Using SuZIE arcminute-scale CMB anisotropy data to probe open and flat-ΛCDM cosmogonies

Abstract

We use arcminute-scale data from the Sunyaev-Zel'dovich Infrared Experiment to set limits on anisotropies in the cosmic microwave background radiation in open and spatially-flat-Lambda cold dark matter cosmogonies. There are no 2-sigma detections for the models tested. The upper limits obtained are consistent with the amplitude of anisotropy detected by the COBE/DMR experiment.

17 pages including 4 postscript figures. Latex. Uses aaspp4. ApJ, in press

References in corpus (3)

• Measurement of the Hubble Constant from X-ray and 2.1 mm Observations of Abell 2163
• The Sunyaev-Zel'dovich Infrared Experiment: A Millimeter-wave Receiver for Cluster Cosmology
• Using SuZIE arcminute-scale CMB anisotropy data to probe open and flat-ΛCDM cosmogonies

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• Contributions to the Power Spectrum of Cosmic Microwave Background from Fluctuations Caused by Clusters of Galaxies
• Nonflat time-variable dark energy cosmology
• Inflation in a closed universe
• An Upper Limit to Arcminute Scale Anisotropy in the Cosmic Microwave Background Radiation at 142 GHz
• CMB Anisotropy Constraints on Open and Flat-Lambda CDM Cosmogonies from UCSB South Pole, ARGO, MAX, White Dish, and SuZIE Data
• CMB Anisotropy Correlation Function and Topology from Simulated Maps for MAP
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• MAX 4 and MAX 5 CMB anisotropy measurement constraints on open and flat-Lambda CDM cosmogonies
• Python I, II, and III CMB Anisotropy Measurement Constraints on Open and Flat-Lambda CDM Cosmogonies
• ARGO CMB Anisotropy Measurement Constraints on Open and Flat-Lambda CDM Cosmogonies
• Using White Dish CMB Anisotropy Data to Probe Open and Flat-Lambda CDM Cosmogonies
• CMB Telescopes and Optical Systems
• CMB Anisotropy Constraints on Flat-Lambda and Open CDM Cosmogonies from DMR, UCSB South Pole, Python, ARGO, MAX, White Dish, OVRO, and SuZIE Data
• OVRO CMB Anisotropy Measurement Constraints on Flat-Lambda and Open CDM Cosmogonies