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Interferometric Observation of Cosmic Microwave Background Anisotropies
Martin White, John E. Carlstrom, Mark Dragovan +1
We present a formalism for analyzing interferometric observations of Cosmic Microwave Background (CMB) anisotropy and polarization data. The formalism is based upon the ell-space e…
Radio Sources in Galaxy Clusters at 28.5 GHz
Asantha R. Cooray, Laura Grego, William L. Holzapfel +2
We present serendipitous detections of radio sources at 28.5 GHz (1 cm), which resulted from our program to image thermal Sunyaev-Zeldovich (SZ) effect in 56 galaxy clusters. We fi…
Measurement of the Hubble Constant from X-ray and 2.1 mm Observations of Abell 2163
W. L. Holzapfel, M. Arnaud, P. A. R. Ade +6
We report 2.1 mm observations of the Sunyaev-Zel'dovich (S-Z) effect; these observations confirm our previous detection of a decrement in the Cosmic Microwave Background intensity…
Limits on the Peculiar Velocities of Two Distant Clusters Using the Kinematic Sunyaev-Zel'dovich Effect
W. L. Holzapfel, P. A. R. Ade, S. E. Church +4
We report millimeter-wavelength observations of the Sunyaev-Zel'dovich (S-Z) effect in two distant galaxy clusters. A relativistically correct analysis of the S-Z data is combined…
The Sunyaev-Zel'dovich Infrared Experiment: A Millimeter-wave Receiver for Cluster Cosmology
W. L. Holzapfel, T. M. Wilbanks, P. A. R. Ade +5
Measurements of the Sunyaev-Zel'dovich (S-Z) effect towards distant clusters of galaxies can be used to determine the Hubble constant and the radial component of cluster peculiar v…
An Upper Limit to Arcminute Scale Anisotropy in the Cosmic Microwave Background Radiation at 142 GHz
S. E. Church, K. M. Ganga, P. A. R. Ade +4
We present limits to anisotropies in the cosmic microwave background radiation (CMB) at angular scales of a few arcminutes. The observations were made at a frequency of 142 GHz usi…