Stability of the submillimeter brightness of the atmosphere above

The summit of Mauna Kea in Hawaii, the area near Cerro Chajnantor in Chile, and the South Pole are sites of large millimeter or submillimeter wavelength telescopes. We have placed 860 GHz sky brightness monitors at all three sites and present a comparative study of the measured submillimeter brightn...

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Bibliographic Details
Main Authors: J. B. Peterson, S. J. E. Radford, P. A. R. Ade, R. A. Chamberlin, M. J. O’kelly, K. M. Peterson, E. Schartman
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2003
Subjects:
South Pole
South pole
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.315.4907
http://arxiv.org/pdf/astro-ph/0211134v1.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.315.4907 2023-05-15T18:21:59+02:00 Stability of the submillimeter brightness of the atmosphere above J. B. Peterson S. J. E. Radford P. A. R. Ade R. A. Chamberlin M. J. O’kelly K. M. Peterson E. Schartman The Pennsylvania State University CiteSeerX Archives 2003 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.315.4907 http://arxiv.org/pdf/astro-ph/0211134v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.315.4907 http://arxiv.org/pdf/astro-ph/0211134v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0211134v1.pdf text 2003 ftciteseerx 2016-09-04T00:05:55Z The summit of Mauna Kea in Hawaii, the area near Cerro Chajnantor in Chile, and the South Pole are sites of large millimeter or submillimeter wavelength telescopes. We have placed 860 GHz sky brightness monitors at all three sites and present a comparative study of the measured submillimeter brightness due to atmospheric thermal emission. We report the stability of that quantity at each site. 1. Text South pole Unknown South Pole
institution Open Polar
collection Unknown
op_collection_id ftciteseerx
language English
description The summit of Mauna Kea in Hawaii, the area near Cerro Chajnantor in Chile, and the South Pole are sites of large millimeter or submillimeter wavelength telescopes. We have placed 860 GHz sky brightness monitors at all three sites and present a comparative study of the measured submillimeter brightness due to atmospheric thermal emission. We report the stability of that quantity at each site. 1.
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author J. B. Peterson
S. J. E. Radford
P. A. R. Ade
R. A. Chamberlin
M. J. O’kelly
K. M. Peterson
E. Schartman
spellingShingle J. B. Peterson
S. J. E. Radford
P. A. R. Ade
R. A. Chamberlin
M. J. O’kelly
K. M. Peterson
E. Schartman
Stability of the submillimeter brightness of the atmosphere above
author_facet J. B. Peterson
S. J. E. Radford
P. A. R. Ade
R. A. Chamberlin
M. J. O’kelly
K. M. Peterson
E. Schartman
author_sort J. B. Peterson
title Stability of the submillimeter brightness of the atmosphere above
title_short Stability of the submillimeter brightness of the atmosphere above
title_full Stability of the submillimeter brightness of the atmosphere above
title_fullStr Stability of the submillimeter brightness of the atmosphere above
title_full_unstemmed Stability of the submillimeter brightness of the atmosphere above
title_sort stability of the submillimeter brightness of the atmosphere above
publishDate 2003
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.315.4907
http://arxiv.org/pdf/astro-ph/0211134v1.pdf
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source http://arxiv.org/pdf/astro-ph/0211134v1.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.315.4907
http://arxiv.org/pdf/astro-ph/0211134v1.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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