UCSB South Pole 1994 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies

We develop methods to account for experimental and observational uncertainties in likelihood analyses of data from cosmic microwave background (CMB) anisotropy experiments and apply them to an analysis of the UCSB South Pole 1994 (SP94) experiment. Observationally motivated open and spatially-flat $...

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Main Authors: Ganga, Ken, Ratra, Bharat, Gundersen, Josh, Sugiyama, Naoshi
Format: Text
Language:unknown
Published: arXiv 1996
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/9602141
https://arxiv.org/abs/astro-ph/9602141
id ftdatacite:10.48550/arxiv.astro-ph/9602141
record_format openpolar
spelling ftdatacite:10.48550/arxiv.astro-ph/9602141 2023-05-15T18:22:14+02:00 UCSB South Pole 1994 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies Ganga, Ken Ratra, Bharat Gundersen, Josh Sugiyama, Naoshi 1996 https://dx.doi.org/10.48550/arxiv.astro-ph/9602141 https://arxiv.org/abs/astro-ph/9602141 unknown arXiv https://dx.doi.org/10.1086/304296 Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 1996 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/9602141 https://doi.org/10.1086/304296 2022-04-01T17:42:08Z We develop methods to account for experimental and observational uncertainties in likelihood analyses of data from cosmic microwave background (CMB) anisotropy experiments and apply them to an analysis of the UCSB South Pole 1994 (SP94) experiment. Observationally motivated open and spatially-flat $Λ$, cold dark matter cosmogonies are considered. Among the models we consider, the full SP94 data set is most consistent with $Ω_0 \sim 0.1-0.2$ open models and less so with old $(t_0 \gap 15 - 16 Gyr)$, high baryon density $(Ω_B \gap 0.0175 h^{-2})$, low density ($Ω_0 \sim 0.2 - 0.4), flat-$Λ$ models. The SP94 data do not rule out any of the models we consider at the $2σ$ level. The SP94 experiment is most sensitive to anisotropies on a somewhat larger, model-dependent, angular scale than the scale at which the window function peaks. For establishing the significance of a detection of CMB anisotropy we derive limits using the highest posterior density (HPD) prescription, since it yields smaller lower limits. Since HPD limits lead to tighter constraints on the CMB amplitude, they also provide for greater discrimination between models. Model normalizations deduced from the SP94 data subsets are mostly consistent with those deduced from the two-year COBE-DMR data, although the Ka-band data prefer a normalization $\sim 1σ$ lower than do the Q-band data, the Q and Ka + Q data favour a slightly higher normalization for the $Ω_0 = 0.1$ open model than does the DMR, and the Ka and Ka + Q data prefer a somewhat lower normalization for the older, higher $Ω_B$, low-density $Λ$ models than does the DMR. : Substantially shortened and rewritten. Accepted by ApJ. PostScript. 49 pages of text + tables. 16 pages of figures Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole Lambda ENVELOPE(-62.983,-62.983,-64.300,-64.300)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
Ganga, Ken
Ratra, Bharat
Gundersen, Josh
Sugiyama, Naoshi
UCSB South Pole 1994 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies
topic_facet Astrophysics astro-ph
FOS Physical sciences
description We develop methods to account for experimental and observational uncertainties in likelihood analyses of data from cosmic microwave background (CMB) anisotropy experiments and apply them to an analysis of the UCSB South Pole 1994 (SP94) experiment. Observationally motivated open and spatially-flat $Λ$, cold dark matter cosmogonies are considered. Among the models we consider, the full SP94 data set is most consistent with $Ω_0 \sim 0.1-0.2$ open models and less so with old $(t_0 \gap 15 - 16 Gyr)$, high baryon density $(Ω_B \gap 0.0175 h^{-2})$, low density ($Ω_0 \sim 0.2 - 0.4), flat-$Λ$ models. The SP94 data do not rule out any of the models we consider at the $2σ$ level. The SP94 experiment is most sensitive to anisotropies on a somewhat larger, model-dependent, angular scale than the scale at which the window function peaks. For establishing the significance of a detection of CMB anisotropy we derive limits using the highest posterior density (HPD) prescription, since it yields smaller lower limits. Since HPD limits lead to tighter constraints on the CMB amplitude, they also provide for greater discrimination between models. Model normalizations deduced from the SP94 data subsets are mostly consistent with those deduced from the two-year COBE-DMR data, although the Ka-band data prefer a normalization $\sim 1σ$ lower than do the Q-band data, the Q and Ka + Q data favour a slightly higher normalization for the $Ω_0 = 0.1$ open model than does the DMR, and the Ka and Ka + Q data prefer a somewhat lower normalization for the older, higher $Ω_B$, low-density $Λ$ models than does the DMR. : Substantially shortened and rewritten. Accepted by ApJ. PostScript. 49 pages of text + tables. 16 pages of figures
format Text
author Ganga, Ken
Ratra, Bharat
Gundersen, Josh
Sugiyama, Naoshi
author_facet Ganga, Ken
Ratra, Bharat
Gundersen, Josh
Sugiyama, Naoshi
author_sort Ganga, Ken
title UCSB South Pole 1994 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies
title_short UCSB South Pole 1994 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies
title_full UCSB South Pole 1994 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies
title_fullStr UCSB South Pole 1994 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies
title_full_unstemmed UCSB South Pole 1994 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies
title_sort ucsb south pole 1994 cmb anisotropy measurement constraints on open and flat-lambda cdm cosmogonies
publisher arXiv
publishDate 1996
url https://dx.doi.org/10.48550/arxiv.astro-ph/9602141
https://arxiv.org/abs/astro-ph/9602141
long_lat ENVELOPE(-62.983,-62.983,-64.300,-64.300)
geographic South Pole
Lambda
geographic_facet South Pole
Lambda
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1086/304296
op_rights Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004
http://arxiv.org/licenses/assumed-1991-2003/
op_doi https://doi.org/10.48550/arxiv.astro-ph/9602141
https://doi.org/10.1086/304296
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