\begin{table}%t1
\caption{\label{tab-sources}Sample of selected sources detected in the EPIC observations.}
%%%\centerline
\par
{
\begin{tabular}{lcrrrrcrl}
\hline\hline\noalign{\smallskip}
\multicolumn{1}{l}{Source} &
\multicolumn{1}{c}{$ML$} &
\multicolumn{1}{c}{PSPC} &
\multicolumn{1}{c}{HRI} &
\multicolumn{1}{c}{$R$} &
\multicolumn{1}{c}{$B$} &
\multicolumn{1}{c}{USNO} &
\multicolumn{1}{c}{delta} &
\multicolumn{1}{c}{Comment} \\
\multicolumn{1}{l}{XMMU~J05...} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{[mag]} &
\multicolumn{1}{c}{[mag]} &
\multicolumn{1}{c}{U0225\_02...} &
\multicolumn{1}{c}{[\arcsec]} &
\multicolumn{1}{c}{} \\
\noalign{\smallskip}\hline\noalign{\smallskip}
 2924.3-655724 & 1.60\expo{3} & 210 & 190 &             &             &        &     & foreground star? GSC8891.0505 13.68 mag\\
 2940.5-655318 & 1.38\expo{3} & 189 & 198 & $\ga$17.9 & $\ga$19.0 &        &     & AGN?\\
 2947.4-655639 & 2.26\expo{3} & 204 & 202 &        15.0 &        14.3 & 044134 & 4.3 & HMXB-Be RX J0529.8-6556 69.5 s pulsar\\
 3011.2-655122 & 1.61\expo{4} & 183 & 205 &        14.7 &        14.2 & 054120 & 1.5 & HMXB-Be? 272 s pulsar\\
 3034.9-655653 & 1.27\expo{2} & 205 &     &             &             &        &     & SNR?\\
\noalign{\smallskip}
 3041.0-660532 & 3.07\expo{3} &     & 210 & $\ga$17.3 & $\ga$18.1 &        &     & AGN?\\
 3049.9-655522 & 1.12\expo{3} & 197 &     & $\ga$17.8 & $\ga$18.5 &        &     & AGN?\\
 3056.2-654809 & 1.49\expo{2} &     &     & $\ga$17.9 & $\ga$19.4 &        &     & SSS?\\
 3102.5-660649 & 3.52\expo{3} &     & 215 &             &             &        &     & AGN?\\
 3113.3-660705 & 4.04\expo{4} & 252 & 218 &        13.9 &        14.7 & 079445 & 2.5 & HMXB-Be \exo\ 13.7 s pulsar\\
\noalign{\smallskip}
 3137.2-660131 & 4.20\expo{2} & 225 &     &        14.0 &        16.0 & 088686 & 2.2 & foreground star?\\
 3150.9-655616 & 3.76\expo{3} & 202 &     &             &             &        &     & AGN?\\
 3153.8-660217 & 1.71\expo{3} & 229 & 222 & $\ga$17.1 & $\ga$18.0 &        &     & AGN?\\
 3153.9-654959 & 1.56\expo{3} &     &     &             &             &        &     & AGN?\\
 3157.1-660233 & 1.25\expo{3} &     &     & $\ga$17.9 & $\ga$18.7 &        &     & AGN?\\
\noalign{\smallskip}
 3226.2-655352 & 3.19\expo{2} & 190 &     &             &             &        &     & SNR?\\
 3230.2-655735 & 1.43\expo{3} & 211 &     &             &             &        &     & AGN?\\
 3232.4-655139 & 7.84\expo{2} & 184 & 233 &        13.9 &        12.4 & 109716 & 2.0 & HMXB-OB RX J0532.5-6551\\
 3236.7-655551 & 2.15\expo{3} &     & 236 & $\ga$17.3 & $\ga$18.1 &        &     & AGN?\\
 3243.9-660258 & 9.85\expo{1} &     &     &        11.7 &        14.4 & 113921 & 4.0 & foreground star?\\
\hline
\end{tabular}}
\smallskip
Notes: Maximum Likelihood ({\it ML}) corresponding to probability $P = 1$ -- exp(--$ML$) of existence; PSPC
and HRI~catalogue entries from \citet{1999AetAS..139..277H} and \citet{2000AetAS..143..391S}; $R$ and~$B$
from brightest USNO~A2.0 object within~5\arcsec of X-ray position which provides a lower limit for the optical
counterparts to the AGN~candidates; delta denotes the angular distance between
optical (USNO~A2.0) and X-ray position for the cases with optical identification (HMXBs and foreground stars).
\end{table}