Table 4: Spectral fits of the subset S4.
Source ID Type z Inst. $N_{\rm H}$a $\Gamma $ Cst/bins Fb Fub log  $L_{2-10~\rm keV}$c
03120016 AGN2* 0.841 pm 35.5 $\pm_{21.6}^{43.1}$ 1.9 22.6/24 3.1 5.3 44.23
03120035 AGN1 1.272 m 0.23 $\pm_{0.23}^{2.15}$ 1.9 19.3/20 1.4 1.4 44.09
03120127 AGN1 2.251 pm <115 1.9 15.6/18 3.4 3.4 45.07
03120181 ELG 0.709 pm 24.6 $\pm_{20.3}^{40.2}$ 1.9 14.0/14 1.2 2.0 43.63
03120501 ETG 0.205 m uncons 1.9 16.5/20 1.3 1.3 42.18
26900072 ELG 1.389 p 59.3 $\pm_{49.5}^{77.7}$ 1.9 14.9/15 8.2 13.4 45.16
05370035 AGN1 0.897 p 0.18 $\pm_{0.18}^{0.85}$ 1.9 13.3/11 0.9 0.9 43.55
05370078 AGN1 1.622 m 14.2 $\pm_{10.0}^{48.4}$ 1.9 24.5/23 2.0 2.3 44.56
05370175 AGN1 1.246 pm 50.7 $\pm_{33.3}^{60.3}$ 1.9 21.9/22 2.5 4.1 44.53
0537052a AGN1 1.665 pm 0.83 $\pm_{0.83}^{1.36}$ 1.9 31.6/20 0.8 0.8 44.12
15800025 ELG 0.470 m 0.29 $\pm_{0.28}^{0.61}$ 1.9 16.3/15 1.9 1.9 43.18
15800062 AGN2 1.568 m 26.3 $\pm_{18.1}^{44.7}$ 1.9 25.2/18 2.8 3.4 44.69
15800092 ELG 0.993 m 16.8 $\pm_{9.0}^{16.0}$ 1.9 28.6/20 3.3 4.2 44.3
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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