Table 1: Spectral fits of the subset S1.
Source ID Type z Inst. $N_{\rm H}$a $\Gamma $ $\chi^2$/d.o.f. Fb Fub log  $L_{2-10~\rm keV}$c
03120002 AGN1 1.187 pm <0.05 1.88 $\pm_{0.06}^{0.07}$ 190.0/183 41.0 41.3 45.48
03120003 AGN1 0.420 pm <0.03 1.98 $\pm_{0.11}^{0.12}$ 88.4/72 14.8 14.9 43.97
03120004 AGN1 0.890 pm <0.08 2.44 $\pm_{0.15}^{0.16}$ 62.6/53 5.2 5.2 44.43
03120005 AGN1 1.274 pm <0.14 1.83 $\pm_{0.15}^{0.16}$ 43.3/46 9.4 9.4 44.89
03120006 AGN2 0.680 pm <0.16 1.56 $\pm_{0.14}^{0.17}$ 33.1/39 10.8 10.8 44.24
03120007 AGN1 0.381 m 0.12 $\pm_{0.12}^{0.24}$ 1.51 $\pm_{0.35}^{0.41}$ 17.0/18 19.5 19.7 43.93
03120009 AGN1 1.522 pm <0.84 1.86 $\pm_{0.33}^{0.49}$ 16.4/19 2.4 2.4 44.49
03120010 AGN1 0.246 pm <0.14 2.69 $\pm_{0.48}^{0.79}$ 24.1/19 1.3 1.3 42.44
03120012 AGN1 0.507 pm <0.24 2.49 $\pm_{0.44}^{0.79}$ 20.0/16 2.1 2.2 43.43
03120013 AGN1 1.446 pm 0.71 $\pm_{0.71}^{2.10}$ 2.83 $\pm_{0.80}^{1.51}$ 18.4/14 0.8 0.8 44.34
03120014 ELG 0.206 pm <0.26 1.54 $\pm_{0.31}^{0.53}$ 21.5/18 5.3 5.3 42.78
03120017 ETG 0.320 pm 0.13 $\pm_{0.13}^{0.45}$ 2.28 $\pm_{0.66}^{1.15}$ 14.1/11 1.9 2.0 42.86
03120018 ETG 0.159 pm 0.46 $\pm_{0.46}^{0.84}$ 1.87 $\pm_{0.78}^{1.08}$ 22.4/14 2.4 2.5 42.23
03120020 ELG 0.964 pm <0.70 2.03 $\pm_{0.41}^{0.70}$ 9.5/12 2.4 2.4 44.07
03120021 AGN1 2.736 pm <4.19 1.53 $\pm_{0.52}^{0.69}$ 10.4/11 2.1 2.2 44.87
03120028 ELG 0.641 pm 0.54 $\pm_{0.54}^{2.70}$ 1.63 $\pm_{0.80}^{1.54}$ 9.8/12 2.2 2.2 43.51
26900001 AGN1 0.336 pm <0.06 1.78 $\pm_{0.14}^{0.20}$ 42.8/43 8.4 8.4 43.47
26900002 AGN1 0.850 pm 0.54 $\pm_{0.30}^{0.29}$ 1.63 $\pm_{0.24}^{0.28}$ 32.4/30 14.6 14.8 44.62
26900003 AGN1 0.433 pm <0.08 2.13 $\pm_{0.20}^{0.29}$ 33.1/34 6.7 6.7 43.68
26900004 AGN1 0.284 pm <0.05 2.03 $\pm_{0.21}^{0.26}$ 30.4/26 7.8 7.8 43.3
26900007 AGN1 1.234 pm <0.29 2.07 $\pm_{0.32}^{0.43}$ 14.9/12 2.1 2.1 44.29
26900010 AGN1 1.355 pm <0.38 1.91 $\pm_{0.37}^{0.47}$ 8.5/10 2.9 2.9 44.47
26900012 AGN1 0.433 pm 0.14 $\pm_{0.14}^{0.27}$ 2.66 $\pm_{0.69}^{1.09}$ 7.4/15 0.8 0.8 42.85
