University of california at Santa Barbara Anisotropy Program: degree scale results from the South Pole 1990-1991.
We report on the preliminary result of a search for anisotropy in the cosmic background radiation (CBR). Our receiver operates with four equally spaced channels from 25 to 35 GHz with a beam size of approximately 1.5 degrees full width at half maximum. The system operated successfully for 500 hr at...
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ftpubmed:oai:pubmedcentral.nih.gov:46598 2023-05-15T18:21:54+02:00 University of california at Santa Barbara Anisotropy Program: degree scale results from the South Pole 1990-1991. Gaier, T Schuster, J Gundersen, J Meinhold, P Lubin, P 1993-06-01 http://www.ncbi.nlm.nih.gov/pmc/articles/PMC46598 http://www.ncbi.nlm.nih.gov/pubmed/11607385 en eng http://www.ncbi.nlm.nih.gov/pmc/articles/PMC46598 http://www.ncbi.nlm.nih.gov/pubmed/11607385 Research Article Text 1993 ftpubmed 2013-08-29T08:07:36Z We report on the preliminary result of a search for anisotropy in the cosmic background radiation (CBR). Our receiver operates with four equally spaced channels from 25 to 35 GHz with a beam size of approximately 1.5 degrees full width at half maximum. The system operated successfully for 500 hr at the South Pole during 1990-1991 austral summer. The data from one region, representing 25 hr after editing, are presented here. A strong signal is present in the lower-frequency channels with a spectrum unlike CBR fluctuations. The highest-frequency channel has the smallest contribution from this signal and has been used to set a 95% confidence level upper limit DeltaT/T </= 1.4 10-5. Text South pole PubMed Central (PMC) Austral South Pole |
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Research Article Gaier, T Schuster, J Gundersen, J Meinhold, P Lubin, P University of california at Santa Barbara Anisotropy Program: degree scale results from the South Pole 1990-1991. |
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Research Article |
description |
We report on the preliminary result of a search for anisotropy in the cosmic background radiation (CBR). Our receiver operates with four equally spaced channels from 25 to 35 GHz with a beam size of approximately 1.5 degrees full width at half maximum. The system operated successfully for 500 hr at the South Pole during 1990-1991 austral summer. The data from one region, representing 25 hr after editing, are presented here. A strong signal is present in the lower-frequency channels with a spectrum unlike CBR fluctuations. The highest-frequency channel has the smallest contribution from this signal and has been used to set a 95% confidence level upper limit DeltaT/T </= 1.4 10-5. |
format |
Text |
author |
Gaier, T Schuster, J Gundersen, J Meinhold, P Lubin, P |
author_facet |
Gaier, T Schuster, J Gundersen, J Meinhold, P Lubin, P |
author_sort |
Gaier, T |
title |
University of california at Santa Barbara Anisotropy Program: degree scale results from the South Pole 1990-1991. |
title_short |
University of california at Santa Barbara Anisotropy Program: degree scale results from the South Pole 1990-1991. |
title_full |
University of california at Santa Barbara Anisotropy Program: degree scale results from the South Pole 1990-1991. |
title_fullStr |
University of california at Santa Barbara Anisotropy Program: degree scale results from the South Pole 1990-1991. |
title_full_unstemmed |
University of california at Santa Barbara Anisotropy Program: degree scale results from the South Pole 1990-1991. |
title_sort |
university of california at santa barbara anisotropy program: degree scale results from the south pole 1990-1991. |
publishDate |
1993 |
url |
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC46598 http://www.ncbi.nlm.nih.gov/pubmed/11607385 |
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Austral South Pole |
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Austral South Pole |
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South pole |
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South pole |
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http://www.ncbi.nlm.nih.gov/pmc/articles/PMC46598 http://www.ncbi.nlm.nih.gov/pubmed/11607385 |
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1766201224977186816 |