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\begin{table*}
\caption[]{Variable sources in the LMC region I.}
\begin{flushleft}\begin{tabular}{rccrccrrclc}
\hline\noalign{\smallskip}
1~   &2         &3        &4~    &5& 6                 & 7~~~         & 8~~~          & 9  & ~~10     & 11        \\
\hline\noalign{\smallskip}
No   &RA        &Dec      &\perr &E& Count Rate         &HR1~~         &HR2~~          &Off &Rorkey    &Survey Rate \\
     &(2000.0)  &         &      & & [\ct]             &              &               &[\arcmin]&     & [\ct]    \\
\noalign{\smallskip}\hline\noalign{\smallskip}
  61 &$^a$5 43 35.0 &-64 22 56&$^a$1.9 &5& 6.53e-2$\pm$8.8e-3&-0.00$\pm$0.13& 0.05$\pm$0.19 &33  &140639p   &6.38e-2$\pm$8.1e-3\\ 
  78 &5 36 21.7 &-64 49 42&  6.0 &5& 3.68e-2$\pm$5.3e-3& 0.53$\pm$0.13&-0.06$\pm$0.17 &10  &140635p   &2.52e-2$\pm$5.1e-3\\ 
 106 &5 31 36.1 &-65 18 16& 18.8 &2& 2.49e-2$\pm$1.6e-3& 1.00$-$0.39& 0.23$\pm$0.06 &36  &200692p   &3.13e-2$\pm$4.4e-3\\ 
 122 &5 28 44.4 &-65 26 59&  0.6 &2&    8.07$\pm$0.08  &-0.00$\pm$0.01& 0.07$\pm$0.01 &2.4 &200874p-0   &   5.58$\pm$2.0e-2\\ 
 131 &5 35 53.8 &-65 30 34& 13.0 &2& 1.31e-1$\pm$8.1e-3& 1.00$-$0.19& 0.22$\pm$0.06 &32  &201250p   &1.34e-1$\pm$7.6e-3\\ 
\noalign{\smallskip}
 137 &5 32 25.3 &-65 35 09& 17.4 &2& 7.09e-3$\pm$1.8e-3& 1.00$-$0.47& 0.14$\pm$0.30 &15 &201253p   &6.69e-3$\pm$2.3e-3\\ 
 184 &5 32 32.1 &-65 51 42&  3.3 &2& 1.11e-2$\pm$6.3e-4& 1.00$-$0.10& 0.43$\pm$0.05 &11  &200692p   &6.43e-3$\pm$2.7e-3\\ 
 204 &5 29 48.2 &-65 56 44&  2.8 &5& 2.43e-1$\pm$1.6e-2& 0.84$\pm$0.04& 0.49$\pm$0.06 &9.0 &201255p   &   1.9e-3         \\
 252 &5 31 12.9 &-66 07 04&  2.2 &5& 5.34e-1$\pm$2.1e-2& 0.64$\pm$0.03& 0.27$\pm$0.04 &13  &201257p   &   5.1e-3         \\
 316 &5 32 49.4 &-66 22 13&  0.6 &2& 4.30e-1$\pm$5.5e-3& 0.51$\pm$0.01& 0.12$\pm$0.02 &2.3 &400246p   &   1.63$\pm$2.0e-2\\
\noalign{\smallskip} 
 380 &5 03 02.8 &-66 33 44&  9.0 &2& 1.17e-1$\pm$3.7e-3& 0.83$\pm$0.03& 0.17$\pm$0.03 &39  &900320p   &7.09e-2$\pm$1.0e-2\\ 
 436 &5 35 41.7 &-66 51 58&  9.8 &2& 1.32e-2$\pm$3.8e-3& 1.00$-$0.40& 0.23$\pm$0.28 &4.7 &900552p   &6.06e-1$\pm$1.4e-2\\ 
 439 &5 37 10.2 &-66 53 07&  8.7 &5& 5.21e-2$\pm$8.9e-3& 0.14$\pm$0.17& 0.19$\pm$0.22 &11  &900535p-1 &   1.5e-2         \\
 462 &5 35 05.9 &-67 00 16&  4.0 &2& 6.38e-2$\pm$7.2e-3& 1.00$-$0.15& 0.41$\pm$0.11 &3.8 &900549p   &   2.7e-3         \\
 477 &5 35 38.4 &-67 05 13&  7.9 &5& 5.28e-2$\pm$7.9e-3&-0.02$\pm$0.15& 0.19$\pm$0.21 &11  &900552p   &   1.8e-2         \\
\noalign{\smallskip} 
 478 &5 30 49.4 &-67 05 54& 11.4 &5& 4.77e-2$\pm$8.9e-3&-0.25$\pm$0.18& 0.34$\pm$0.28 &13  &900547p-1 &9.70e-3$\pm$2.8e-3\\ 
 509 &5 15 59.2 &-67 16 28&  5.1 &5& 2.17e-2$\pm$1.9e-3&-0.11$\pm$0.09& 0.26$\pm$0.12 &12  &500052p-1 &   1.8e-2         \\
 513 &5 12 41.8 &-67 17 23&  4.0 &2& 1.31e-2$\pm$1.4e-3& 1.00$-$0.17& 0.54$\pm$0.10 &8.0 &500052p-1 &   5.6e-3         \\
 569 &$^a$5 07 12.1 &-67 43 11 &$^a$9.8 &1& 9.33e-3$\pm$1.6e-3&-1.00$^b$ &       -       &18  &500063p   &      2.2e-2      \\
