\begin{table}%T1
\par
\caption{Spectral fits of the subset S1.}\label{t1}
%\centerline
{
\begin{tabular}{l|c|c|c|c|c|c|c|c|c}
\hline\hline
Source ID &  Type  &  $z$   &   Inst.&  $N_{\rm H}$$^a$ & $\Gamma$ &  $\chi^2$/d.o.f.
&  $F^b$ &  $F_u$$^b$ & log~$L_{2-10~\rm keV}$$^c$\\
\hline
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\\
\hline
\end{tabular}}
\par
\medskip
$^a$ $N_{\rm H}$ in source frame, units of 10$^{22}$~cm$^{-2}$;
$^b$ Flux in the 2--10~keV band, $F$: observed, $F_u$: corrected
for absorption, in units of 10$^{-14}$~erg~cm$^{-2}$~s$^{-1}$;
$^c$ Log of the luminosity in units of~erg~s$^{-1}$.
\end{table}