Using White Dish CMB Anisotropy Data to Probe Open and Flat-A CDM Cosmogonies
We usedata from the White Dish experiment to set limits on cosmic microwave background radiation anisotropies in open and spatially-flat-A cold dark matter cosmogonies. We account for the White Dish calibration uncertainty, and over the offset and gradient removed from the data. Our 2-u upper limits...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.32.8997 2023-05-15T18:22:27+02:00 Using White Dish CMB Anisotropy Data to Probe Open and Flat-A CDM Cosmogonies Bharat Ratra Ken Ganga Naoshi Sugiyama G. S. Tucker G. S. Griffin H. T. Nguyen J. B. Peterson The Pennsylvania State University CiteSeerX Archives 1997 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.32.8997 http://techreports.jpl.nasa.gov/1997/97-1207.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.32.8997 http://techreports.jpl.nasa.gov/1997/97-1207.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://techreports.jpl.nasa.gov/1997/97-1207.pdf text 1997 ftciteseerx 2016-09-04T00:17:41Z We usedata from the White Dish experiment to set limits on cosmic microwave background radiation anisotropies in open and spatially-flat-A cold dark matter cosmogonies. We account for the White Dish calibration uncertainty, and over the offset and gradient removed from the data. Our 2-u upper limits are larger than those derived previously. These upper limits are consistent with those derived from the data for models tested. Subject headings: cosmic microwave background- cosmology: observations---large-scale structure of the universe -31. Introduction Ganga et al. (1997a, hereafter developed techniques to account for uncertainties, such as those in the beamwidth and calibration, in likelihood analyses of cosmic microwave background anisotropy data. GRGS and Ganga et used these techniques, in conjunction with theoretical CMB anisotropy spectra, in analyses of the UCSB South Pole 1994 et al. 1995), the (Church et al. 1997), and the MAX 4+5 (Tanaka et al. 1996; Lim et al. 1996, and ref. Text South pole Unknown South Pole |
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English |
description |
We usedata from the White Dish experiment to set limits on cosmic microwave background radiation anisotropies in open and spatially-flat-A cold dark matter cosmogonies. We account for the White Dish calibration uncertainty, and over the offset and gradient removed from the data. Our 2-u upper limits are larger than those derived previously. These upper limits are consistent with those derived from the data for models tested. Subject headings: cosmic microwave background- cosmology: observations---large-scale structure of the universe -31. Introduction Ganga et al. (1997a, hereafter developed techniques to account for uncertainties, such as those in the beamwidth and calibration, in likelihood analyses of cosmic microwave background anisotropy data. GRGS and Ganga et used these techniques, in conjunction with theoretical CMB anisotropy spectra, in analyses of the UCSB South Pole 1994 et al. 1995), the (Church et al. 1997), and the MAX 4+5 (Tanaka et al. 1996; Lim et al. 1996, and ref. |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Bharat Ratra Ken Ganga Naoshi Sugiyama G. S. Tucker G. S. Griffin H. T. Nguyen J. B. Peterson |
spellingShingle |
Bharat Ratra Ken Ganga Naoshi Sugiyama G. S. Tucker G. S. Griffin H. T. Nguyen J. B. Peterson Using White Dish CMB Anisotropy Data to Probe Open and Flat-A CDM Cosmogonies |
author_facet |
Bharat Ratra Ken Ganga Naoshi Sugiyama G. S. Tucker G. S. Griffin H. T. Nguyen J. B. Peterson |
author_sort |
Bharat Ratra |
title |
Using White Dish CMB Anisotropy Data to Probe Open and Flat-A CDM Cosmogonies |
title_short |
Using White Dish CMB Anisotropy Data to Probe Open and Flat-A CDM Cosmogonies |
title_full |
Using White Dish CMB Anisotropy Data to Probe Open and Flat-A CDM Cosmogonies |
title_fullStr |
Using White Dish CMB Anisotropy Data to Probe Open and Flat-A CDM Cosmogonies |
title_full_unstemmed |
Using White Dish CMB Anisotropy Data to Probe Open and Flat-A CDM Cosmogonies |
title_sort |
using white dish cmb anisotropy data to probe open and flat-a cdm cosmogonies |
publishDate |
1997 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.32.8997 http://techreports.jpl.nasa.gov/1997/97-1207.pdf |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
http://techreports.jpl.nasa.gov/1997/97-1207.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.32.8997 http://techreports.jpl.nasa.gov/1997/97-1207.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766201861572919296 |