 782 &4 54 01.8 &-69 00 34& 11.4 &5& 9.49e-1$\pm$9.4e-2& 0.46$\pm$0.09&-0.73$\pm$0.08 &23  &500258p-2 &   4.6e-3         \\ 
\noalign{\smallskip} 
 914 &5 32 45.1 &-69 26 15&  6.5 &5& 1.84e-2$\pm$3.3e-3& 1.00$-$0.31& 0.29$\pm$0.19 &7.3 &110173p   &   6.4e-3         \\
 935 &5 16 45.5 &-69 29 41& 28.4 &5& 1.11e-1$\pm$2.6e-2& 0.10$\pm$0.16& 0.00$\pm$0.60 &25  &110088p   &   1.1e-2         \\
 946 &5 20 30.3 &-69 32 04& 16.6 &4& 4.83e-2$\pm$4.0e-3& 1.00$-$0.13& 0.59$\pm$0.07 &33  &300126p   &   1.6e-2         \\
1030 &5 13 50.9 &-69 51 46&  1.0 &1&    1.94$\pm$0.02  &-0.86$\pm$0.01&-0.98$\pm$0.01 &2.3 &900398p-2 &   1.14$\pm$0.03\\
1039 &5 27 48.7 &-69 54 07&  2.8 &1& 1.11e-1$\pm$4.5e-3&-1.00$+$0.01&       -       &2.3 &400148p   &1.23e-1$\pm$1.1e-2\\ 
\noalign{\smallskip} 
1093 &5 25 57.7 &-70 11 03&  3.7 &5& 4.14e-2$\pm$2.7e-3& 0.68$\pm$0.06& 0.23$\pm$0.07 &15  &300126p   &1.62e-2$\pm$4.7e-3\\ 
1161 &5 37 44.1 &-70 33 50& 17.2 &1& 3.53e-3$\pm$8.4e-4&-1.00$+$0.33&       -       &13  &300335p   &   4.4e-3         \\
1225 &5 44 06.3 &-71 00 50&  3.3 &4& 4.41e-2$\pm$2.0e-3& 1.00$-$0.03& 0.65$\pm$0.03 &15  &400013p   &   4.8e-3         \\
\noalign{\smallskip}\hline\noalign{\smallskip}
\end{tabular}\end{flushleft}
Column 1: catalogue entry; 
     2-3: coordinates;
       4: 90\% statistical position uncertainty, the systematic error is
          $\sim$7\arcsec;
       5: energy band of detection as described in text; 
       6: count rate in broad band (5);
     7,8: hardness ratios HR1=(hard-soft)/(hard+soft) and 
          HR2=(hard2-hard1)/(hard2+hard1) with count rates from the energy 
          bands as defined in text;
       9: off-axis angle;
      10: observation identifier; 
      11: survey count rate from Pietsch et al. 1998, 
          rates without errors are 2$\sigma$ upper limits\\
     $^a$ Improved coordinates derived from HRI observation\\
     $^b$ Only counts in soft band
\end{table*}




\begin{table*}
\caption[]{Variable sources in the LMC region II.}
\begin{flushleft}\begin{tabular}{rcccccccccl}
\hline\noalign{\smallskip}
1   &2     &3      &4       & 5      & 6   & 7 & 8& 9&10& 11    \\
\hline\noalign{\smallskip}
No  & Ul   & Min   & Max    & Sup    & Var & P &N$_g$ &N$_s$ &N$_u$ & Remarks\\
 &10$^{-2}$& \ct   & \ct    & \ct    &     & $\sigma$ & & & &   \\
    &\ct   &       &        &        &     &          & & & &   \\
\noalign{\smallskip}\hline\noalign{\smallskip}
  61& 1.82 & 0.065 &  0.169 &        &     $>$9.3   &$>$4.6& 3& 0& 2& RASS 280\\
  78&      & 0.026 &  0.086 &        &     3.3   &4.8& 4& 0& 0& RASS 250, GSC 8887.0400\\
 106& 0.80 &       &        &  0.067 &       $>$8.3 &$>$4.8& 0& 1& 1& RASS 223\\
 122&      & 4.923 & 17.215 &        &     3.5   &   &17& 0& 0& Fg Star K0, HD 36705, CAL 42, RASS 216\\
 131& 5.38 & 0.114 &  0.348 &  0.553 &    $>$10     &   & 5& 3& 2& RASS 246\\
\noalign{\smallskip}
 137&      & 0.007 &  0.016 &        &     2.2   &$<$3& 5& 0& 0& RASS 228\\                                                    
 184& 0.20 & 0.008 &  0.047 &        &    $>$24     &   & 6& 0& 3& RXJ0532.5-6551, HMXB OB, RASS 231 (H97)\\
