Mapping of the SZ effect in the cluster Cl 0016+16 with the Ryle Telescope
arXiv:astro-ph/0102496 · doi:10.1046/j.1365-8711.2002.05050.x
Abstract
We have mapped the high-redshift (z = 0.546) cluster Cl 0016+16 with the Ryle Telescope at 15 GHz. The Sunyaev-Zel'dovich decrement is clearly detected, and resolved. We combine our data with an X-ray image from ROSAT, and a gas temperature from ASCA to estimate the Hubble Constant H0 = 69 +21/-16 km/s/Mpc for an Omega_M=1.0 cosmology or H0 = 84 +25/-19 km/s/Mpc for Omega_M=0.3 and Omega_Lambda=0.7.
arXiv comment10 pages, 2 tables, 6 figures Submitted to MNRAS
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- The Sunyaev-Zeldovich effect in CMB-calibrated theories applied to the Cosmic Background Imager anisotropy power at l > 2000
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- Cluster Sunyaev-Zeldovich Effect Scaling Relations
- Bayesian modelling of clusters of galaxies from multi-frequency pointed Sunyaev--Zel'dovich observations
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- AGN heating, thermal conduction and Sunyaev-Zeldovich effect in galaxy groups and clusters
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- The temperature and distribution of gas in CL 0016+16 measured with XMM-Newton
- Measurement of the Sunyaev-Zel'dovich Increment in Massive Galaxy Clusters
- A maximum-likelihood approach to removing radio sources from SZ observations, with application to Abell 611
- Joint analysis of X-ray and Sunyaev Zel'dovich observations of galaxy clusters using an analytic model of the intra-cluster medium
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