Table 6.
Cluster scaling laws used in Sect. 5.
| Law | X0 | α | γ | Scatter |
|---|---|---|---|---|
| (natural log) | ||||
| T300 kpc − M500, WL | 2.46 ± 0.65 keV | 0.85 ± 0.39 | 0.32 ± 0.75 | 0.13 |
 |
(20.9 ± 5.0) ×1041 erg.s−1 | 2.63 ± 0.34 | 2.17 ± 0.94 | 0.38 |
| rc − r500 | 0.15 | – | – | 0.1 |
Notes. We disperse over the luminosity, temperature, and core radius distributions in this case. Uncertainties on parameters indicate that these parameters are left free during the analysis. The values shown in this table are calculated assuming Ωm = 0.28 and h = 0.7. During the analysis, the parameter means and covariances are rescaled as a function of cosmology as described in Sect. 5.
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