A High Resolution Measurement of Temperature Anisotropies in the Cosmic Microwave Background Radiation with the Complete ACBAR Data Set
The Arcminute Cosmology Bolometer Array Receiver (ACBAR) is a 16-element spiderweb bolometer array operating at 150 GHz. Mounted on the 2.1m Viper telescope, ACBAR has dedicated four years to cosmic microwave background (CMB) observations at the South Pole. We describe the focal plane reconstruction...
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ftdatacite:10.7907/a0nq-td75 2023-05-15T18:22:06+02:00 A High Resolution Measurement of Temperature Anisotropies in the Cosmic Microwave Background Radiation with the Complete ACBAR Data Set Reichardt, Christian L. 2008 PDF https://dx.doi.org/10.7907/a0nq-td75 https://resolver.caltech.edu/CaltechETD:etd-12202007-130152 en eng California Institute of Technology No commercial reproduction, distribution, display or performance rights in this work are provided. observations cosmic microwave background South Pole Physics cosmology Thesis Text Dissertation thesis 2008 ftdatacite https://doi.org/10.7907/a0nq-td75 2021-11-05T12:55:41Z The Arcminute Cosmology Bolometer Array Receiver (ACBAR) is a 16-element spiderweb bolometer array operating at 150 GHz. Mounted on the 2.1m Viper telescope, ACBAR has dedicated four years to cosmic microwave background (CMB) observations at the South Pole. We describe the focal plane reconstruction and performance of ACBAR for the 2005 austral winter. We present a new CMB temperature anisotropy power spectrum for the complete ACBAR data set. The addition of data from the 2005 observing season expands the data set by 210%; and the sky coverage by 490%; over the previous ACBAR releases. The expanded data set allows us to derive a new set of band-power measurements with finer ℓ-resolution and dramatically smaller uncertainties. In particular, the band-power uncertainties have been reduced by more than a factor of two on angular scales encompassing the third and fourth acoustic peaks and the damping tail of the CMB power spectrum. The calibration has been significantly improved from 6%; to 2.2%; in temperature by using a direct comparison between CMB anisotropy maps measured by WMAP3 and ACBAR to transfer the WMAP dipole-based calibration to ACBAR. The resulting power spectrum is consistent with theoretical predications for a spatially flat, dark energy-dominated Lambda CDM cosmology. Thesis South pole DataCite Metadata Store (German National Library of Science and Technology) Austral South Pole Lambda ENVELOPE(-62.983,-62.983,-64.300,-64.300) |
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Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
English |
topic |
observations cosmic microwave background South Pole Physics cosmology |
spellingShingle |
observations cosmic microwave background South Pole Physics cosmology Reichardt, Christian L. A High Resolution Measurement of Temperature Anisotropies in the Cosmic Microwave Background Radiation with the Complete ACBAR Data Set |
topic_facet |
observations cosmic microwave background South Pole Physics cosmology |
description |
The Arcminute Cosmology Bolometer Array Receiver (ACBAR) is a 16-element spiderweb bolometer array operating at 150 GHz. Mounted on the 2.1m Viper telescope, ACBAR has dedicated four years to cosmic microwave background (CMB) observations at the South Pole. We describe the focal plane reconstruction and performance of ACBAR for the 2005 austral winter. We present a new CMB temperature anisotropy power spectrum for the complete ACBAR data set. The addition of data from the 2005 observing season expands the data set by 210%; and the sky coverage by 490%; over the previous ACBAR releases. The expanded data set allows us to derive a new set of band-power measurements with finer ℓ-resolution and dramatically smaller uncertainties. In particular, the band-power uncertainties have been reduced by more than a factor of two on angular scales encompassing the third and fourth acoustic peaks and the damping tail of the CMB power spectrum. The calibration has been significantly improved from 6%; to 2.2%; in temperature by using a direct comparison between CMB anisotropy maps measured by WMAP3 and ACBAR to transfer the WMAP dipole-based calibration to ACBAR. The resulting power spectrum is consistent with theoretical predications for a spatially flat, dark energy-dominated Lambda CDM cosmology. |
format |
Thesis |
author |
Reichardt, Christian L. |
author_facet |
Reichardt, Christian L. |
author_sort |
Reichardt, Christian L. |
title |
A High Resolution Measurement of Temperature Anisotropies in the Cosmic Microwave Background Radiation with the Complete ACBAR Data Set |
title_short |
A High Resolution Measurement of Temperature Anisotropies in the Cosmic Microwave Background Radiation with the Complete ACBAR Data Set |
title_full |
A High Resolution Measurement of Temperature Anisotropies in the Cosmic Microwave Background Radiation with the Complete ACBAR Data Set |
title_fullStr |
A High Resolution Measurement of Temperature Anisotropies in the Cosmic Microwave Background Radiation with the Complete ACBAR Data Set |
title_full_unstemmed |
A High Resolution Measurement of Temperature Anisotropies in the Cosmic Microwave Background Radiation with the Complete ACBAR Data Set |
title_sort |
high resolution measurement of temperature anisotropies in the cosmic microwave background radiation with the complete acbar data set |
publisher |
California Institute of Technology |
publishDate |
2008 |
url |
https://dx.doi.org/10.7907/a0nq-td75 https://resolver.caltech.edu/CaltechETD:etd-12202007-130152 |
long_lat |
ENVELOPE(-62.983,-62.983,-64.300,-64.300) |
geographic |
Austral South Pole Lambda |
geographic_facet |
Austral South Pole Lambda |
genre |
South pole |
genre_facet |
South pole |
op_rights |
No commercial reproduction, distribution, display or performance rights in this work are provided. |
op_doi |
https://doi.org/10.7907/a0nq-td75 |
_version_ |
1766201457113038848 |