\begin{table}%t1
\caption{\label{tab1}Selection of X-ray bursts from \bron\ studied here. For more
details, see \cite{gal06}.}
\par
\small%\centerline
 {
\begin{tabular}{llllc}
\hline\hline
MJD & ObsID & Times & Active & $\Delta^a$ \\
    &       & covered wrt & PCUs  & (\arcmin) \\
    &       & burst start&   &  \\
    &       & time (s)$^b$    & &  \\
\hline
50~971.23019          & 30054-04-02-01  &  --2600/+1200 & 0, 1, 2, 3, 4  & 0.0 \\
50~971.70032          & 30054-04-02-000 &  --2700/+900  & 0, 1, 2, 3, 4  & 0.0 \\
50~988.82503          & 30060-03-01-01  &  --1700/+1800 & 0, 1, 2, 3    & 0.0 \\
51~725.87648          & 50035-01-02-00  &  --3000/+200  & 0, 2, 3, 4    & 0.5 \\ 
51~726.71988$^{c,p,t}$ & 50035-01-02-02  &  --1200/+2100 & 0, 1, 2, 3    & 0.5 \\
51~728.77338$^{c,p,t}$ & 50035-01-02-04  &  --4000/+2600 & 0, 1, 2, 3    & 0.5 \\
51~814.34546$^{c,p,t}$ & 50035-01-03-10  &  --2200/+1500 & 0, 2        & 0.5 \\
52~484.41775$^{c,p,t}$ & 70044-01-01-000 &  --4000/+2200 & 0, 2, 3      & 0.0 \\
52~484.56684$^c$      & 70044-01-01-00  &  --2400/+700  & 0, 2, 3      & 0.0 \\
52~485.00672$^{c,p,t}$ & 70044-01-01-02  &  --4000/+2600 & 0, 2, 3      & 0.0 \\
52~537.22347          & 70025-01-01-00  &  --4000/+2400 & 0, 1, 2, 3    & 0.0 \\
52~738.47686$^{c,p,t}$ & 80048-01-01-04  &  --4000/+3200 & 0, 2, 3      & 0.0 \\
52~738.74636$^{c,p,t}$ & 80048-01-01-07  &  --4000/+2700 & 0, 1, 2, 3    & 0.0 \\
52~820.56256$^{c,p,t}$ & 80049-01-01-00  &  --1100/+2000 & 0, 2, 3, 4    & 0.0 \\
52~893.05439          & 80105-11-01-00  &  --4000/+3000 & 0, 2, 3      & 0.0 \\
53~205.19659$^{c,p,t}$ & 70044-01-02-00  &  --1900/+1500 & 0, 2, 3      & 0.0 \\
53~207.07579          & 90043-01-01-01  &  --4000/+3600 & 0, 2        & 2.5 \\
53~207.21911$^c$      & 90043-01-01-01  &  --4000/+1400 & 0, 2, 3      & 2.5 \\
53~206.49150$^{c,p,t}$ & 90043-01-01-020 &  --4000/+2800 & 0, 2, 3      & 2.5 \\
53~206.63615$^{c,p,t}$ & 90043-01-01-02  &  --4000/+1900 & 0, 2, 3      & 2.5 \\
53~956.08413$^{p,t}$  & 92031-01-01-000 &  --4000/+2200 & 0, 2, 4      & 13.8 \\
53~956.22695$^{p,t}$  & 92031-01-01-000 &  --2100/+1100 & 0, 1, 2      & 13.8 \\
53~957.06785$^{p,t}$  & 92031-01-01-010 &  --4000/+2000 & 0, 2, 3      & 13.8 \\
53~957.20458$^{p,t}$  & 92031-01-01-010 &  --1800/+1600 & 0, 2, 3      & 13.8 \\
53~959.15478$^{p,t}$  & 92031-01-02-000 &  --4000/+2900 & 1, 2        & 13.8 \\
54~167.72354$^{c,p,t}$ & 91017-01-01-000 &  --1900/+1100 & 1, 2        & 0.0 \\
54~168.31443$^{c,p,t}$ & 91017-01-02-03  &  --2000/+1600 & 2          & 0.0 \\
54~168.75518$^{c,p,t}$ & 91017-01-02-010 &  --4000/+2500 & 0, 2, 3      & 0.0 \\
54~168.90229$^{c,p,t}$ & 91017-01-02-010 &  --1900/+1600 & 0, 2        & 0.0 \\
\hline
\end{tabular}}
\medskip
$^a$ Off-axis angle; $^b$~these values are rounded off to an integer times 100~s and may include gaps. $^c$~The spectra for these ObsIDs were used to generate average time-resolved spectra (cf., Fig.~\ref{figxtespectra}); $^p$~data were used to calculate average pre-burst power density spectrum (Fig.~\ref{figpds}); $^t$~data were used to calculate average tail power density spectrum.
\end{table}