Table 5: Spectral fits of the subset S5.
Source ID Inst. $N_{\rm H}$a $\Gamma $ Cst/bins $N_{\rm H}$a $\Gamma $ Cst/bins Fb Fub Rc log  $L_{2-10~\rm keV}$d
    z = 1 z = 2    
03120036 p 1.15 $\pm_{0.98}^{1.35}$ 1.9 12.3/18 3.22 $\pm_{2.72}^{3.93}$ 1.9 13.1/18 1.9 1.9 24.6 44.79
03120124 m 5.26 $\pm_{3.27}^{5.54}$ 1.9 11.0/17 15.8 $\pm_{10.1}^{18.6}$ 1.9 11.1/17 2.2 2.4 22.5  
26900029 pm 0.75 $\pm_{0.57}^{0.90}$ 1.9 14.2/19 2.03 $\pm_{1.53}^{2.60}$ 1.9 14.3/19 2.8 2.8 25.1 45.11
05370037 p 1.37 $\pm_{0.93}^{1.82}$ 1.9 17.9/19 4.09 $\pm_{2.83}^{4.77}$ 1.9 17.5/19 4.4 4.5 21.5  
05370060 pm 0.90 $\pm_{0.90}^{1.93}$ 1.9 18.5/23 2.41 $\pm_{2.41}^{5.45}$ 1.9 18.5/23 1.0 1.0 23.9 44.11
05370072 pm 5.65 $\pm_{3.38}^{6.01}$ 1.9 15.6/25 16.9 $\pm_{10.4}^{19.1}$ 1.9 15.6/25 1.0 1.1 $\geq$24 44.16
05370091 m 24.7 $\pm_{19.4}^{54.9}$ 1.9 24.6/22 55.5 $\pm_{40.3}^{98.4}$ 1.9 25.0/22 4.2 5.7 23.7 44.26
0537011b m 34.0 $\pm_{24.9}^{61.6}$ 1.9 7.7/11 66.4 $\pm_{46.3}^{86.2}$ 1.9 9.2/11 1.4 2.0 21.7  
05370153 pm 10.3 $\pm_{7.1}^{16.0}$ 1.9 25.2/24 34.2 $\pm_{23.9}^{48.0}$ 1.9 25.2/24 1.2 1.4 $\geq$24.6 44.54
05370157 pm 11.4 $\pm_{5.3}^{9.0}$ 1.9 27.3/26 33.0 $\pm_{15.9}^{24.9}$ 1.9 28.5/26 1.4 1.8 $\geq$24.5 44.52
05370162 pm 5.26 $\pm_{4.00}^{11.00}$ 1.9 32.5/20 15.4 $\pm_{12.2}^{36.7}$ 1.9 32.7/20 1.3 1.5 21.6  
0537042b m 8.32 $\pm_{4.63}^{18.90}$ 1.9 15.6/13 22.8 $\pm_{12.8}^{36.4}$ 1.9 16.5/13 2.2 2.5 21.5  
0537052b m 7.13 $\pm_{3.93}^{6.35}$ 1.9 11.7/14 22.8 $\pm_{13.0}^{20.9}$ 1.9 11.4/14 1.7 2.0 23.7 44.34
a $N_{\rm H}$ in source frame, z=1 or z=2, units of 1022 cm-2; b Flux in the 2-10 keV band, F: observed, Fu: corrected for absorption, in units of 10-14 erg cm-2 s-1; c R magnitude of optical counterpart; d Log of the luminosity in units of erg s-1, only for sources with R greater than 23, for the redshift values given in Table 7 (see Sect. 4.2).


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