\begin{table}%t2
\caption{\label{xbtab}Detected HMXBs and candidates in the fields of the SMC observed by XMM-Newton.}
%\centerline
{
\begin{tabular}{lrllccrc}
\hline\hline
\multicolumn{1}{c}{1} & \multicolumn{1}{c}{2} & \multicolumn{1}{c}{3} & \multicolumn{1}{c}{4} &
\multicolumn{1}{c}{5} & \multicolumn{1}{c}{6} & \multicolumn{1}{c}{7} & \multicolumn{1}{c}{8} \\
\hline
\multicolumn{1}{c}{No.} & \multicolumn{1}{c}{Obs.\ ID} & \multicolumn{1}{c}{RA} &
\multicolumn{1}{c}{Dec} & \multicolumn{1}{c}{Pos.\ err.} & \multicolumn{1}{c}{Count rate} & \multicolumn{1}{c}{Det. $ML$} & 
\multicolumn{1}{c}{Flux} \\
\multicolumn{1}{c}{} & \multicolumn{1}{c}{} & \multicolumn{2}{c}{(J2000.0)} &
\multicolumn{1}{c}{[\arcsec]} & \multicolumn{1}{c}{[s$^{-1}$]} & \multicolumn{1}{c}{} & 
\multicolumn{1}{c}{[erg~cm$^{-2}$~s$^{-1}$]} \\
\hline\\[-3mm]
01 & 00842008~M1 & 00 51 56.05 & --73 41 51.4 & 2.1 & $6.33 \times 10^{-3} \pm 1.04 \times 10^{-3}$ & 84.2 &$\sim$$1 \times 10^{-13}$\\
[1.5mm]%\hline
02 & 00842008~PN & 00 54 33.4  & --73 41 04$^{\diamondsuit}$& -- & $<$$2.33 \times 10^{-03~\dagger}$ & 3.4 & $<$$1.5 \times 10^{-14}$\\
[1.5mm]
03 & 00842001~PN & 00 54 56.02 & --72 26 48.6 & 1.0 & $3.30 \times 10^{-2} \pm 3.44 \times 10^{-3}$ & 267.1 & $5.3 \times 10^{-14}$ \\
[1.5mm]
04 & 00842001~PN & 00 56 05.24 & --72 22 00.9 & 2.0 & $7.46 \times 10^{-3} \pm 1.32 \times 10^{-3}$ &  76.0 & $2.4 \times 10^{-14}$ \\
[1.5mm]
05 & 00842001~PN & 00 57 19.58 & --72 25 35.1 & 0.5 & $8.79 \times 10^{-2} \pm 4.16 \times 10^{-3}$ & 225.6 & $1.4 \times 10^{-13}$ \\
[1.5mm]
06 & 00842001~PN & 00 57 35.71 & --72 19 32.6 & 0.9 & $3.07 \times 10^{-2} \pm 2.46 \times 10^{-3}$ & 478.5 & $9.5 \times 10^{-14}$ \\[0.05mm]
%\noalign{\smallskip}
06a& 01100002~PN & 00 57 35.56 & --72 19 36.8 & 2.9 & $2.53 \times 10^{-2} \pm 6.94 \times 10^{-3}$ &  55.9 & $1.9 \times 10^{-14}$ \\
[1.5mm]
07 & 01100002~PN & 00 57 50.22 & --72 02 37.0 & 0.7 & $1.32 \times 10^{-1} \pm 8.75 \times 10^{-3}$ &1147.0 & $2.3 \times 10^{-13}$ \\
[1.5mm]
08 & 01100002~PN & 00 57 50.80 & --72 07 58.7 & 0.5 & $1.79 \times 10^{-1} \pm 8.11 \times 10^{-3}$ &2798.1 & $5.8 \times 10^{-13}$ \\
[1.5mm]            
09 & 00842001~PN & 00 58 11.68 & --72 30 50.4 & 1.7 & $5.37 \times 10^{-2} \pm 8.49 \times 10^{-3}$ & 120.2 & $\sim$$3 \times 10^{-13}$ \\
[1.5mm]            
10 & 01100002~M1 & 00 59 21.01 & --72 23 18.4 & 0.8 & $5.22 \times 10^{-2} \pm 3.22 \times 10^{-3}$ &1269.6 & $2.3 \times 10^{-13}$ \\[0.05mm]
%\noalign{\smallskip}
10a& 00842001~PN & 00 59 21.10 & --72 23 15.8 & 0.9 & $1.05 \times 10^{-1} \pm 7.23 \times 10^{-3}$ &828.9  & $1.2 \times 10^{-13}$ \\
