H₀ from Cosmic Background Imager Observations of the Sunyaev-Zel’dovich Effect in Nearby Clusters.

Author: Udomprasert, Patricia Simcoe

Year: 2004

Degree: Dissertation (Ph.D.)

Advisor: Readhead, Anthony C. S.

Committee Members: Lange, Andrew E.; Blain, Andrew W.; Djorgovski, George; Phinney, E. Sterl; Readhead, Anthony C. S.

Option: Astronomy

DOI: 10.7907/VR2Z-MP09

Abstract

We present H₀ results from Cosmic Background Imager (CBI) observations of the Sunyaev-Zeldovich Effect (SZE) in 7 galaxy clusters, A85, A399, A401, A478, A754, A1651, and A2597. These observations are part of a program to study a complete, volume-limited sample of low-redshift (z < 0.1), X-ray selected clusters. Our focus on nearby objects allows us to study a well-defined, orientation unbiased sample, minimizing systematic errors due to cluster asphericity. We use density models derived from ROSAT imaging data and temperature measurements from ASCA and BeppoSAX spectral observations. We quantify in detail sources of error in our derivation of H₀, including calibration of the CBI data, density and temperature models from the X-ray data, Cosmic Microwave Background (CMB) primary anisotropy fluctuations, and residuals from radio point source subtraction. From these 7 clusters we obtain a result of Ho = 67+30-18(ran)+15-6(sys) km/s-1 Mpc-1 for an unweighted sample average. The respective quoted errors are random and systematic uncertainties at 68% confidence. The dominant source of error is confusion from intrinsic anisotropy fluctuations. We present results from simulations of an eigenmode weighting analysis that reduce the uncertainties due to CMB in h-1/2 by ~30%.

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