\begin{table}%T5
\par
\caption{\label{ESO383_res}Results obtained from the X-ray spectral analysis of ESO~383-18.}
\small%\centering
\par
\begin{tabular}{lllllllll}
\hline\hline\noalign{\smallskip}
Instruments & Energy&  $\chi ^2$ (d.o.f.)& $\Gamma$& $N_{\rm H}$ &$N_{\rm H}^1$&  $f^1$ & $N_{\rm H}^2$ &  $f^2$  \\
& {[keV] }& &  &{[$10^{20}\rm ~cm^{-2}$] }& {[$10^{22}\rm ~cm^{-2}$] }& &{[$10^{22}\rm ~cm^{-2}$] } &  \\
\hline\noalign{\smallskip}
EPIC$^a$& 0.3--10& 1087 (432)& $1.2\pm0.1$ & $15\pm 1$ &  -- & -- &  -- &  -- \\
EPIC$^b$& 0.3--10&533 (431)& $1.47^{\rm +0.03}_{-0.05}$ & $0.042$ &  $19.5^{\rm +0.7}_{-0.7}$ & $0.989^{\rm +0.002}_{-0.003}$ & -- &  --  \\
EPIC$^c$& 0.3--10& 461 (423)& $ 1.8^{\rm +0.1}_{-0.1}$ & $ 0.042 $ &  $10^{\rm +1}_{-2}$ & $0.97^{\rm +0.02}_{-0.04}$ & $ 20^{\rm +2}_{-3}$ & $ 0.86^{\rm +0.05}_{-0.05}$ \\
(EPIC + ISGRI)$^c$& 0.3--110&  472 (426)& $ 1.7^{\rm +0.2}_{-0.2}$ & $ 0.042 $ &  $11^{\rm +17}_{-5}$ & $0.95^{\rm +0.03}_{-0.15}$ & $ 15^{\rm +4}_{-7}$ & $ 0.85^{\rm +0.06}_{-0.07}$ \\\noalign{\smallskip}
\hline
\end{tabular}
\tablefoot{The data were modeled with an absorbed power law model ($a$), a power law absorbed by Galactic cold matter plus a layer of partially absorbing neutral material ($b$), and a power law plus two Gaussian lines (representing the iron K$\alpha$ and the OVIII Ly$\alpha$ emission lines)s absorbed by Galactic cold matter and by two layers of partially absorbing neutral material ($c$). EPIC includes PN, MOS1 and MOS2 data.}
\end{table}