All Tables

Table 1: Observations excluded from the sample due to high soft proton contamination.
Table 2: Observations of clusters that show evidence of recent and strong interactions.
Table 3: Physical properties and observation details for the 48 clusters of our sample.
Table 4: Mean temperature values rescaled by ${k}T_{\rm M}$ and corrected for the biases discussed in the text, for each interval in units of R₁₈₀.
Table A.1: Best fit parameters for the NXB broken power law. $\Gamma _1$ and $\Gamma _2$ are the slopes below and above the break energy, $E_{\rm B}$ .
Table A.2: Instrumental emission lines in the 0.7-10.0 keV energy band.
Table B.1: Best fit results for the analysis of blank field observations in the 10 $^\prime$ -12 $^\prime$ ring.
Table B.2: Correction factors.