\begin{table}%t4
\caption{\label{tab:properties}Synoptic table reporting the main known parameters for IGR~J16358-4724 and IGR~J16393-4643. }
\par
%\centerline
{
\begin{tabular}{l   cc}
\hline
\hline
\noalign{\smallskip}
Parameter & IGR~J16358-4724  & IGR~J16393-4643\\
\hline 
Spectral type &  &   \\
of the secondary & K-M III [1]& K-M III [1] \\
$V$-band magnitude & $>$$23.67$ [2] & 21.53 [2]\\
$A_{V}$ (mag)  &  12--13 [1] & 4--6 [1]  \\
Distance (kpc)  & 5--6; 12--13 [3] & $\sim$10 [4] \\
X-ray spectrum &  [5]  &  [4] \\
$L_{\rm X}$  (erg s$^{-1}$) & $3 \times 10^{32}$--$2 \times 20^{36}$ [5] & ${2\times 10^{34}}$ [4,1]\\
$L_{\rm X} / L_{\rm secondary}$ & --   & -- \\
$\dot{M}$ (g s$^{-1}$) & $1.6 \times 10^{12}$--$1.1 \times 10^{16}$ [1]  & ${1.1\times10^{14}}$ [1]\\
$P_{\rm spin}$ (s)  &   5850 [6] & $\sim$912 [4,7]\\
$\dot{P}_{\rm spin} / P_{\rm spin} $ (s$^{-1}$)   & 3.1 $\times 10^{-8}$ [5] & 1.0 $\times 10^{-11}$ ? [7,1]\\
$P_{{\rm orb}}$ (d) & -- &  50.2 ? [7,1]\\
\hline
\end{tabular}}
\tablefoot{The X-ray luminosity is given in the 2--10 keV band. The mass accretion rate $\dot{M}$ was estimated assuming typical parameters for a neutron star, i.e. $R_{\rm X} = 10$ km and $M_{\rm X} = 1.4$~$M_{\odot}$.}\vspace{-2mm}
\tablebib{
[1] this work; [2] Chaty et al. (2008); [3] Lutovinov et al. (2005); 
[4] Bodaghee at al. (2006); [5] Patel at al. (2007); [6] Patel et al. (2004); 
[7] Thompson et al. (2006).}\vspace{-3mm}
\end{table}