Preprint typeset using L ATEX style emulateapj v. 04/03/99 COSMIC MICROWAVE BACKGROUND ANISOTROPY MEASUREMENT FROM PYTHON V
We analyze observations of the microwave sky made with the Python experiment in its fifth year of operation at the Amundsen-Scott South Pole Station in Antarctica. After modeling the noise and constructing a map, we extract the cosmic signal from the data. We simultaneously estimate the angular powe...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.256.1747 2023-05-15T13:24:26+02:00 Preprint typeset using L ATEX style emulateapj v. 04/03/99 COSMIC MICROWAVE BACKGROUND ANISOTROPY MEASUREMENT FROM PYTHON V K. Coble S. Dodelson M. Dragovan K. Ganga L. Knox J. Kovac B. Ratra T. Souradeep The Pennsylvania State University CiteSeerX Archives 2001 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.1747 http://arxiv.org/pdf/astro-ph/0112506v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.1747 http://arxiv.org/pdf/astro-ph/0112506v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0112506v1.pdf text 2001 ftciteseerx 2016-01-07T19:56:47Z We analyze observations of the microwave sky made with the Python experiment in its fifth year of operation at the Amundsen-Scott South Pole Station in Antarctica. After modeling the noise and constructing a map, we extract the cosmic signal from the data. We simultaneously estimate the angular power spectrum in eight bands ranging from large (ℓ ∼ 40) to small (ℓ ∼ 260) angular scales, with power detected in the first six bands. There is a significant rise in the power spectrum from large to smaller (ℓ ∼ 200) scales, consistent with that expected from acoustic oscillations in the early Universe. We compare this Python V map to a map made from data taken in the third year of Python. Python III observations were made at a frequency of 90 GHz and covered a subset of the region of the sky covered by Python V observations, which were made at 40 GHz. Good agreement is obtained both visually (with a filtered version of the map) and via a likelihood ratio test. Subject headings: cosmic microwave background- cosmology: observations 1. Text Amundsen-Scott Antarc* Antarctica South pole South pole Unknown 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 |
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Open Polar |
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Unknown |
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ftciteseerx |
language |
English |
description |
We analyze observations of the microwave sky made with the Python experiment in its fifth year of operation at the Amundsen-Scott South Pole Station in Antarctica. After modeling the noise and constructing a map, we extract the cosmic signal from the data. We simultaneously estimate the angular power spectrum in eight bands ranging from large (ℓ ∼ 40) to small (ℓ ∼ 260) angular scales, with power detected in the first six bands. There is a significant rise in the power spectrum from large to smaller (ℓ ∼ 200) scales, consistent with that expected from acoustic oscillations in the early Universe. We compare this Python V map to a map made from data taken in the third year of Python. Python III observations were made at a frequency of 90 GHz and covered a subset of the region of the sky covered by Python V observations, which were made at 40 GHz. Good agreement is obtained both visually (with a filtered version of the map) and via a likelihood ratio test. Subject headings: cosmic microwave background- cosmology: observations 1. |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
K. Coble S. Dodelson M. Dragovan K. Ganga L. Knox J. Kovac B. Ratra T. Souradeep |
spellingShingle |
K. Coble S. Dodelson M. Dragovan K. Ganga L. Knox J. Kovac B. Ratra T. Souradeep Preprint typeset using L ATEX style emulateapj v. 04/03/99 COSMIC MICROWAVE BACKGROUND ANISOTROPY MEASUREMENT FROM PYTHON V |
author_facet |
K. Coble S. Dodelson M. Dragovan K. Ganga L. Knox J. Kovac B. Ratra T. Souradeep |
author_sort |
K. Coble |
title |
Preprint typeset using L ATEX style emulateapj v. 04/03/99 COSMIC MICROWAVE BACKGROUND ANISOTROPY MEASUREMENT FROM PYTHON V |
title_short |
Preprint typeset using L ATEX style emulateapj v. 04/03/99 COSMIC MICROWAVE BACKGROUND ANISOTROPY MEASUREMENT FROM PYTHON V |
title_full |
Preprint typeset using L ATEX style emulateapj v. 04/03/99 COSMIC MICROWAVE BACKGROUND ANISOTROPY MEASUREMENT FROM PYTHON V |
title_fullStr |
Preprint typeset using L ATEX style emulateapj v. 04/03/99 COSMIC MICROWAVE BACKGROUND ANISOTROPY MEASUREMENT FROM PYTHON V |
title_full_unstemmed |
Preprint typeset using L ATEX style emulateapj v. 04/03/99 COSMIC MICROWAVE BACKGROUND ANISOTROPY MEASUREMENT FROM PYTHON V |
title_sort |
preprint typeset using l atex style emulateapj v. 04/03/99 cosmic microwave background anisotropy measurement from python v |
publishDate |
2001 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.1747 http://arxiv.org/pdf/astro-ph/0112506v1.pdf |
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_source |
http://arxiv.org/pdf/astro-ph/0112506v1.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.1747 http://arxiv.org/pdf/astro-ph/0112506v1.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766379691258675200 |