\begin{table}%t2
\caption{List of detected sources with 2--10~keV flux 
$F_{\rm X}\geq10^{-13}$~erg/s/cm$^2$.}\label{tb:source}
%\centerline
{
\begin{tabular}{lccccl}
\hline\hline
Source ID & $F_{\rm X}$[2--10~keV] &  $L_{\rm X}$[2--10~keV]$^{(1)}$ &Rmag$^{(2)}$& $F$$_{\rm x}$/$F$$_{\rm opt}$ &Comments       \\
        &   erg/s/cm$^2$& erg/s &   &     \\     
\hline
XMMUJ053856.7--640503 & $2.67\times10^{-11}$&$8.0\times10^{36}$& 16.7& 33 &HMXB LMC X-3   \\
XMMUJ054011.5--691953  & $2.45\times10^{-11}$&$7.4\times10^{36}$& & &Crab-like pulsar PSR B0540--69  \\
XMMUJ052844.9--652656  & $1.30\times10^{-11}$&&6.4$^{*}$& 0.0012  &foreground star ABDor\\
XMMUJ045818.0--751637    & $6.06\times10^{-12}$& &7.5$^{*}$&0.0016  &foreground star YYMen\\
XMMUJ053747.4--691020 & $5.39\times10^{-12}$&$1.6\times10^{36}$ &&&Crab-like pulsar PSRJ0537--6910\\
XMMUJ053113.1--660707 & $3.01\times10^{-12}$&$9.0\times10^{35}$ &14.0&0.31 &HMXB Be EXO053109--6609 \\
XMMUJ052402.1--701108 & $2.08\times10^{-12}$& && &AGN RX~J0524.0-7011 \\
XMMUJ043831.4--681203  & $8.88\times10^{-13}$&$2.7\times10^{35}$ && & \\
XMMUJ053844.2--690608     & $8.35\times10^{-13}$&$2.5\times10^{35}$ &&
& W--R stars (?) in R136 \\
XMMUJ053011.3--655123    & $6.59\times10^{-13}$&$2.0\times10^{35}$ &14.7&0.13 &HMXB Be (?) 272s pulsar$^{(3)}$ \\
XMMUJ050550.2--675018       & $5.80\times10^{-13}$&$1.7\times10^{35}$ &17.6 &1.5 & \\
XMMUJ053115.4--705350     & $5.25\times10^{-13}$&$1.6\times10^{35}$ &13.8 &0.043 & \\
XMMUJ053218.6--710746       & $4.28\times10^{-13}$&$1.3\times10^{35}$ &17.9 &1.6 & \\
XMMUJ053833.9--691157       & $3.65\times10^{-13}$&$1.1\times10^{35}$ &17.8&1.3\\
XMMUJ050026.6--750449    & $3.50\times10^{-13}$&$1.1\times10^{35}$ &18.2&1.7& \\
XMMUJ052847.3--653956     & $2.70\times10^{-13}$&$8.1\times10^{34}$ && &\\
XMMUJ045208.7--705652  & $2.33\times10^{-13}$&$7.0\times10^{34}$&& &  \\
XMMUJ045637.9--751015	  & $2.06\times10^{-13}$&$6.2\times10^{34}$ &18.3&1.1&\\
XMMUJ054134.7--682550     & $2.04\times10^{-13}$&$6.1\times10^{34}$ & 14.0&$0.020$  & \\
XMMUJ052312.9--701531       & $1.94\times10^{-13}$&$5.8\times10^{34}$ && & \\
XMMUJ050526.6--674313  & $1.91\times10^{-13}$& &10.8$^{(4)}$& 0.0011 &foreground star GSC 9161.1103 \\
XMMUJ053528.5--691614  &  $1.89\times10^{-13}$&$5.7\times10^{34}$ &&&SNR SN1987A  \\
XMMUJ054151.2--682609  & $1.75\times10^{-13}$&$5.3\times10^{34}$ && & \\
