All Tables

Table 1: The luminosity-redshift bins used for the selection of the sample (for H₀=70 km s^-1 Mpc^-1, $\Omega _{\rm m} = 0.3$ , $\Omega _{\Lambda }=0.7$ ).
Table 2: The luminosity-redshift bins used for the alternatively constructed test selection function.
Table 3: The REFLEX XMM Large Program cluster sample.
Table 4: The additional clusters contained in the redshift-luminosity bins, which are not part of the observed cluster sample with more than30 detected X-ray counts in the RASS and $N_{\rm H} \le 6\times 10^{20}$ cm^-2.
Table 5: Overview of the XMM-Newton observation parameters of the cluster sample, up to and including AO4.