\begin{table}%t5
\caption{\label{tab:spectral}Results of the X-ray spectral analysis. Errors and upper limits are all given at 
the 90\% level.}
%%\centering

\par
\begin{tabular}{lcllllll}
\hline\hline\noalign{\smallskip}
Name & Net number & Galactic \nh\tablefootmark{\dagger}  & \nh\ & $\Gamma$& 2--10 keV flux\tablefootmark{\ddagger} & \multicolumn{2}{c}{20--40 keV flux}\\
(IGR) &  of counts & $\times10^{22}$~cm$^{-2}$ & $\times10^{22}$~cm$^{-2}$  &   & \ergcms & \multicolumn{2}{c}{\ergcms}\\
&&&&   && Extrapolated  & IBIS source \\
\hline
J02086$-$1742      & 931 & 0.01 & $<$0.017 & $1.55_{\rm -0.08}^{+0.1}$ & $6.4\times10^{-12}$ & $6.3\times10^{-12}$ & $6.8\times10^{-12}$\\
J02524$-$0829\tablefootmark{\star}      & 617 & 0.04 & $12\pm3$ & $2.4\pm0.6$ & $1.2\times10^{-11}$ & $4.7\times10^{-12}$ & 3.1$\times10^{-11}$\\ 
J03184$-$0014      & 22   & 0.05 & $<$1.1 & $1.4_{\rm -0.9}^{+1.5}$ & $1.5\times10^{-13}$ &$2.0\times10^{-13}$  & $2.9\times10^{-11}$ \\
J11457$-$1827\tablefootmark{\P}      & 4020 & 0.03 & $1.298_{\rm -0.003}^{+0.01}$ & $1.91_{\rm -0.04}^{+0.08}$ & $1.4\times10^{-11}$ &$1.1\times10^{-11}$ & $3.3\times10^{-11}$ \\
J12060+3818\tablefootmark{\P}       & 48    & 0.016 & $<$0.13 & $2.4_{\rm -0.9}^{+1.2}$ & $1.5\times10^{-13}$ & $5.6\times10^{-14}$ & $3.1\times10^{-11}$\\
J12070+2535\tablefootmark{\P}         & 74    & 0.016 & $0.3\pm0.2$ & $1.9_{\rm -0.5}^{+0.6}$ & $1.4\times10^{-12}$ &  $1.1\times10^{-12}$&  $1.4\times10^{-11}$\\
J13042$-$1020\tablefootmark{a}      & 268 & 0.033 & $29_{\rm -6}^{+8}$& $2\pm0.2$& $4.0\times10^{-12}$& $1.7\times10^{-12}$ & $7.5\times10^{-12}$ \\
J13412+3022\tablefootmark{a}         & 90  & 0.014 & $30_{\rm -8}^{+11}$ & $1.4_{\rm -0.6}^{+0.2}$ & $8.0\times10^{-12}$& $9.5\times10^{-12}$& $9.1\times10^{-12}$\\
J14488$-$5942\#1  & 344 & 1.8    & $13_{\rm -4}^{+6}$ & $2.8_{\rm -0.9}^{+1.1}$ & $7.9\times10^{-12}$ & $7.1\times10^{-13}$ & $3.8\times10^{-12}$\\
\hspace*{0.55cm} $''$ \#2 & 22 &$''$  & $<$2.4 & $2.2_{\rm -1.6}^{+2.2}$ & $4.7\times10^{-14}$ &$7.9\times10^{-15}$ & $''$  \\
J23130+8608         & 20  & 0.052 &   -- & $1.4_{\rm -0.9}^{+0.7}$ & $7.0\times10^{-14}$ & $9.4\times10^{-14}$ & $1.4\times10^{-11}$\\
\hline
\end{tabular}
\tablefoot{
\tablefoottext{\dagger}{Value obtained from the LAB survey \citep{kalberla05}.} 
\tablefoottext{\ddagger}{Flux corrected for the absorption.}
\tablefoottext{\star}{Hard fluxes are estimated over the 17--60 keV ranges.}
\tablefoottext{\P}{Hard fluxes are estimated over the 20--60 keV ranges.}
\tablefoottext{a}{Spectra fitted with a partial covering absorber and a power-law.}} 
\end{table}