26900015 AGN1 1.610 pm 1.52 $\pm_{1.27}^{2.47}$ 2.72 $\pm_{0.74}^{1.28}$ 8.8/14 1.1 1.1 44.57
05370002 AGN1 1.244 pm <0.10 1.95 $\pm_{0.09}^{0.10}$ 85.0/96 15.5 15.5 45.13
05370003 AGN1 0.317 pm <0.10 2.04 $\pm_{0.19}^{0.23}$ 37.1/52 10.1 10.1 43.53
05370004 AGN1 0.894 pm <0.24 1.58 $\pm_{0.14}^{0.20}$ 55.9/47 8.1 8.1 44.39
05370005 AGN1 1.158 pm 0.16 $\pm_{0.16}^{0.69}$ 1.60 $\pm_{0.34}^{0.42}$ 15.7/14 11.1 11.1 44.79
05370007 AGN1 0.842 pm <0.14 1.91 $\pm_{0.25}^{0.34}$ 20.9/21 2.7 2.7 43.94
05370008 AGN2* 0.379 pm <0.18 2.29 $\pm_{0.33}^{0.48}$ 17.8/25 3.9 4.0 43.34
05370009 AGN1 0.770 pm 0.14 $\pm^{ 1.20 }_{0.14}$ 2.10 $\pm^{ 1.28}_{ 0.53}$ 16.8/16 2.2 2.2 43.81
05370013 AGN1 0.901 pm <0.39 1.85 $\pm^{ 0.53}_{
0.35}$ 11.5/11 3.0 3.0 44.04
05370014 AGN1 1.659 pm <1.32 1.25 $\pm_{0.35}^{0.54}$ 7.7/14 6.3 6.3 44.74
05370015 AGN1 0.880 pm 0.37 $\pm_{0.37}^{1.17}$ 2.32 $\pm_{0.78}^{1.53}$ 11.6/13 2.4 2.5 44.07
05370016 AGN2 0.995 pm 1.32 $\pm_{0.88}^{1.56}$ 2.05 $\pm_{0.52}^{0.81}$ 9.8/17 3.5 3.6 44.28
05370017 AGN1 0.904 pm <0.28 1.86 $\pm_{0.36}^{0.54}$ 6.4/9 2.7 2.7 44.0
05370021 ELG* 1.192 pm 0.16 $\pm_{0.16}^{1.50}$ 1.54 $\pm_{0.54}^{0.99}$ 9.0/11 3.9 3.9 44.34
05370024 ETG 0.075 pm <0.12 1.18 $\pm_{0.36}^{0.42}$ 19.0/12 4.0 4.0 41.72
0537011a AGN2 0.981 pm 1.33 $\pm_{0.90}^{1.50}$ 1.88 $\pm_{0.40}^{0.63}$ 26.7/16 4.1 4.2 44.29
50900020 AGN1 0.770 m 0.48 $\pm_{0.48}^{1.53}$ 2.42 $\pm_{0.87}^{1.51}$ 5.1/8 4.2 4.3 44.18
50900031 AGN1 0.556 m <0.10 1.83 $\pm_{0.64}^{0.67}$ 21.2/11 4.3 4.3 43.69
15800001 AGN1 1.211 m <0.31 2.12 $\pm_{0.22}^{0.36}$ 14.8/19 8.7 8.7 44.91
15800002 AGN1 0.848 m <0.13 1.94 $\pm^{ 0.30}_{
0.26 }$ 17.0/17 7.3 7.3 44.39
15800008 AGN1 1.151 m <1.42 1.43 $\pm_{0.44}^{0.76}$ 6.2/8 3.9 3.9 44.27
a $N_{\rm H}$ in source frame, 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 Log of the luminosity in units of erg s-1.


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