[1.5mm]        
11 & 01100002~PN & 01 00 16.18 & --72 04 45.8 & 1.2 & $2.42 \times 10^{-2} \pm 2.86 \times 10^{-3}$ & 237.5 & $4.2 \times 10^{-14}$ \\
[1.5mm]         
12 & 01100002~PN & 01 00 30.23 & --72 20 35.1 & 3.2 & $9.81 \times 10^{-3} \pm 3.00 \times 10^{-3}$ &  25.8 &$\sim$$6 \times 10^{-14}$\\
[1.5mm]         
13 & 01357206~PN & 01 01 02.98 & --72 06 59.5 & 2.9 & $1.77 \times 10^{-2} \pm 4.16 \times 10^{-3}$ &  38.2 & $2.6 \times 10^{-14}$ \\[0.05mm]
%\noalign{\smallskip}
13a& 01100002~PN & 01 01 03.87 & --72 07 02.4 & 3.8 & $9.16 \times 10^{-3} \pm 2.68 \times 10^{-3}$ &  23.0 & $3.2 \times 10^{-14}$ \\
[1.5mm]
14 & 01100002~PN & 01 01 20.82 & --72 11 21.1 & 0.6 & $1.40 \times 10^{-1} \pm 7.47 \times 10^{-3}$ &1689.6 & $3.1 \times 10^{-13}$ \\[0.05mm]
%\noalign{\smallskip}
14a& 01357206~PN & 01 01 20.87 & --72 11 16.8 & 1.0 & $8.83 \times 10^{-2} \pm 8.74 \times 10^{-3}$ & 368.7 & $8.5 \times 10^{-14}$ \\
[1.5mm]      
15 & 01357206~PN & 01 01 37.56 & --72 04 18.7 & 1.0 & $5.01 \times 10^{-2} \pm 4.26 \times 10^{-3}$ & 436.3 & $5.7 \times 10^{-14}$ \\[0.05mm]
%\noalign{\smallskip}
15a& 01100002~PN & 01 01 37.77 & --72 04 22.1 & 1.2 & $3.55 \times 10^{-2} \pm 4.36 \times 10^{-3}$ & 222.7 & $4.6 \times 10^{-14}$ \\
[1.5mm]
16 & 01357206~PN & 01 03 14.11 & --72 09 14.2 & 0.5 & $1.34 \times 10^{-1} \pm 6.38 \times 10^{-3}$ &2049.8 & $3.5 \times 10^{-13}$ \\
[1.5mm]
17 & 01357206~PN & 01 03 37.57 & --72 01 33.2 & 0.2 & $5.09 \times 10^{-1} \pm 9.62 \times 10^{-3}$ &17172.3& $2.6 \times 10^{-12}$ \\
[1.5mm]
18 & 01357206~PN & 01 05 55.38 & --72 03 47.9 & 1.6 & $3.05 \times 10^{-2} \pm 3.79 \times 10^{-3}$ & 119.5 & $3.9 \times 10^{-14}$ \\
\hline
\end{tabular}}       
\medskip
Notes to Col.~2:
Observation ID and the instrument with which the detection with the highest 
likelihood was achieved. \\
Notes to Cols.~3--5:
Position of the XMM-Newton detections with 1~$\sigma$ statistical positional 
error, except for No.~02, for which the position of the optical 
counterpart$^{\diamondsuit}$
is given. \\
Notes to Col.~6:
Count rate for EPIC PN detection (except for entries Nos.~01 and~10 which are 
EPIC MOS1 detections, and $^{\dagger}$ 3~$\sigma$ upper limit for No.~02). \\
Notes to Col.~7:
Maximum likelihood ($ML$) of detection for the total band (0.3--10.0~keV). \\
Notes to Col.~8:
Flux (0.3--10.0~keV) calculated from the best fit model spectrum, setting
the Galactic foreground absorption to zero. See Sect.~\ref{timspec} 
for used models. In order to obtain the luminosity, multiply by 
$4.3 \times 10^{47}$~cm$^{2}$.
\end{table}