Very Small Array observations of the Sunyaev-Zel'dovich effect in nearby galaxy clusters

Details Very Small Array observations of the Sunyaev-Zel'dovich effect in nearby galaxy clusters Very Small Array observations of the Sunyaev-Zel'dovich effect in nearby galaxy clusters

2004-05-28

arxiv.org/abs/astro-ph/0405582v2

Mon.Not.Roy.Astron.Soc. 359 (2005) 16-30

Astronomy and Astrophysics

Astrophysics

Replaces earlier version. 16 pages, 5 figures, LaTeX. Minor revisions to content, accepted by MNRAS for publication

Scientific paper

10.1111/j.1365-2966.2005.08696.x

We present VSA observations (~34GHz) on scales ~20 arcmin towards a complete, X-ray-flux-limited sample of seven clusters at redshift z<0.1. Four have significant SZ detections in the presence of CMB primordial anisotropy. We use a bayesian MCMC method for inference from the VSA data, with X-ray priors on cluster positions and temperatures, and radio priors on sources. We make assumptions of beta-model gas distributions and of hydrostatic equilibrium, to evaluate probability densities for the gas mass and total mass out to r_200. Our combined estimate of the gas fraction is 0.08^{+0.06}_{-0.04}h^{-1} The random errors are poor (note that the errors are higher than would have been obtained with the usual chi-squared method) but the control of bias is good. We have described the MCMC analysis method specifically in terms of SZ but hope the description will be of more general use. We find that the effects of primordial CMB contamination tend to be similar in the estimates of both the gas mass and total mass over our narrow range of angular scales, so that there is little effect of primordials on the gas fraction determination. Using our total mass estimates we find a normalisation of the mass-temperature relation based on the profiles from the VSA cluster pressure maps that is in good agreement with recent M-T determinations from X-ray cluster measurements.

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