\begin{table}%t3
\caption{Best fit spectral parameters using an absorbed power-law, a soft thermal component and a Gaussian narrow line.}\label{table=po}
%\centerline
 {\small\begin{tabular}{lccccccccc}
\hline
\hline\noalign{\smallskip}
\multicolumn{1}{c}{Name} &
\multicolumn{1}{c}{$N_{\rm H, int}$} &
\multicolumn{1}{c}{$\Gamma$} &
\multicolumn{1}{c}{$E_\alpha$} &
\multicolumn{1}{c}{$EW_\alpha$} &
\multicolumn{1}{c}{$C$} &
\multicolumn{1}{c}{$kT$/$\Gamma_{\rm soft}$} &
\multicolumn{1}{c}{$F_{\rm 2-10}$} &
\multicolumn{1}{c}{$F_{\rm 20-100}$} &
\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)} &
\multicolumn{1}{c}{(6)} &
\multicolumn{1}{c}{(7)} &
\multicolumn{1}{c}{(8)} &
\multicolumn{1}{c}{(9)} &
\multicolumn{1}{c}{(10)} \\
\hline
LEDA~168563 & --  & $\rm 1.68^{+0.05}_{-0.05}$ & $\rm 6.44^{+0.09}_{-0.11}$ & $<$52	 & $\rm 0.6^{+0.2}_{-0.2}$ & $\rm 3.8^{+0.2}_{-0.2}$    & 1.46 & 5.6  & 507/488  \\	
IGR~J07597-3842    & --   &$\rm 1.57^{+0.01}_{-0.02}$ & $\rm 6.44^{+0.04}_{-0.06}$ & $\rm 48^{+39}_{-13}$ & $\rm 0.8^{+0.1}_{-0.1}$ & $\rm 0.09^{+0.01}_{-0.01}$ & 1.56 & 3.6  & 352/339  \\
ESO~209-12 & --   & $\rm 1.73^{+0.02}_{-0.03}$ & $\rm 6.39^{+0.04}_{-0.05}$ & $\rm 163^{+57}_{-62}$ & $\rm 1.2^{+0.3}_{-0.2}$ & $\rm 0.05^{+0.01}_{-0.01}$ & 0.83 & 1.9  & 500/508  \\
FRL~1146(AO3) & $\rm 0.36^{+0.05}_{-0.05}$ & $\rm 1.84^{+0.05}_{-0.05}$ & $\rm 6.39^{+0.07}_{-0.07}$ & $<$146 & $\rm 1.1^{+0.3}_{-0.3}$ & $\rm 0.15^{+0.02}_{-0.01}$ & 1.15 & 2.0  & 418/421  \\
FRL~1146(AO4)$^{\dag}$& $\rm 0.28^{+0.04}_{-0.04}$ & $\rm 1.69^{+0.04}_{-0.06}$ & $\rm 6.37^{+0.03}_{-0.03}$ & $\rm 111^{+37}_{-38}$ & $\rm 0.7^{+0.2}_{-0.2}$ & $\rm 0.16^{+0.01}_{-0.01}$ & 1.21 & 2.0 & 424/438  \\
$\rm 4U~1344-60^{\dag}$ & $\rm 0.98^{+0.14}_{-0.17}$ & $\rm 2.04^{+0.08}_{-0.09}$ & $\rm 6.41^{+0.03}_{-0.04}$ & $\rm 51^{+20}_{-19}$ & $\rm 0.9^{+0.1}_{-0.1}$ & --  & 3.58 & 6.6 & 706/638 \\  
IGR~J16482-3036    & $\rm 0.09^{+0.01}_{-0.01}$ & $\rm 1.59^{+0.02}_{-0.03}$ & $\rm 6.46^{+0.06}_{-0.06}$ & $\rm 96^{+32}_{-72}$ & $\rm 0.5^{+0.1}_{-0.1}$ & --  & 1.97 & 1.9 & 607/563  \\
IGR~J16558-5203$^{\dag}$& -- & $\rm 2.25^{+0.03}_{-0.03}$ & $\rm 6.48^{+0.05}_{-0.06}$ & $\rm 61^{+50}_{-34}$ & $\rm 2.7^{+0.5}_{-0.5}$ & -- & 1.05 & 2.8 & 540/592  \\
IGR~J17418-1212$^{\dag}$& $\rm 0.13^{+0.01}_{-0.01}$ & $\rm 1.98^{+0.01}_{-0.02}$ & $\rm 6.28^{+0.04}_{-0.05}$ & $\rm 51^{+37}_{-20}$ & $\rm 1.5^{+0.3}_{-0.3}$ & --  & 1.29 & 2.1 & 651/606 \\
IGR~J18027-1455$^{\dag}$& $\rm 0.41^{+0.05}_{-0.05}$ & $\rm 1.61^{+0.04}_{-0.04}$ & $\rm 6.39^{+0.01}_{-0.03}$ & $\rm 134^{+33}_{-34}$ & $\rm 2.9^{+0.4}_{-0.3}$ & $\rm 0.19^{+0.08}_{-0.07}$ & 0.61 & 4.6 & 363/316 \\ 
\hline
\end{tabular}}
\medskip
Note: (1): Galaxy name. (2): Intrinsic fully-covering column density in units of 10$^{22}$~cm$^{-2}$. (3): Power-law photon index. (4): Energy of the FeK line, in~keV. (5): Equivalent width of the FeK line, in~eV. (6): Value of the {\it XMM-Newton}/{\it INTEGRAL} cross-calibration constant. (7): Temperature of the thermal component ($kT$ in~keV) or photon index of the soft power-law component ($\Gamma_{\rm soft}$) in the case of LEDA~168563. (8-9): Model fluxes in the 2--10~keV and 20--100~keV bands in units of 10$^{-11}$~erg~cm$^{-2}$~s$^{-1}$. (10): Chi-squared and degrees of freedom. $\dag$: Sources with extra spectral components (see Sect.~4).
\end{table}