\begin{table}%t5
\caption{Best fit spectral parameters using a pexrav model.}\label{table=pex}
\small
%\centerline
 {\begin{tabular}{lccccc}
\hline
\hline\noalign{\smallskip}
\multicolumn{1}{c}{Name} &
\multicolumn{1}{c}{$\Gamma$} &
\multicolumn{1}{c}{$E_{\rm cut-off}$} &
\multicolumn{1}{c}{$R$} &
\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)} &
\multicolumn{1}{c}{(6)} \\
\hline\noalign{\smallskip}
LEDA~168563& $\rm 1.67^{+0.14}_{-0.17}$ & $>$41  & $<$1.69 & $\rm 0.7^{+0.9}_{-0.3}$ & 499/486 \\
IGR~J07597-3842 & $\rm 1.48^{+0.05}_{-0.03}$ & $\rm 52^{+32}_{-7}$ & $<$0.59 & $\rm 1.5^{+0.1}_{-0.2}$ & 328/338\\
ESO~209-12 & $\rm 1.71^{+0.02}_{-0.03}$ & $>$62  & $<$0.77 & $\rm 1.5^{+0.5}_{-0.5}$ & 497/506  \\      
FRL~1146(AO3)   & $\rm 2.13^{+0.09}_{-0.08}$ & $>$48  & $<$2.00 & $\rm 0.7^{+0.3}_{-0.2}$ & 407/419\\
FRL~1146(AO4)   & $\rm 1.68^{+0.06}_{-0.06}$ & $>$30 & $<$2.63 & $\rm 0.9^{+0.8}_{-0.4}$ & 421/436\\
4U~1344-60       & $\rm 1.78^{+0.14}_{-0.15}$ & $>$94  & $<$2.83 & $\rm 0.7^{+0.2}_{-0.3}$ & 698/635\\
IGR~J16482-3036 & $\rm 1.62^{+0.07}_{-0.07}$ & $\rm 87^{+97}_{-22}$& $\rm 1.6^{+1.5}_{-1.1}$ & $0.4^{+0.2}_{-0.1}$ & 591/561 \\
IGR~J16558-5203 & $\rm 2.30^{+0.04}_{-0.05}$ & -- & $<$9.63 & $\rm 1.1^{+1.6}_{-0.6}$ & 537/590 \\
IGR~J17418-1212 & $\rm 2.07^{+0.05}_{-0.05}$ & -- & $\rm 2.0^{+1.1}_{-0.9}$ & $\rm 0.9^{+0.2}_{-0.2}$ & 637/605 \\
IGR~J18027-1455 & $\rm 1.48^{+0.01}_{-0.01}$ & $>$400  & $<$0.35  & $\rm 3.8^{+0.7}_{-0.7}$ & 338/314 \\
\hline
\end{tabular}}
\medskip
Note: (1): Galaxy name. (2): Power-law photon index. (3): Energy of the exponential cut-off in~keV. (4): Reflection parameter. (5): Value of the {\it XMM-Newton}/{\it INTEGRAL} cross-calibration constant.  (6): Chi-squared and degrees of freedom.
\end{table}