OVRO CMB Anisotropy Measurement Constraints on Flat-Λ and Open CDM
We use Owens Valley Radio Observatory (OVRO) cosmic microwave background (CMB) anisotropy data to constrain cosmological parameters. We account for the OVRO beamwidth and calibration uncertainties, as well as the uncertainty induced by the removal of non-CMB foreground contamination. We consider ope...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.258.2535 2023-05-15T18:22:30+02:00 OVRO CMB Anisotropy Measurement Constraints on Flat-Λ and Open CDM Pia Mukherjee Tarun Souradeep Bharat Ratra Naoshi Sugiyama Krzysztof M. Górski The Pennsylvania State University CiteSeerX Archives 2002 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.258.2535 http://arxiv.org/pdf/astro-ph/0208216v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.258.2535 http://arxiv.org/pdf/astro-ph/0208216v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/0208216v1.pdf text 2002 ftciteseerx 2016-01-07T20:02:39Z We use Owens Valley Radio Observatory (OVRO) cosmic microwave background (CMB) anisotropy data to constrain cosmological parameters. We account for the OVRO beamwidth and calibration uncertainties, as well as the uncertainty induced by the removal of non-CMB foreground contamination. We consider open and spatiallyflat-Λ cold dark matter cosmogonies, with nonrelativistic-mass density parameter Ω0 in the range 0.1–1, baryonic-mass density parameter ΩB in the range (0.005–0.029)h −2, and age of the universe t0 in the range (10–20) Gyr. Marginalizing over all parameters but Ω0, the OVRO data favors an open (spatially-flat-Λ) model with Ω0 ≃ 0.33 (0.1). At the 2 σ confidence level model normalizations deduced from the OVRO data are mostly consistent with those deduced from the DMR, UCSB South Pole 1994, Python I-III, ARGO, MAX 4 and 5, White Dish, and SuZIE data sets. Subject headings: cosmic microwave background—cosmology: observations—large-scale structure of the universe 1. Text South pole Unknown South Pole |
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description |
We use Owens Valley Radio Observatory (OVRO) cosmic microwave background (CMB) anisotropy data to constrain cosmological parameters. We account for the OVRO beamwidth and calibration uncertainties, as well as the uncertainty induced by the removal of non-CMB foreground contamination. We consider open and spatiallyflat-Λ cold dark matter cosmogonies, with nonrelativistic-mass density parameter Ω0 in the range 0.1–1, baryonic-mass density parameter ΩB in the range (0.005–0.029)h −2, and age of the universe t0 in the range (10–20) Gyr. Marginalizing over all parameters but Ω0, the OVRO data favors an open (spatially-flat-Λ) model with Ω0 ≃ 0.33 (0.1). At the 2 σ confidence level model normalizations deduced from the OVRO data are mostly consistent with those deduced from the DMR, UCSB South Pole 1994, Python I-III, ARGO, MAX 4 and 5, White Dish, and SuZIE data sets. Subject headings: cosmic microwave background—cosmology: observations—large-scale structure of the universe 1. |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Pia Mukherjee Tarun Souradeep Bharat Ratra Naoshi Sugiyama Krzysztof M. Górski |
spellingShingle |
Pia Mukherjee Tarun Souradeep Bharat Ratra Naoshi Sugiyama Krzysztof M. Górski OVRO CMB Anisotropy Measurement Constraints on Flat-Λ and Open CDM |
author_facet |
Pia Mukherjee Tarun Souradeep Bharat Ratra Naoshi Sugiyama Krzysztof M. Górski |
author_sort |
Pia Mukherjee |
title |
OVRO CMB Anisotropy Measurement Constraints on Flat-Λ and Open CDM |
title_short |
OVRO CMB Anisotropy Measurement Constraints on Flat-Λ and Open CDM |
title_full |
OVRO CMB Anisotropy Measurement Constraints on Flat-Λ and Open CDM |
title_fullStr |
OVRO CMB Anisotropy Measurement Constraints on Flat-Λ and Open CDM |
title_full_unstemmed |
OVRO CMB Anisotropy Measurement Constraints on Flat-Λ and Open CDM |
title_sort |
ovro cmb anisotropy measurement constraints on flat-λ and open cdm |
publishDate |
2002 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.258.2535 http://arxiv.org/pdf/astro-ph/0208216v1.pdf |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
http://arxiv.org/pdf/astro-ph/0208216v1.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.258.2535 http://arxiv.org/pdf/astro-ph/0208216v1.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766201919394545664 |