\begin{table}%T4
\par
\caption{Spectral fits of the subset S4.}\label{t4}
%\centerline
{
\begin{tabular}{l|c|c|c|c|c|c|c|c|c}
\hline\hline
Source ID &  Type  &  $z$   &   Inst.&  $N_{\rm H}$$^a$ & $\Gamma$ & Cst/bins
&  $F^b$ &  $F_u$$^b$  & log~$L_{2-10~\rm keV}$$^c$ \\
\hline
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\\
\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}