This thesis presents a measurement of the Sunyaev-Zeldovich effect in the Coma cluster of galaxies. The observed effect is ΔT[subscript 0,obs] = -302.1±48μK, and was measured at a frequency of 32GHz with the 5.5m telescope at the Owens Valley Radio Observatory. Interpreted in the context of existing X-ray models, I derive a peak central SZ effect of ΔT[subscript 0,peak] = -495.3±78.7µK. With this interpretation, I also calculate a value of H[subscript 0] = 74.2±27.9kms[superscript -1]Mpc[superscript -1] for the Hubble constant. This is the first successful measurement of the SZ effect in a nearby cluster, an important advance because of the much better potential for its astronomical and cosmological interpretation
The Sunyaev-Zel'dovich (SZ) effect spectrum crosses through a null where ΔT CMB = 0 near ν0 = 217 GH...
International audienceWe report the direct detection of the kinetic Sunyaev-Zel’dovich (kSZ) effect ...
In a search for evidence of the short wavelength increment in the Sunyaev–Zel'dovich (SZ) effect, we...
We have measured the Sunyaev-Zeldovich (SZ) effect toward the Coma Cluster (A1656) with the Millimet...
The Sunyaev-Zeldovich (SZ) effect was previously measured in the Coma cluster by the OVRO and MITO e...
The Sunyaev-Zel'dovich (SZ) effect was previously measured in the Coma Cluster by the Owens Valley R...
We present an improved measurement of the Hubble Constant (H 0) based on observations of the Sunyaev...
The Sunyaev-Zeldovich (S-Z) effect is a spectral distortion of the cosmic background radiation induc...
Compton scattering of the cosmic microwave background radiation by electrons in the hot gas in clust...
In this paper, we recall the basics of the the Sunyaev-Zeldovich effect from groups and clusters of ...
Clusters of galaxies provide us with a sensitive probe with which to study the Universe. Their mass ...
This work is concerned with the Sunyaev-Zel'dovich (S-Z) effect in clusters of galaxies and its use ...
The Sunyaev–Zeldovich (SZ) effect is a spectral effect on the COSMIC MICROWAVE BACKGROUND (CMB) caus...
International audienceThe Sunyaev-Zel'dovich (SZ) effect is a spectral distortion of the cosmic micr...
The Sunyaev-Zeldovich (SZ) effect is a spectral distortion in the Cosmic Microwave Background (CMB),...
The Sunyaev-Zel'dovich (SZ) effect spectrum crosses through a null where ΔT CMB = 0 near ν0 = 217 GH...
International audienceWe report the direct detection of the kinetic Sunyaev-Zel’dovich (kSZ) effect ...
In a search for evidence of the short wavelength increment in the Sunyaev–Zel'dovich (SZ) effect, we...
We have measured the Sunyaev-Zeldovich (SZ) effect toward the Coma Cluster (A1656) with the Millimet...
The Sunyaev-Zeldovich (SZ) effect was previously measured in the Coma cluster by the OVRO and MITO e...
The Sunyaev-Zel'dovich (SZ) effect was previously measured in the Coma Cluster by the Owens Valley R...
We present an improved measurement of the Hubble Constant (H 0) based on observations of the Sunyaev...
The Sunyaev-Zeldovich (S-Z) effect is a spectral distortion of the cosmic background radiation induc...
Compton scattering of the cosmic microwave background radiation by electrons in the hot gas in clust...
In this paper, we recall the basics of the the Sunyaev-Zeldovich effect from groups and clusters of ...
Clusters of galaxies provide us with a sensitive probe with which to study the Universe. Their mass ...
This work is concerned with the Sunyaev-Zel'dovich (S-Z) effect in clusters of galaxies and its use ...
The Sunyaev–Zeldovich (SZ) effect is a spectral effect on the COSMIC MICROWAVE BACKGROUND (CMB) caus...
International audienceThe Sunyaev-Zel'dovich (SZ) effect is a spectral distortion of the cosmic micr...
The Sunyaev-Zeldovich (SZ) effect is a spectral distortion in the Cosmic Microwave Background (CMB),...
The Sunyaev-Zel'dovich (SZ) effect spectrum crosses through a null where ΔT CMB = 0 near ν0 = 217 GH...
International audienceWe report the direct detection of the kinetic Sunyaev-Zel’dovich (kSZ) effect ...
In a search for evidence of the short wavelength increment in the Sunyaev–Zel'dovich (SZ) effect, we...