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Table 2:

400 SD high z sample.

Cluster
Obs ID z T (keV) $L_{\rm X}$ $c_{\rm SB}$ $R_{\rm src}$
(1) (2) (3) (4) (5) (6) (7)

WARP J0030.5+2618
5762 0.500 $\rm 5.62^{+1.53}_{-1.04}$ 1.65 0.040 $\pm$ 0.011 no
400d J1002+6858 5773 0.500 $\rm 6.86^{+1.01}_{-0.72}$ 2.41 0.060 $\pm$ 0.012 yes
WARP J1524.6+0957 1664 0.516 $\rm 4.59^{+0.65}_{-0.40}$ 2.29 0.032 $\pm$ 0.006 no
400d J1357+6232 5763, 7267 0.525 $\rm 5.29^{+0.61}_{-0.56}$ 1.87 0.054 $\pm$ 0.010 no
400d J1354-0221 4932, 5835 0.546 $\rm 6.82^{+1.59}_{-1.13}$ 4.57 0.043 $\pm$ 0.009 no
400d J1117+1744 4933, 5836 0.547 $\rm 5.99^{+1.41}_{-1.45}$ 0.78 0.041 $\pm$ 0.010 no
400d J1120+2326 3235 0.562 $\rm 5.80^{+0.79}_{-0.54}$ 5.06 0.027 $\pm$ 0.011 no
WARP J0216.5-1747 5760, 6393 0.578 $\rm 5.95^{+0.72}_{-0.72}$ 1.01 0.055 $\pm$ 0.014 no
400d J0521-2530 5758 0.581 $\rm 2.98^{+1.51}_{-0.91}$ 0.51 0.046 $\pm$ 0.007 no
400d J0956+4107 5294, 5759 0.587 $\rm 6.86^{+1.01}_{-0.72}$ 2.01 0.040 $\pm$ 0.007 no
400d J0328-2140 5755, 6258 0.590 $\rm 5.54^{+0.61}_{-0.48}$ 2.47 0.062 $\pm$ 0.009 no
WARP J1120.1+4318* 5771 0.600 $\rm 4.68^{+0.53}_{-0.46}$ 4.37 0.063 $\pm$ 0.005 no
ZwCl 1332.8+5043 5772 0.620 $\rm 5.14^{+1.26}_{-1.10}$ 2.42 0.068 $\pm$ 0.017 no
RDCS J0542-4100* 914 0.642 $\rm 6.63^{+0.83}_{-0.73}$ 3.55 0.043 $\pm$ 0.007 no
400d J1202+5751 5757 0.677 $\rm 5.96^{+1.35}_{-0.91}$ 2.11 0.030 $\pm$ 0.008 no
400d J0405-4100 7191 0.686 $\rm 3.28^{+0.68}_{-0.64}$ 7.78 0.073 $\pm$ 0.009 no
400d J1221+4918 1662 0.700 $\rm 7.45^{+1.04}_{-0.64}$ 3.60 0.026 $\pm$ 0.006 yes
400d J0230+1836 5754 0.799 $\rm 5.78^{+1.23}_{-0.74}$ 3.28 0.036 $\pm$ 0.009 no
WARP J0152.7-1357N* 913 0.833 $\rm 5.30^{+1.05}_{-0.78}$ 3.41 0.027 $\pm$ 0.008 no
WARP J1226.9+3332* 3180, 5014 0.890 $\rm 12.34^{+1.20}_{-0.95}$ 9.68 0.086 $\pm$ 0.007 yes

Notes. (1) Cluster name; (2) Chandra observation identifier; (3) redshift; (4) spectral temperature; (5) total rest-frame soft-band luminosity in units 1044 [erg s-1]; (6) surface brightness concentration; and (7) presence of a radio source in the cluster center according to NVSS. (*) Also in the RDCS+WARPS.


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