Preprint typeset using L ATEX style emulateapj v. 04/03/99 FIRST RESULTS FROM VIPER: DETECTION OF SMALL-SCALE ANISOTROPY AT 40 GHZ

Results of a search for small-scale anisotropy in the cosmic microwave background (CMB) are presented. Observations were made at the South Pole using the Viper telescope, with a.26 ◦ (FWHM) beam and a passband centered at 40 GHz. Anisotropy band-power measurements in bands centered

Bibliographic Details
Main Authors: J. B. Peterson, G. S. Griffin, M. G. Newcomb, D. L. Alvarez, D. Morgan, K. W. Miller, K. Ganga, D. Pernic, M. Thoma
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2008
Subjects:
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.317.6366
http://arxiv.org/pdf/astro-ph/9910503v1.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.317.6366 2023-05-15T18:21:58+02:00 Preprint typeset using L ATEX style emulateapj v. 04/03/99 FIRST RESULTS FROM VIPER: DETECTION OF SMALL-SCALE ANISOTROPY AT 40 GHZ J. B. Peterson G. S. Griffin M. G. Newcomb D. L. Alvarez D. Morgan K. W. Miller K. Ganga D. Pernic M. Thoma The Pennsylvania State University CiteSeerX Archives 2008 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.317.6366 http://arxiv.org/pdf/astro-ph/9910503v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.317.6366 http://arxiv.org/pdf/astro-ph/9910503v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/9910503v1.pdf text 2008 ftciteseerx 2016-09-04T00:10:14Z Results of a search for small-scale anisotropy in the cosmic microwave background (CMB) are presented. Observations were made at the South Pole using the Viper telescope, with a.26 ◦ (FWHM) beam and a passband centered at 40 GHz. Anisotropy band-power measurements in bands centered Text South pole Unknown South Pole
institution Open Polar
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language English
description Results of a search for small-scale anisotropy in the cosmic microwave background (CMB) are presented. Observations were made at the South Pole using the Viper telescope, with a.26 ◦ (FWHM) beam and a passband centered at 40 GHz. Anisotropy band-power measurements in bands centered
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author J. B. Peterson
G. S. Griffin
M. G. Newcomb
D. L. Alvarez
D. Morgan
K. W. Miller
K. Ganga
D. Pernic
M. Thoma
spellingShingle J. B. Peterson
G. S. Griffin
M. G. Newcomb
D. L. Alvarez
D. Morgan
K. W. Miller
K. Ganga
D. Pernic
M. Thoma
Preprint typeset using L ATEX style emulateapj v. 04/03/99 FIRST RESULTS FROM VIPER: DETECTION OF SMALL-SCALE ANISOTROPY AT 40 GHZ
author_facet J. B. Peterson
G. S. Griffin
M. G. Newcomb
D. L. Alvarez
D. Morgan
K. W. Miller
K. Ganga
D. Pernic
M. Thoma
author_sort J. B. Peterson
title Preprint typeset using L ATEX style emulateapj v. 04/03/99 FIRST RESULTS FROM VIPER: DETECTION OF SMALL-SCALE ANISOTROPY AT 40 GHZ
title_short Preprint typeset using L ATEX style emulateapj v. 04/03/99 FIRST RESULTS FROM VIPER: DETECTION OF SMALL-SCALE ANISOTROPY AT 40 GHZ
title_full Preprint typeset using L ATEX style emulateapj v. 04/03/99 FIRST RESULTS FROM VIPER: DETECTION OF SMALL-SCALE ANISOTROPY AT 40 GHZ
title_fullStr Preprint typeset using L ATEX style emulateapj v. 04/03/99 FIRST RESULTS FROM VIPER: DETECTION OF SMALL-SCALE ANISOTROPY AT 40 GHZ
title_full_unstemmed Preprint typeset using L ATEX style emulateapj v. 04/03/99 FIRST RESULTS FROM VIPER: DETECTION OF SMALL-SCALE ANISOTROPY AT 40 GHZ
title_sort preprint typeset using l atex style emulateapj v. 04/03/99 first results from viper: detection of small-scale anisotropy at 40 ghz
publishDate 2008
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.317.6366
http://arxiv.org/pdf/astro-ph/9910503v1.pdf
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genre_facet South pole
op_source http://arxiv.org/pdf/astro-ph/9910503v1.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.317.6366
http://arxiv.org/pdf/astro-ph/9910503v1.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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