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Table 2:

Properties of the local cluster sample from Vikhlinin et al. (2006).
Cluster z $kT_{\rm gas}$ R500 $f_{\rm gas}$
    keV kpc (<R500)
A133 0.057 $4.15\pm0.07$ $1027\pm38$ $0.087\pm0.006$
A1795 0.062 $6.10\pm0.06$ $1320\pm47$ $0.108\pm0.006$
A2029 0.078 $8.46\pm0.09$ $1419\pm32$ $0.128\pm0.007$
A478 0.088 $7.95\pm0.14$ $1398\pm62$ $0.125\pm0.011$
A1413 0.143 $7.38\pm0.12$ $1377\pm49$ $0.112\pm0.007$
A907 0.160 $5.96\pm0.08$ $1149\pm32$ $0.129\pm0.006$
A383 0.188 $4.80\pm0.12$ $983\pm34$ $0.129\pm0.007$
A2390 0.230 $8.90\pm0.17$ $1489\pm50$ $0.147\pm0.009$
Column (1): name; Col. (2): adopted redshift; Col. (3): best-fit spectral temperature; Col. (4): R500; Col. (5): gas mass fraction within R500. A cosmology of $(H_0, \Omega _{\rm m}, \Omega _{\Lambda }) = (70$ km s-1 Mpc -1, 0.3, 0.7) is adopted here.

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