Anisotropy of the microwave sky at 90 GHz: results from Python II
We report on additional observations of degree scale anisotropy at 90~GHz from the Amundsen-Scott South Pole Station in Antarctica. Observations during the first season with the Python instrument yielded a statistically significant sky signal; in this paper we report the confirmation of that signal...
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ftcern:oai:cds.cern.ch:286364 2023-05-15T13:24:23+02:00 Anisotropy of the microwave sky at 90 GHz: results from Python II Ruhl, J E Dragovan, M Platt, S R Kovács, J Novák, G S 1995-08-16 http://cds.cern.ch/record/286364 eng eng http://cds.cern.ch/record/286364 astro-ph/9508065 EFI-95-38-[CHICAGO] oai:cds.cern.ch:286364 Astrophysics and Astronomy 1995 ftcern 2018-07-28T02:42:49Z We report on additional observations of degree scale anisotropy at 90~GHz from the Amundsen-Scott South Pole Station in Antarctica. Observations during the first season with the Python instrument yielded a statistically significant sky signal; in this paper we report the confirmation of that signal with data taken in the second year, and on results from an interleaving set of fields. Other/Unknown Material Amundsen-Scott Antarc* Antarctica South pole South pole CERN Document Server (CDS) Amundsen Scott South Pole Station ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen-Scott ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen-Scott South Pole Station ENVELOPE(139.273,139.273,-89.998,-89.998) South Pole |
institution |
Open Polar |
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CERN Document Server (CDS) |
op_collection_id |
ftcern |
language |
English |
topic |
Astrophysics and Astronomy |
spellingShingle |
Astrophysics and Astronomy Ruhl, J E Dragovan, M Platt, S R Kovács, J Novák, G S Anisotropy of the microwave sky at 90 GHz: results from Python II |
topic_facet |
Astrophysics and Astronomy |
description |
We report on additional observations of degree scale anisotropy at 90~GHz from the Amundsen-Scott South Pole Station in Antarctica. Observations during the first season with the Python instrument yielded a statistically significant sky signal; in this paper we report the confirmation of that signal with data taken in the second year, and on results from an interleaving set of fields. |
author |
Ruhl, J E Dragovan, M Platt, S R Kovács, J Novák, G S |
author_facet |
Ruhl, J E Dragovan, M Platt, S R Kovács, J Novák, G S |
author_sort |
Ruhl, J E |
title |
Anisotropy of the microwave sky at 90 GHz: results from Python II |
title_short |
Anisotropy of the microwave sky at 90 GHz: results from Python II |
title_full |
Anisotropy of the microwave sky at 90 GHz: results from Python II |
title_fullStr |
Anisotropy of the microwave sky at 90 GHz: results from Python II |
title_full_unstemmed |
Anisotropy of the microwave sky at 90 GHz: results from Python II |
title_sort |
anisotropy of the microwave sky at 90 ghz: results from python ii |
publishDate |
1995 |
url |
http://cds.cern.ch/record/286364 |
long_lat |
ENVELOPE(0.000,0.000,-90.000,-90.000) ENVELOPE(0.000,0.000,-90.000,-90.000) ENVELOPE(139.273,139.273,-89.998,-89.998) |
geographic |
Amundsen Scott South Pole Station Amundsen-Scott Amundsen-Scott South Pole Station South Pole |
geographic_facet |
Amundsen Scott South Pole Station Amundsen-Scott Amundsen-Scott South Pole Station South Pole |
genre |
Amundsen-Scott Antarc* Antarctica South pole South pole |
genre_facet |
Amundsen-Scott Antarc* Antarctica South pole South pole |
op_relation |
http://cds.cern.ch/record/286364 astro-ph/9508065 EFI-95-38-[CHICAGO] oai:cds.cern.ch:286364 |
_version_ |
1766379471747678208 |