\begin{table}%t1
\par
\caption{\label{tab:log-gen} Log of the \xte\ observations analysed in this paper.}
%\centerline
{
\small\begin{tabular}{c c c c  c c c}
\hline \hline
Observatory &Instrument & Bandpass & Period &
Total Exposure & Number & Observation Type \\
& &   & (MJD--53596.5)$^a$ & (ks) & of Obs. &\\
\hline
\integral & IBIS/ISGRI & 18--200~keV & 2.5--23.8 & 315 & 3/4  & ToO (5$\times$5$^b$)/Galactic Bulge$^c$ (hex$^d$)\\
 & JEM-X & 5--25~keV & 5.9--14.8 & 240 & 3 & ToO \\ 
\rxte & PCA & 3--25~keV  & 3.1--103.3    & 146      & 54   & Public\\
 & HEXTE        & 20--150~keV & 3.1--103.3    & 146      & 54   & Public\\
\swift$^e$    & XRT          & 0.3--10~keV   & 5.8 & 0.13     & 1    & Public \\
REM$^e$       & ROSS         & 550--800~nm  & 22.7--76.5     & 3.2      & 10   & ToO \\
NTT$^e$       & SUSI-2         & 320--900~nm  & 9.6--0.6      & 1    & ToO \\
VLA$^e$       & L,C,X,U      & 1.4--15~GHz  & 5.6--196.01     & 4.8/15.4 & 1/13 & ToO/Public\\
VLBA$^e$ & S/X & 2.3-8.4~GHz & 8.54--8.67 & 10.8 & 1 & ToO \\ 
\hline
\end{tabular}}
\medskip
\par
Notes:\\
$^a$ MJD 53596.5 corresponds to the maximum flux of the source measured during the period covered by \rxte/ASM.\\
$^b$ 5$\times$5 dither pattern around the nominal target location.\\
$^c$ Monitoring program of E. Kuulkers et~al. (see \citealt{Kuulkers:2007}).\\
$^d$ Hexagonal pattern around the nominal target location.\\
$^e$ Snap-shot observations with the specified instruments or receivers.  
\end{table}