\begin{table}%t2
\caption{X-ray detected sources.\label{table2}}
%\centerline
 {\begin{tabular}{c c c c c c l l l c r r c r r c l }
\hline \hline 
\noalign{\smallskip}
Name & $\alpha_{\rm MIR}$ & $\delta_{\rm MIR}$ &$\alpha_{\rm X}$ & $\delta_{\rm X}$ &$\Delta$ & $\Gamma$ & {\it KT} & $N_{\rm H}$ & $\chi^2/\rm d.o.f.$ & $F_{0.5-10}$ & $F_{2-10}$ & $z$ &
$L_{0.5-10}$ & $L_{2-10}$ & $Cl_{\rm O}$ & $Cl_{\rm X}$ \\
 (1) & (2) & (3) & (4) & (5) & (6) & (7) & (8) & (9) & (10) & (11) & (12)  & (13) & (14) & (15) & (16) & (17)\\
\hline
\noalign{\smallskip}
C15\_J003234-431940&  8.143084&--43.327194& 8.14298&--43.32731&0.5&$1.80$              & ...               &$0.00_{\rm0.00}^{0.43} $& 6.8/10  & 2.28& 1.44&1.637&44.53&44.32& 1 & AGN1\\ 
C15\_J003315-432829&  8.315042&--43.475304& 8.31612&--43.47545&2.9&$2.37_{\rm 2.00}^{4.22}$& ...               &$8.0_{\rm 7.5}^{20.2}   $& 10.6/14& 1.81& 1.69&$>$0.5&$>$43.78&$>$43.40&...& AGN \\
C15\_J003317-431706&  8.321417&--43.285069& 8.31999&--43.28590&4.8&$1.80$              & ...               &$4.32_{\rm 1.21}^{1.66} $& 2.0/4  & 2.49& 2.28&0.689&43.68&43.63& 5 & AGN2 \\
C15\_J003318-431659&  8.326542&--43.284195& 8.32648&--43.28473&1.9&$1.80$              & ...               &$3.39_{\rm 0.98}^{1.25} $&27.3/27 & 2.38& 2.24&0.199&42.68&42.47& 5 & AGN2 \\
C15\_J003330-431553&  8.376667&--43.265110& 8.37693&--43.26542&1.3&$1.80$              & ...               &$~7.2_{\rm ~5.1}^{12.8} $&12.3/22 &0.43&0.34&2.170&44.21&43.94& 1 &  AGN1 \\
C15\_J003346-431942&  8.442875&--43.328835& 8.44301&--43.32917&1.3&$1.49_{\rm 0.10}^{0.16}$& ...               &$0.00_{\rm 0.00}^{0.10} $&60.9/61 & 5.44& 3.97&0.403&43.43&43.29& 3 & AGN2 \\
C15\_J003407-433559&  8.530666&--43.599583& 8.53035&--43.59983&1.2&$2.02_{\rm 0.60}^{1.07}$& ...               &$1.45_{\rm 0.97}^{1.68} $&26.5/31 & 1.89& 1.54&0.294&42.94&42.66& 5 & AGN2 \\
C15\_J003416-430941&  8.566916&--43.161446& 8.56900&--43.16218&6.1&$1.80$              &...                &$0.02_{\rm 0.02}^{1.03} $& 3.0/4  & 0.32& 0.05&0.313&42.20&42.00& 3 & AGN2 \\
C15\_J003432-433922&  8.635791&--43.656029& 8.63476&--43.65776&6.8&$1.80$             &$0.60_{\rm 0.35}^{1.11}$&$0.00_{\rm 0.00}^{0.12} $& 8.1/8  & 2.01& 1.07&0.020&40.28&39.99& 6 & STB \\
C15\_J003515-433356&  8.815042&--43.566029& 8.81537&--43.56558&1.8&$2.68_{\rm 0.00}^{0.04}$& ...               &$0.00_{\rm 0.00}^{0.00} $&285/160 &86.24&27.62&0.143&43.75&43.22& 1 & AGN1 \\
C15\_J003517-431121&  8.821792&--43.189335& 8.82196&--43.18954&0.9&$1.90_{\rm 0.10}^{0.22}$& ...               &$0.00_{\rm 0.00}^{0.04} $&52.7/56 & 6.15& 3.66&0.175&42.73&42.49& 6 & AGN2 \\
C15\_J003519-433711&  8.830126&-43.619667& 8.82976&--43.61887&3.0&$1.80$              & ...               &$2.04_{\rm 0.79}^{1.11} $&13.7/11 & 2.52& 2.22&0.286&42.98&42.78& 5 & AGN2 \\
C15\_J003640-433925&  9.168375&--43.657333& 9.16840&--43.65727&0.2&$1.80$              & ...               &$10.8_{\rm ~4.7}^{13.5} $&28.1/26 & 1.47& 1.34&1.181&44.20&44.01& 1 & AGN1 \\
\hline
\end{tabular}}
\par
\smallskip
{Notes.  The columns are as follows: (1) ELAIS ID
  name; (2, 3) Right Ascension and Declination at 15 $\mu$m (deg); (4, 5) Right Ascension and Declination in the 0.5--10~keV band;} 
{(6) distance of the MIR and X-ray sources (arcsec); (7) photon spectral index; (8) temperature of the MEKAL model (keV); (9) $N_{\rm H}$ column densities
in 10$^{22}$ cm$^{-2}$ units; } 
{ (10) $\chi^2$ and degrees of freedom of the XSPEC fit; (11, 12 ) 0.5--10 keV and 2--10 keV band fluxes in 10$^{-14}$ erg/s/cm$^2$ units;
(13) redshift; } 
{ (14, 15) log of the 0.5--10 keV band and 2--10 keV band luminosity in erg/s units; (16)
optical spectroscopic class as in La Franca
et~al. (2004) (1~=~AGN1, 2~=~AGN2, 3~=~e(a) gal,} 
{  4~=~e(b) gal, 5~=~e(c) gal, 6~=~k(e) gal, 7~=~k gal); (17) optical plus X-ray final classification.} 
\par
\end{table}