\begin{table}%t4
\caption{Best fit spectral parameters using an exponential cut-off power-law model.}\label{table=cut}
%\centerline
 {\small \begin{tabular}{lcccc}
\hline
\hline\noalign{\smallskip}
\multicolumn{1}{c}{Name} &
\multicolumn{1}{c}{$\Gamma$} &
\multicolumn{1}{c}{$E_{\rm cut-off}$} &
\multicolumn{1}{c}{$C$} &
\multicolumn{1}{c}{$\chi^{2}$/d.o.f.} \\
\multicolumn{1}{c}{(1)} &
\multicolumn{1}{c}{(2)} &
\multicolumn{1}{c}{(3)} &
\multicolumn{1}{c}{(4)} &
\multicolumn{1}{c}{(5)} \\
\hline\noalign{\smallskip}
LEDA~168563     & $\rm 1.59^{+0.08}_{-0.10}$ & $7\rm 3^{+152}_{-36}$ & $\rm 0.9^{+0.2}_{-0.3}$ & 500/487  \\   
IGR~J07597-3842 & $\rm 1.51^{+0.03}_{-0.04}$ & $\rm 64^{+40}_{-20}$  & $\rm 1.4^{+0.3}_{-0.3}$ & 327/338   \\
ESO~209-12      & $\rm 1.73^{+0.02}_{-0.03}$ & $>$60	     & $\rm 1.5^{+0.5}_{-0.4}$ & 497/507   \\
FRL~1146(AO3)   & $\rm 1.81^{+0.04}_{-0.04}$ & $>$45	& $\rm 1.3^{+0.7}_{-0.5}$ & 417/420   \\
FRL~1146(AO4)   & $\rm 1.61^{+0.09}_{-0.08}$ & $>$29	& $\rm 1.1^{+0.6}_{-0.4}$ & 422/437   \\
4U~1344-60       & $\rm 1.75^{+0.18}_{-0.14}$ & $>$78            & $\rm 0.8^{+0.2}_{-0.1}$ & 698/636  \\  
IGR~J16482-3036 & $\rm 1.53^{+0.04}_{-0.04}$ & $\rm 65^{+52}_{-24}$  & $\rm 0.7^{+0.2}_{-0.2}$ & 590/562   \\
IGR~J16558-5203 & $\rm 2.25^{+0.01}_{-0.01}$ & $>$134   & $\rm 2.9^{+0.7}_{-0.3}$ & 540/591   \\
IGR~J17418-1212 & $\rm 1.97^{+0.02}_{-0.02}$ & $>$170 & $\rm 1.6^{+0.3}_{-0.3}$ & 651/605  \\
IGR~J18027-1455 & $\rm 1.53^{+0.05}_{-0.05}$ & $\rm 108^{+75}_{-32}$ & $\rm 3.6^{+0.6}_{-0.5}$ & 341/315  \\ 
\hline
\end{tabular}}
\medskip
Note: (1): Galaxy name. (2): Power-law photon index. (3): Energy of the exponential cut-off in~keV. (4):  Value of the {\it XMM-Newton}/{\it INTEGRAL} cross-calibration constant. (5): Chi-squared and degrees of freedom.
\end{table}