Table 3: Spectral fits of the subset S3.
Source ID Inst. $N_{\rm H}$a $\Gamma $ $\chi^2$/d.o.f. $N_{\rm H}$a $\Gamma $ $\chi^2$/d.o.f. Fb Fub Rc log  $L_{2-10~\rm keV}$d
    z = 1 z = 2    
03120029 pm <0.56 1.9 8.2/8 <1.51 1.9 8.2/8 1.2 1.2 18.8  
03120031 pm 1.58 $\pm_{0.93}^{1.59}$ 1.9 0.9/6 4.38 $\pm_{2.60}^{4.76}$ 1.9 0.9/5 1.7 1.8 23.6 44.29
03120045 pm 3.20 $\pm_{1.82}^{3.34}$ 1.9 6.1/8 9.29 $\pm_{5.46}^{10.76}$ 1.9 6.2/8 2.8 3.0 24.4 44.81
03120065 pm 1.15 $\pm_{1.15}^{0.28}$ 1.9 6.6/9 3.22 $\pm_{3.22}^{7.10}$ 1.9 6.6/9 1.6 1.7 $\geq$24 43.98
26900014 pm 0.25 $\pm_{0.25}^{0.64}$ 2.24 $\pm_{0.61}^{0.80}$ 7.0/9 0.69 $\pm_{0.69}^{1.73}$ 2.24 $\pm_{0.61}^{0.79}$ 7.0/9 1.4 1.4 21.6  
26900075 pm 10.2 $\pm_{5.9}^{14.2}$ 1.9 0.3/4 32.9 $\pm_{20.2}^{44.7}$ 1.9 0.4/4 3.3 4.0 24.6 45.05
05370010 pm <0.45 1.82 $\pm_{0.52}^{0.75}$ 12.3/15 <1.26 1.83 $\pm_{0.30}^{0.52}$ 12.2/15 2.7 2.7 22.4  
05370012 pm 0.03 $\pm_{0.03}^{0.42}$ 1.83 $\pm_{0.31}^{0.52}$ 15.9/14 <1.24 1.83 $\pm_{0.30}^{0.52}$ 15.9/14 2.4 2.4 22.5  
05370022 pm 0.18 $\pm_{0.18}^{0.38}$ 1.9 7.5/6 0.51 $\pm_{0.51}^{1.04}$ 1.9 7.5/6 2.8 2.8 $\geq$23.0 44.19
05370054 pm 0.78 $\pm_{0.78}^{5.69}$ 1.69 $\pm_{0.80}^{1.92}$ 4.6/8 1.68 $\pm_{1.68}^{14.60}$ 1.61 $\pm_{0.71}^{1.73}$ 4.7/8 2.1 2.1 25.0 44.88
05370111 pm 7.04 $\pm_{4.12}^{9.66}$ 1.9 3.3/8 20.1 $\pm_{12.2}^{26.5}$ 1.9 3.8/8 2.1 2.3 24.5 44.69
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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