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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Bibliographic Details
Main Authors: Hamilton, J.-Ch., Ganga, K. M.
Format: Article in Journal/Newspaper
Language:unknown
Published: EDP Sciences 2001
Subjects:
cosmic microwave background - cosmology: observations
South pole
Online Access:https://doi.org/10.1051/0004-6361:20010061
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spelling ftcaltechauth:oai:authors.library.caltech.edu:m0hqy-z5347 2024-09-15T18:36:44+00:00 Correlation of the South Pole 94 data with 100µm and 408 MHz maps Hamilton, J.-Ch. Ganga, K. M. 2001-11-04 https://doi.org/10.1051/0004-6361:20010061 unknown EDP Sciences https://doi.org/10.1051/0004-6361:20010061 oai:authors.library.caltech.edu:m0hqy-z5347 eprintid:85152 resolverid:CaltechAUTHORS:20180307-070305356 info:eu-repo/semantics/openAccess Other Astronomy & Astrophysics, 368(3), 760-765, (2001-11-04) cosmic microwave background - cosmology: observations info:eu-repo/semantics/article 2001 ftcaltechauth https://doi.org/10.1051/0004-6361:20010061 2024-08-06T15:34:58Z 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. © 2001 ESO. Received: 11 October 2000. Accepted: 8 January 2000. The authors would like to thank J. O. Gundersen and the ACME team for making the SP94 data available. We would also like to thank F. X. Désert for fruitful discussions. Published - aa10347.pdf Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology)
institution Open Polar
collection Caltech Authors (California Institute of Technology)
op_collection_id ftcaltechauth
language unknown
topic cosmic microwave background - cosmology: observations
spellingShingle cosmic microwave background - cosmology: observations
Hamilton, J.-Ch.
Ganga, K. M.
Correlation of the South Pole 94 data with 100µm and 408 MHz maps
topic_facet cosmic microwave background - cosmology: observations
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. © 2001 ESO. Received: 11 October 2000. Accepted: 8 January 2000. The authors would like to thank J. O. Gundersen and the ACME team for making the SP94 data available. We would also like to thank F. X. Désert for fruitful discussions. Published - aa10347.pdf
format Article in Journal/Newspaper
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 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 100âµm and 408 mhz maps
publisher EDP Sciences
publishDate 2001
url https://doi.org/10.1051/0004-6361:20010061
genre South pole
genre_facet South pole
op_source Astronomy & Astrophysics, 368(3), 760-765, (2001-11-04)
op_relation https://doi.org/10.1051/0004-6361:20010061
oai:authors.library.caltech.edu:m0hqy-z5347
eprintid:85152
resolverid:CaltechAUTHORS:20180307-070305356
op_rights info:eu-repo/semantics/openAccess
Other
op_doi https://doi.org/10.1051/0004-6361:20010061
_version_ 1810480449941667840

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