correlation of the south pole 94 data with 100microns and 408 mhz maps
publisher arXiv
publishDate 2001
url https://dx.doi.org/10.48550/arxiv.astro-ph/0101131
https://arxiv.org/abs/astro-ph/0101131
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1051/0004-6361:20010061
op_rights Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004
http://arxiv.org/licenses/assumed-1991-2003/
op_doi https://doi.org/10.48550/arxiv.astro-ph/0101131
https://doi.org/10.1051/0004-6361:20010061
_version_ 1766201473506476032

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