\begin{table}%t3
\caption{List of HMXB candidates}
\label{tb:hmxbcand}
%\centerline
{
\begin{tabular}{lcccccccl}
\hline\hline
\#  & RA  & Dec  &  $F_{\rm X}$ (1) & $L_{\rm X}$ (1) &$m_R$&$V-R$ & $F_{\rm x}$/$F_{\rm opt}$ &Comments       \\
 & & &    erg/s/cm$^{-2}$& erg s$^{-1}$ &   &     \\     
\hline
\multicolumn{8}{c}{\em Likely HMXB candidates$^{(3)}$}\\
\hline
%142%84.7361 & -64.0843
%05 38 56.7&-64 05 03.5
1 &  05 38 56.7&$-$64 05 03   &$2.67\times10^{-11}$&$8.0\times10^{36}$& 16.7&$-$0.2$^{5}$& 33 &LMC X-3  \\
%132%82.8046  & -66.1187
%05 31 13.1& -66 07 07.3
2 &  05 31 13.1& $-$66 07 07   &$3.01\times10^{-12}$&$9.0\times10^{35}$ & 14.0&0.23 &0.31&Be/X EXO053109--6609\\
%130%82.5473   &-65.8565
%05 30 11.4 & -65 51 23.4
3 &  05 30 11.4 & $-$65 51 23.4   &$6.59\times10^{-13}$&$2.0\times10^{35}$& 14.7&0.18 &0.13&Be/X ? 272s pulsar$^{(2)}$ \\
%152%82.8143 &-70.8972
%05 31 15.4 & -70 53 49.9
4 &  05 31 15.4 & $-$70 53 50  &$5.25\times10^{-13}$&$1.6\times10^{35}$& 13.6&0.1 &0.038 & \\
%121%85.3944 & -68.4306
%05 41 34.7& -68 25 50.2
5 &  05 41 34.7& $-$68 25 50  &$2.04\times10^{-13}$&$6.1\times10^{34}$& 14.0& $-$0.03 & 0.02&\\
% 127%82.4488  -65.9453
%05 29 47.7& -65 56 43.1
6 &  05 29 47.7& $-$65 56 43   &$1.51\times10^{-13}$&$4.5\times10^{34}$&14.6& $-$0.02 &0.027&Be/X transient RX~J0529.8--6556\\
% 129%83.1355 & -65.8613
%05 32 32.5& -65 51 40.7
7 &  05 32 32.5& $-$65 51 41  &$5.93\times10^{-14}$&$1.8\times10^{34}$&13.4&$-$0.36 &0.0036&OB RX~J0532.5--6551  \\
%147 %80.1224 & -69.5322
%05 20 29.4& -69 31 55.9
8 &  05 20 29.4& $-$69 31 56   &$4.05\times10^{-14}$&$1.2\times10^{34}$&14.1&0.03&0.0046 &RX~J0520.5--6932\\
%128%82.8260 & -66.1249
%05 31 18.2& -66 07 29.6
%17
9 & 05 31 18.2& $-$66 07 30  &  $3.42\times10^{-14}$&$1.0 \times10^{34}$&16.0 &$-$1.3$^{6}$&0.023 &\\
\hline
\multicolumn{8}{c}{\em Sources of uncertain nature$^{(4)}$}\\
\hline
%156%80.7501 & -70.3089
%05 23 00.0& -70 18 32.0
%24
10 & 05 23 00.0& $-$70 18 32   &
$7.93\times10^{-14}$&$2.4\times10^{34}$&17.3 &0.45&0.17 & M\\
%143%84.3209 & -64.2048
%05 37 17.0& -64 12 17.3 
%19
11 & 05 37 17.0& $-$64 12 17  &
$6.19\times10^{-14}$&$1.9\times10^{34}$&17.2 &&0.063& GSC, N\\ 
%140%85.3476 & -69.6093
%05 41 23.4& -69 36 33.5
%18
12 & 05 41 23.4& $-$69 36 34  &
$5.84\times10^{-14}$&$1.8\times10^{34}$&17.1 &&0.11 & C\\ 
%113%73.2992 & -68.6631
%04 53 11.8&-68 39 47.2
%12
13 & 04 53 11.8&$-$68 39 47    &
$5.71\times10^{-14}$&$1.7\times10^{34}$&16.7&0.17&0.071& C\\
%148%82.5097 & -71.0129
%05 30 02.3& -71 00 46.4
%21
14 & 05 30 02.3& $-$71 00 46   &
$5.3\times10^{-14}$&$1.6\times10^{34}$&14.9 &&0.013& USNO-B\\
%119%86.1429 & -68.4706
%05 44 34.3& -68 28 14.1
%16
15 & 05 44 34.3& $-$68 28 14  &
$4.99\times10^{-14}$&$1.5\times10^{34}$&17.4 &&0.12& USNO-B\\