 204& 0.13 & 0.004 &  0.243 &        &   $>$187     &   & 4& 0& 5& RXJ0529.8-6556, Be/X pulsar (H95b)\\
 252& 0.31 & 0.022 &  0.534 &        &   $>$172     &   & 3& 0& 7& EXO053109-6609, Be/X pulsar (H95a, D96)\\
 316& 4.38 & 0.238 &  9.523 & 12.218 &   $>$279     &   &19& 1& 2& LMC\,X-4, HMXB pulsar, CAL 49, RASS 232\\
\noalign{\smallskip}
 380&      & 0.040 &  0.117 &  0.210 &     $>$5.3   &   & 2& 1& 0& 1E0502-667, Sy1 (S94), CAL F, RASS 125\\
 436& 0.63 & 0.008 &  0.478 &        &    $>$77$^a$ &   & 9& 0& 1& A0538-66, Be/X pulsar, RASS 244 (M93)\\
 439& 0.57 & 0.006 &  0.052 &        &     $>$9.2   &$>$4.1& 7& 0& 1& \\
 462& 0.26 & 0.064 &  0.064 &        &    $>$24     &$>$5.5& 1& 0&16& \\
 477&      & 0.008 &  0.085 &  0.103 &    $>$13     &   & 8& 2& 0& \\
\noalign{\smallskip}
 478&      & 0.008 &  0.049 &        &     6.0   &4.9& 7& 0& 0& Fg star, dMe (S94), CAL B, RASS 221\\
 509&      & 0.006 &  0.022 &        &     3.4   &   & 2& 0& 0& \\
 513& 0.14 & 0.013 &  0.013 &        &     $>$9.3   &$>$5.9& 1& 0& 1& \\
 569& 0.08 &       &        &  0.009 &    $>$11$^a$ &$>$4.7& 0& 1& 1& \\
 782& 0.33 &       &        &  0.949 &   $>$286     &   & 0& 1& 1& \\
\noalign{\smallskip}
 914&      & 0.003 &  0.022 &        &    6.8$^a$&4.9& 5& 0& 0& (W91)\\
 935& 0.78 & 0.111 &  0.111 &  0.152 &    $>$20     &$>$4.3& 1& 2&11& \\
 946& 0.25 &       &        &  0.048 &    $>$19     &   & 0& 1& 1& RXJ0520.5-6932, HMXB? O8e (S94)\\
1030& 0.25 & 1.936 &  1.936 &        &   $>$760     &   & 1& 0& 7& RXJ0513.9-6951, SSS, HV5682, RASS 167\\    
1039&      & 0.028 &  0.208 &  0.258 &     $>$9.4   &   &14& 2& 0& RXJ0527.8-6954, SSS, RASS 212\\
\noalign{\smallskip}
1093& 2.87 & 0.041 &  0.158 &  0.252 &    $>$8.8$^a$&   & 3& 2& 2& Fg star, RS CVn (S94), CAL 38, RASS 206\\
1161&      & 0.004 &  0.020 &        &     5.7   &   & 2& 0& 0& RXJ0537.7-7034, SSS? (O97)\\
1225&      & 0.011 &  0.044 &        &    4.2$^a$&   & 2& 0& 0& \\
\noalign{\smallskip}\hline\noalign{\smallskip}
\end{tabular}\end{flushleft}
Column 1: catalogue entry, 
       2: lowest upper limit, 
       3: detection minimum, 
       4: detection maximum, 
       5: highest detection influenced by support structure 
          (which gives a lower limit),
       6: variability, 
       7: probability for variability in $\sigma$ (not given if higher
          than 6), 
  8,9,10: number of good detections, detections near WSS 
          and upper limits, used for the variability study, 
      11: the RASS numbers denote the source number from the all-sky LMC 
          source catalogue of Pietsch et al. (1998), 
      Fg stands for Foreground
$^a$ Variability amplitude (and also the confidence of the variability) 
    increases when including survey detections 
   (source 436: var = 1240; 1093: 16) or HRI results (569: 44; 914: 16; 1225: 11)\\
D96: Dennerl et al. 1996;
H95a: Haberl et al. 1995a; H95b: Haberl et al. 1995b; H97: Haberl et al. 1997;
M93: Mavromatakis \& Haberl 1993;
S94: Schmidtke et al. 1994; W91: Wang et al. 1991; O97: Orio et al. 1997

\end{table*}
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