\begin{table}%t1
\par
\caption{\label{tab:events}Summary\tablefootmark{\dagger} of the, so far, 15 dwarf star microlensing events in the Bulge that have been observed with high-resolution spectrographs. 
They have been sorted according to their metallicities (as given in Table~\ref{tab:parameters}).}
\small%\centering
\par
\begin{tabular}{rcccccrrrrrlll}
\hline\hline
\noalign{\smallskip}
\multicolumn{1}{c}{Object}     &
RAJ2000                        &
DEJ2000                        &
 $l$                           &
 $b$                           &
 \multicolumn{1}{c}{$T_{\rm E}$}   &
 $T_{\rm max}$                     &  
 $A_{\rm max}$                     &
 \multicolumn{1}{c}{$T_{\rm obs}$} &  
 Exp.                          &
 $S/N$                         &
 Spec.                         &
 \multicolumn{1}{c}{$R$}       &
 Ref.                          \\
                               &
[hh:mm:ss]                     &
[dd:mm:ss]                     &
 [deg]                         &    
 [deg]                         &  
 [days]                        &
 [HJD]                         &
                               &   
 \multicolumn{1}{c}{[MJD]}     &  
 \multicolumn{1}{c}{[s]}       &
                               &
                               &
                               &
                               \\  
\noalign{\smallskip}
\hline
\noalign{\smallskip}
 OGLE-2009-BLG-076S$\phantom{^{b}}$ & 17:58:31.9 & $-$29:12:17.8 & $+1.21$  &  $-2.56$ & 36.9 &  4916.46   &  70 & 4916.291 &       7200  &  \phantom{1}30      &  UVES  & 45~000    & B09a \\ %\cite{bensby2009letter}    \\
  MOA-2009-BLG-493S$\phantom{^{b}}$ & 17:55:46.0 & $-$28:48:25.8 & $+1.25$  &  $-1.84$ & 13.2 &  5094.61   & 150 & 5093.980 &       7200  &  \phantom{1}40      &  UVES  & 45~000    & TW   \\ %This study                 \\
  MOA-2009-BLG-133S$\phantom{^{b}}$ & 18:06:32.8 & $-$31:30:10.7 & $+0.05$  &  $-5.19$ & 26.6 &  4932.10   &  70 & 4932.233 &       7200  &  \phantom{1}35      &  UVES  & 45~000    & TW   \\ %This study                 \\
  MOA-2009-BLG-475S$\phantom{^{b}}$ & 18:02:27.3 & $-$27:26:49.9 & $+3.16$  &  $-2.45$ & 34.0 &  5084.92   &  62 & 5084.980 &       7200  &  \phantom{1}20      &  UVES  & 45~000    & TW   \\ %This study                 \\
MACHO-1999-BLG-022S\tablefootmark{\ddag}       & 18:05:05.8 & $-$28:34:39.5 & $+2.46$  &  $-3.51$ &265.0 &  1365.50   &  28 & 1366.315 &      12600  &  \phantom{1}80      &  HIRES & 29~000    & C03  \\ %\cite{cavallo2003}         \\
 OGLE-2008-BLG-209S$\phantom{^{b}}$ & 18:04:50.0 & $-$29:42:35.3 & $+1.44$  &  $-4.01$ & 19.5 &  4606.09   &  30 & 4606.833 &       5400  &  \phantom{1}30      &  MIKE  & 47~000    & B09b \\ %\cite{bensby2009}          \\
  MOA-2009-BLG-489S$\phantom{^{b}}$ & 17:57:46.5 & $-$28:38:57.8 & $+1.61$  &  $-2.14$ & 58.9 &  5095.52   & 103 & 5094.982 &       7200  &  \phantom{1}65      &  UVES  & 45~000    & TW   \\ %This study                 \\
