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The Sunyaev-Zeldovich (SZ) effect was previously measured in the Coma cluster by the Owens Valley Radio Observatory and Millimeter and IR Testa Grigia Observatory experiments and recently also with the Wilkinson Microwave Anisotropy Probe satellite. We assess the consistency of these results and their implications on the feasibility of high-frequency SZ work with ground-based telescopes. The unique data set from the combined measurements at six frequency bands is jointly analyzed, resulting in a best-fit value for the Thomson optical depth at the cluster center, tau_{0}=(5.35 pm 0.67) 10^{-3}. The combined X-ray and SZ determined properties of the gas are used to determine the Hubble constant. For isothermal gas with a beta density profile we derive H_0 = 84 pm 26 km/(scdot Mpc); the (1sigma) error includes only observational SZ and X-ray uncertainties.
Observations from the first flight of the Medium Scale Anisotropy Measurement (MSAM1-92) are analyzed to search for the Sunyaev-Zeldovich (SZ) effect towards the Coma cluster. This balloon-borne instrument uses a $28arcmin$ FWHM beam and a three posi
We present an interferometric measurement of the Sunyaev-Zeldovich effect (SZE) at 1 cm for the galaxy cluster Abell 2163. We combine this data point with previous measurements at 1.1, 1.4, and 2.1 mm from the SuZIE experiment to construct the most c
The Planck collaboration has recently published precise and resolved measurements of the Sunyaev-Zeldovich effect in Abell 1656 (the Coma cluster of galaxies), so directly gauging the electron pressure profile in the intracluster plasma. On the other
Studying galaxy clusters through their Sunyaev-Zeldovich (SZ) imprint on the Cosmic Microwave Background has many important advantages. The total SZ signal is an accurate and precise tracer of the total pressure in the intra-cluster medium and of clu
X-ray observations of an entropy floor in nearby groups and clusters of galaxies offer evidence that important non-gravitational processes, such as radiative cooling and/or preheating, have strongly influenced the evolution of the intracluster medium