XMMUJ045244.2--704821   & $1.71\times10^{-13}$&$5.1\times10^{34}$ && &\\
XMMUJ050833.2--685427  & $1.70\times10^{-13}$&$5.1\times10^{34}$  &&&\\
XMMUJ052403.1--673606    & $1.67\times10^{-13}$&$5.0\times10^{34}$ &18.3&0.91& \\
XMMUJ053041.1--660535   & $1.66\times10^{-13}$&$5.0\times10^{34}$ &18.2&0.83 & \\
XMMUJ053810.0--685658   & $1.58\times10^{-13}$&$4.7\times10^{34}$ && & \\
XMMUJ052947.7--655643  &  $1.51\times10^{-13}$&$4.5\times10^{34}$  &14.8&0.033 &HMXB Be/X transient RX~J0529.8--6556  \\
XMMUJ045219.8--684151  &$1.49\times10^{-13}$&$4.5\times10^{34}$  &&& \\
XMMUJ053734.9--641012   &$1.46\times10^{-13}$&$4.4\times10^{34}$ && &  \\
XMMUJ053909.8--640310     & $1.33\times10^{-13}$&$4.0\times10^{34}$ &&&   \\
XMMUJ051832.5--693521     &$1.32\times10^{-13}$&$4.0\times10^{34}$  &&&   \\
XMMUJ051747.0--685458     &$1.32\times10^{-13}$&$4.0\times10^{34}$  &&&  \\
XMMUJ051003.9--671858 &  $1.31\times10^{-13}$& $3.9\times10^{34}$ &&&  \\
XMMUJ054237.8--683205 &$1.29\times10^{-13}$&$3.9\times10^{34}$&& &  \\
XMMUJ050736.6--684752   &$1.23\times10^{-13}$&$3.7\times10^{34}$  && &  \\
XMMUJ053257.7--705113    & $1.23\times10^{-13}$&$3.7\times10^{34}$ &19.0$^{*}$&1.3 &  \\
XMMUJ052422.4--672020  &  $1.22\times10^{-13}$&$3.7\times10^{34}$ &&&   \\
XMMUJ052353.7--672824   & $1.21\times10^{-13}$&$3.6\times10^{34}$  &&&  \\
XMMUJ054212.6--692442   & $1.19\times10^{-13}$&$3.6\times10^{34}$ & 19.3$^{*}$&1.6&  \\
XMMUJ054543.2--682528    &   $1.17\times10^{-13}$&$3.5\times10^{34}$ &&& \\
XMMUJ050048.6--750653   &    $1.15\times10^{-13}$&$3.5\times10^{34}$ &&& \\
XMMUJ053632.6--655644     &  $  1.14\times10^{-13}$&$3.4\times10^{34}$  &&& \\
XMMUJ045137.0--710210     &  $ 1.14\times10^{-13}$&$3.4\times10^{34}$  &&& \\
XMMUJ053841.7--690514      & $   1.03\times10^{-13}$&$3.1\times10^{34}$
&&& W--R stars (?) in R140\\
XMMUJ052558.0--701107  & $1.03\times10^{-13}$&&11.0 & 0.00068 & foreground star, K2IV-Vp, RS CVn\\
XMMUJ052952.9--705850     & $1.02\times10^{-13}$&$3.1\times10^{34}$ &&& \\
\hline
\end{tabular}}
\medskip
$^{(1)}$ Calculated assuming distance to LMC 50 kpc.\\
$^{(2)}$ Apparent magnitude in the $R$-band of the optical counterpart from 
GSC2.2.1 catalogue \citep{gsc},  located within  3.6~arcsec from
the \mbox{X-ray} source.\\   
$^{(3)}$ \citet{hp03}.\\
$^{(4)}$ Apparent $R$-band magnitude from the USNO-B catalogue \citep{usno-b}.\\ 
\end{table}