Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE
We describe the Bayesian-based signal-to-noise eigenmode method for cosmological parameter estimation, show how it can be used to optimally compress large CMB anisotropy data sets to manageable sizes, and apply it to the DMR 4-year, South Pole and Saskatchewan data, individually and in combination....
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1997
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| Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.337.9137 http://arxiv.org/pdf/astro-ph/9610091v1.pdf |
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.337.9137 |
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.337.9137 2023-05-15T18:22:02+02:00 Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE J. Richard Bond Andrew H. Jaffe The Pennsylvania State University CiteSeerX Archives 1997 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.337.9137 http://arxiv.org/pdf/astro-ph/9610091v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.337.9137 http://arxiv.org/pdf/astro-ph/9610091v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/astro-ph/9610091v1.pdf text 1997 ftciteseerx 2016-01-07T23:44:59Z We describe the Bayesian-based signal-to-noise eigenmode method for cosmological parameter estimation, show how it can be used to optimally compress large CMB anisotropy data sets to manageable sizes, and apply it to the DMR 4-year, South Pole and Saskatchewan data, individually and in combination. A simple prior probability method is used to include large scale structure observations. Estimates of the Hubble parameter, vacuum energy density, baryon fraction and primordial spectral tilt derived from the combined data are given. 1 Text South pole Unknown Hubble ENVELOPE(158.317,158.317,-80.867,-80.867) South Pole |
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ftciteseerx |
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English |
| description |
We describe the Bayesian-based signal-to-noise eigenmode method for cosmological parameter estimation, show how it can be used to optimally compress large CMB anisotropy data sets to manageable sizes, and apply it to the DMR 4-year, South Pole and Saskatchewan data, individually and in combination. A simple prior probability method is used to include large scale structure observations. Estimates of the Hubble parameter, vacuum energy density, baryon fraction and primordial spectral tilt derived from the combined data are given. 1 |
| author2 |
The Pennsylvania State University CiteSeerX Archives |
| format |
Text |
| author |
J. Richard Bond Andrew H. Jaffe |
| spellingShingle |
J. Richard Bond Andrew H. Jaffe Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE |
| author_facet |
J. Richard Bond Andrew H. Jaffe |
| author_sort |
J. Richard Bond |
| title |
Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE |
| title_short |
Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE |
| title_full |
Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE |
| title_fullStr |
Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE |
| title_full_unstemmed |
Cosmic Parameter Estimation Combining Sub-Degree CMB Experiments with COBE |
| title_sort |
cosmic parameter estimation combining sub-degree cmb experiments with cobe |
| publishDate |
1997 |
| url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.337.9137 http://arxiv.org/pdf/astro-ph/9610091v1.pdf |
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ENVELOPE(158.317,158.317,-80.867,-80.867) |
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Hubble South Pole |
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Hubble South Pole |
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South pole |
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South pole |
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http://arxiv.org/pdf/astro-ph/9610091v1.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.337.9137 http://arxiv.org/pdf/astro-ph/9610091v1.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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1766201394048532480 |