Correlation of the South Pole 94 data with 100µm 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: Article in Journal/Newspaper
Language:English
Published: EDP Sciences 2001
Subjects:
South Pole
South pole
Online Access:https://authors.library.caltech.edu/85152/
https://authors.library.caltech.edu/85152/1/aa10347.pdf
https://resolver.caltech.edu/CaltechAUTHORS:20180307-070305356
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spelling ftcaltechauth:oai:authors.library.caltech.edu:85152 2023-05-15T18:22:03+02:00 Correlation of the South Pole 94 data with 100µm and 408 MHz maps Hamilton, J.-Ch. Ganga, K. M. 2001-11-04 application/pdf https://authors.library.caltech.edu/85152/ https://authors.library.caltech.edu/85152/1/aa10347.pdf https://resolver.caltech.edu/CaltechAUTHORS:20180307-070305356 en eng EDP Sciences https://authors.library.caltech.edu/85152/1/aa10347.pdf Hamilton, J.-Ch. and Ganga, K. M. (2001) Correlation of the South Pole 94 data with 100µm and 408 MHz maps. Astronomy & Astrophysics, 368 (3). pp. 760-765. ISSN 0004-6361. doi:10.1051/0004-6361:20010061. https://resolver.caltech.edu/CaltechAUTHORS:20180307-070305356 <https://resolver.caltech.edu/CaltechAUTHORS:20180307-070305356> other Article PeerReviewed 2001 ftcaltechauth 2021-11-18T18:45:11Z 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. Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology) South Pole
institution Open Polar
collection Caltech Authors (California Institute of Technology)
op_collection_id ftcaltechauth
language English
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.
format Article in Journal/Newspaper
author Hamilton, J.-Ch.
Ganga, K. M.
spellingShingle Hamilton, J.-Ch.
Ganga, K. M.
Correlation of the South Pole 94 data with 100µm and 408 MHz maps
author_facet Hamilton, J.-Ch.
Ganga, K. M.
author_sort Hamilton, J.-Ch.
title Correlation of the South Pole 94 data with 100µm and 408 MHz maps
title_short Correlation of the South Pole 94 data with 100µm and 408 MHz maps
title_full Correlation of the South Pole 94 data with 100µm and 408 MHz maps
title_fullStr Correlation of the South Pole 94 data with 100µm and 408 MHz maps
title_full_unstemmed Correlation of the South Pole 94 data with 100µm and 408 MHz maps
title_sort correlation of the south pole 94 data with 100µm and 408 mhz maps
publisher EDP Sciences
publishDate 2001
url https://authors.library.caltech.edu/85152/
https://authors.library.caltech.edu/85152/1/aa10347.pdf
https://resolver.caltech.edu/CaltechAUTHORS:20180307-070305356
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://authors.library.caltech.edu/85152/1/aa10347.pdf
Hamilton, J.-Ch. and Ganga, K. M. (2001) Correlation of the South Pole 94 data with 100µm and 408 MHz maps. Astronomy & Astrophysics, 368 (3). pp. 760-765. ISSN 0004-6361. doi:10.1051/0004-6361:20010061. https://resolver.caltech.edu/CaltechAUTHORS:20180307-070305356 <https://resolver.caltech.edu/CaltechAUTHORS:20180307-070305356>
op_rights other
_version_ 1766201402004078592

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