\begin{table}%t1
\caption{\label{tab:X-ray}X-ray properties of X-ray, radio and infrared sources in the region around HW~2/3.}
%\centerline
 {\small 
\begin{tabular}{c c c c c r c c c c c r r r}
\hline \hline\noalign{\smallskip}
Source & Radio & Infrared & RA & Dec & Counts$^a$ & Median & Temperature & Absorption & Luminosity & Radio & Spectral & Infrared \\ 
ID  & ID & ID & & &  & energy$^b$ & $kT$~(keV) & $10^{22}$~cm$^{-2}$ & $\log L_{\rm X}$~(erg~s$^{-1}$) & flux (mJy) & index & mag$^c$\\ 
\hline
X1 & & IRS 6b & 22:56:22.2 & +62:02:00.5 & 137 & 2.3 & 2.0--3.0 & 1.4--2.2 & 30.7--30.9 & \multicolumn{2}{c}{--} & 8.4 \\
X2 & & IRS 6d & 22:56:20.9 & +62:02:04.0 & 44 & 4.2 & 2.0$^e$ &  10--18 & 30.9--31.1 & \multicolumn{2}{c}{--} & 11.1\\
& & & & &&& 1.0$^e$   & 20 -- 32 & 32.0--32.3 \\
X3 & & ?$^d$ & 22:56:17.4 & +62:01:58.6 & 36 & 4.3 & 2.0$^e$ &10--18 & 30.9--31.1 & \multicolumn{2}{c}{--}\\
& & &   &  &    &     & 1.0$^e$ & 17--26 & 31.8--32.1 \\
X4 & & GPFW~2 & 22:56:20.2 & +62:01:41.4 & 64 & 3.9 & 0.9--1.7 & 11--32 & 31.2--32.3 & \multicolumn{2}{c}{--} & 15.6\\
X5 & 9  & & 22:56:18.6 & +62:01:47.8 & 60 & 4.1 & 0.7--1.3 & 20--38 & 31.8--33.4 & 3.0 & --0.2\\
X6 & &  & 22:56:18.1 & +62:01:43.2 & 50 & 5.5 & 2.0$^e$ & 32--50 & 31.5--31.8 & \multicolumn{2}{c}{--} \\
& & &  & & &  & 1.0$^e$ & 61--83 & 33.1--33.4 \\
X7 & 3c &  & 22:56:18.0 & +62:01:46.0 & 60 & 6.4 & 2.0$^e$ & 62--106 & 32.1--32.5 & 3.7 & 0.4\\
& & & & && & (1.0$^e$ & 127--175 & 34.0--34.5)$^f$ \\
& 1a &  & 22:56:16.2 & +62:01:37.8 &  2 & \multicolumn{3}{c}{--} & $<$29.8 (30.5) & 2.2 & --0.6 \\
& 1b &  & 22:56:16.6 & +62:01:42.6 &  2 & \multicolumn{3}{c}{--} & $<$29.8 (30.5) & 2.9 & --0.3 \\
&  2 &  & 22:56:19.0 & +62:01:49.4 &  $<$4 & \multicolumn{3}{c}{--} & $<$30.0 (30.7) & 7.5 & 0.7 \\
& 3a & GPFW~1a? & 22:56:17.1 & +62:01:43.9 &  1 &  \multicolumn{3}{c}{--} &$<$29.6 (30.3) & 0.2 & -- & 14.7\\
& 3b &  & 22:56:17.7 & +62:01:45.0 &  6 &  4.6 & \multicolumn{2}{c}{\hspace{-31pt}--} & 29.9 (30.6)  & 5.0 & 0.0 \\
& 3d &  & 22:56:18.2 & +62:01:46.0 &  3 &  \multicolumn{3}{c}{--} &$<$29.9 (30.6) & 7.7 & 0.3 \\
& 4  & GPFW~3 & 22:56:18.5 & +62:01:56.0 &  1 &  \multicolumn{3}{c}{--} &$<$29.6 (30.3) & 4.4 & --0.2 & 12.6 & \\
& 5  &  & 22:56:19.7 & +62:01:59.5 &  1 &  \multicolumn{3}{c}{--} &$<$29.6 (30.3) & 1.3 & --0.5 \\
& 6  &  & 22:56:20.2 & +62:02:03.0 &  0 &  \multicolumn{3}{c}{--} &$<$29.2 (29.9) & 3.8 & --0.3 \\
& 7a &  & 22:56:20.2 & +62:01:39.9 &  2 &  \multicolumn{3}{c}{--} &$<$29.8 (30.5) & 9.6 & --0.1 \\
& 7b &  & 22:56:20.8 & +62:01:39.6 &  1 &  \multicolumn{3}{c}{--} &$<$29.6 (30.3) & 2.8 & --0.4 \\
& 7c &  & 22:56:21.4 & +62:01:37.4 &  0 &  \multicolumn{3}{c}{--} &$<$29.2 (29.9) & 3.8 & --0.4 \\
& 7d$^g$ &  & 22:56:21.9 & +62:01:36.5 &  1 &  \multicolumn{3}{c}{--} &$<$29.7 (30.4) & 2.4 & -- \\
& 8  &  & 22:56:17.7 & +62:01:47.0 &  9 & 6.2 &  \multicolumn{2}{c}{\hspace{-31pt}--} &30.1 (30.8) & $<$0.12 & -- \\
&  & IRS 6c & 22:56:17.5 & +62:01:51.1 & 1 & \multicolumn{3}{c}{--} &$<$29.6 (30.3) & \multicolumn{2}{c}{--} & 8.5$^h$\\
\hline
\end{tabular}}
\medskip
$^a$ Including a background of 1.3~cts; $^b$~in keV; $^c$~$K$-band; $^d$  visible in the \citet{Goetz_1998} IR-images; $^e$ fixed; $^f$~this value is unlikely high for a stellar source, see Sect.~\ref{sect:X7}; $^g$~data from \citet{Hughes_1984}; $^h$ $L$-band.
\end{table}