%102%80.0565 & -69.1617
%05 20 13.6& -69 09 42
%9 
16 & 05 20 13.6& $-$69 09 42   &
$4.72\times10^{-14}$&$1.4\times10^{34}$&16.0&&0.031& M\\
%107%79.5153 &-69.0206
%05 18 03.7&-69 01 14.2
%11
17 & 05 18 03.7&$-$69 01 14    &
$3.51\times10^{-14}$&$1.1\times10^{34}$&17.1&&0.063& USNO-B\\
%150%83.4456 & -70.9876
%05 33 46.9& -70 59 15.4
%22
18 & 05 33 46.9& $-$70 59 15.4   &
$3.46\times10^{-14}$&$1.0\times10^{34}$&14.4 &0.93&0.0052 & C\\
%144%85.1816 & -64.0292
%05 40 43.6& -64 01 45.1
%20
19 & 05 40 43.6& $-$64 01 45  &
$3.36\times10^{-14}$&$1.0\times10^{34}$&17.1 &&0.062& C\\ 
%168%81.0638 & -70.0765
%05 24 15.3& -70 04 35.4
%28
20 & 05 24 15.3& $-$70 04 35   &
$2.80\times10^{-14}$&$8.4\times10^{33}$&17.0 &&0.024 & USNO-B\\
%114%81.8874 & -65.5798
%05 27 33.0& -65 34 47.3
%13
21 & 05 27 33.0& $-$65 34 47  &
$2.77\times10^{-14}$&$8.3\times10^{33}$&16.2&&0.022& M\\
%166%81.7583 & -70.0878
%05 27 02.0& -70 05 16.1
%27
22 & 05 27 02.0& $-$70 05 16   &
$2.75\times10^{-14}$&$8.3\times10^{33}$&17.4 &&0.063 & USNO-B\\
%161%80.8135 & -70.2438
%05 23 15.2& -70 14 37.
%25
23 & 05 23 15.2& $-$70 14 38   &
$2.35\times10^{-14}$&$7.1\times10^{33}$&16.1 &&0.018 & USNO-B\\
%155%81.7608 & -67.4577
%05 27 02.6& -67 27 27.7
%23
24 & 05 27 02.6& $-$67 27 28   &
$2.11\times10^{-14}$&$6.3\times10^{33}$&14.4 &&0.0032 & USNO-B, N\\
%104%80.2818 & -69.0503
%05 21 07.6& -69 03 01
%10
25 & 05 21 07.6& $-$69 03 01   &
$1.66\times10^{-14}$&$5.0\times10^{33}$&16.4&&0.016& USNO-B\\
%117%81.8811 & -65.3427
%05 27 31.5& -65 20 33.7
%15
26 & 05 27 31.5& $-$65 20 34  &
$1.58\times10^{-14}$&$4.7\times10^{33}$&17.3&&0.034& USNO-B\\
%116%81.7314 & -65.3470
%05 26 55.5& -65 20 49.2
%14
27 & 05 26 55.5& $-$65 20 49  &
$1.41\times10^{-14}$&$4.2\times10^{33}$&17.5&&0.037& C\\ 
%165%81.2649 & -70.1379
%05 25 03.6& -70 08 16.4
%26
28 & 05 25 03.6& $-$70 08 16   &
$1.37\times10^{-14}$&$4.1\times10^{34}$&17.4 &&0.033 & USNO-B\\
\hline
\multicolumn{8}{c}{\em 30 Doradus region ($r\le4\arcmin$)}\\
\hline
%xxx%
29 & 05 38 44.2 &69 06 08  & $8.35\times10^{-13}$&$2.5\times10^{35}$&  & & &
Wolf-Rayet star in R136\\
%xxx%
30 & 05 38 41.7 &69 05 14 & $1.03\times10^{-13}$&$3.1\times10^{34}$&  & &&
Wolf-Rayet star in R140\\
\hline
\end{tabular}}
\medskip
(1) -- 2--10~keV band; 
(2) -- \citep{hp03}; 
(3) -- optical counterpart is consistent with being an HMXB;
(4) -- the optical counterpart exists, but the information is
insufficient for its reliable classification;
(5) -- $B{-}V$ color from \citet{hmxbcat};  
(6) -- $B{-}V$ color. \\
Comments: 
USNO-B -- counterpart in USNO-B only;
GSC -- counterpart in GSC only;
M -- multiple non-overlapping optical and/or infrared counterparts;
C -- ambiguous color indexes;
N -- non-HMXB nature is likely.
%\vspace*{3mm}
\end{table}