  MOA-2009-BLG-456S$\phantom{^{b}}$ & 17:48:56.3 & $-$34:13:32.3 & $-4.16$  &  $-3.34$ & 36.2 &  5090.94   &  77 & 5090.982 &       7200  &  \phantom{1}45      &  UVES  & 45~000    & TW   \\ %This study                 \\
 OGLE-2007-BLG-514S$\phantom{^{b}}$ & 17:58:03.0 & $-$27:31:08.2 & $+2.62$  &  $-1.63$ & 76.0 &  4386.28   &1200 & 4385.985 &       4800  &  \phantom{1}30      &  MIKE  & 25~000    & E10  \\ %\cite{epstein2009}         \\
  MOA-2009-BLG-259S$\phantom{^{b}}$ & 17:57:57.6 & $-$29:11:39.1 & $+1.15$  &  $-2.45$ & 69.1 &  5016.77   & 220 & 5016.227 &       7920  &  \phantom{1}50      &  UVES  & 45~000    & TW   \\ %This study                 \\
  MOA-2008-BLG-311S$\phantom{^{b}}$ & 17:56:53.7 & $-$31:23:40.3 & $-0.87$  &  $-3.35$ & 15.7 &  4655.40   & 400 & 4654.952 &       7200  &  \phantom{1}85      &  MIKE  & 29~000    & C09  \\ %\cite{cohen2009}           \\
  MOA-2008-BLG-310S$\phantom{^{b}}$ & 17:54:14.4 & $-$34:46:37.7 & $-4.09$  &  $-4.56$ &  7.1 &  4656.39   & 280 & 4655.957 &       7200  &  \phantom{1}90      &  MIKE  & 41~000    & C09  \\ %\cite{cohen2009}           \\
 OGLE-2007-BLG-349S$\phantom{^{b}}$ & 18:05:23.0 & $-$26:25:27.1 & $+4.38$  &  $-2.52$ &109.4 &  4348.56   & 400 & 4348.237 &       3050  &  \phantom{1}90      &  HIRES & 48~000    & C08  \\ %\cite{cohen2008}           \\
  MOA-2006-BLG-099S$\phantom{^{b}}$ & 17:54:10.2 & $-$35:13:34.9 & $-4.48$  &  $-4.78$ & 30.1 &  3940.35   & 380 & 3940.090 &       2400  &  \phantom{1}30      &  MIKE  & 19~000    & J08  \\ %\cite{johnson2008}         \\
 OGLE-2006-BLG-265S$\phantom{^{b}}$ & 18:07:18.9 & $-$27:47:44.0 & $+3.38$  &  $-3.55$ & 28.6 &  3893.24   & 212 & 3892.581 &        900  &  \phantom{1}45      &  HIRES & 45~000    & J07  \\ 
\hline
\end{tabular}
\tablefoot{\tablefoottext{\dagger}{Given for each microlensing event is: RA and DE coordinates (J2000) read from the
fits headers of the spectra (the direction where the telescope pointed during observation); 
galactic coordinates ($l$ and $b$); 
duration of the event in days ($T_{\rm E}$); time when maximum magnification occured ($T_{\rm max}$); 
maximum magnification ($A_{\rm max}$); time when event was observed
with high-resolution spectrograph ($T_{\rm obs}$); magnification at the time
of observation ($A_{\rm obs}$); the exposure time (Exp.),
the measured signal-to-noise ration per pixel at $\sim$6400~{\AA}; the
spectrograph that was used; the spectral resolution; and the
reference where the star first appeared: TW~=~This Work, B09a~=~\cite{bensby2009letter},
B09b~=~\cite{bensby2009}, J07~=~\cite{johnson2007}, J08~=~\cite{johnson2008},
C08~=~\cite{cohen2008}, C09~=~\cite{cohen2009}, C03~=~\cite{cavallo2003}, E10~=~\cite{epstein2010}.}
\tablefoottext{\ddag}{MACHO ID: 109.20893.3423.}}
\end{table}