\begin{table}%t1
\par
\caption{\label{GRBtable1}Properties of GRBs observed with HESS from March 2003 to October 2007.}
%\centerline
 {
\begin{tabular}{lccll@{}rc@{}c@{}rc@{}c@{}cl@{}r}
\hline\hline
      GRB   & Satellite  & Trigger & RA$^a$ & Dec$^a$ & Error$^a$ & Energy band &
      Fluence$^b$
      & $T_{\rm 90}^b$ & X$^c$ & O$^c$ & R$^c$ & $z$ & Rank$^d$  \\
            &              & number &                            &      & ($\arcsec$) & (keV) & ($10^{-8}$~erg~cm$^{-2}$) & (s)  &  &  & \\
    \hline
    071003  & {\it Swift} & 292~934 & $20^{\rm h}07^{\rm m}24\fs25$ & +$10\degr56\arcmin48\farcs8$  & 5.7 & 15--150     & 830     &
    $\sim$150      & $\surd$ & $\surd$ & $\surd$   & 1.604$^e$    & 5  \\
    070808  & {\it Swift} & 287~260 & $00^{\rm h}27^{\rm m}03\fs36$ & +$01\degr10\arcmin34\farcs8$  & 1.9 & 15--150     & 120     & $\sim$32        & $\surd$ & $\surd$ & $.$       & $\cdots$ & 9  \\
    %070805  & {\it Swift} & 287088 & 15--150     & 72      & 31$\pm$1        & $\times\times$ & $.$     &        & 2  \\
    070724A & {\it Swift} & 285~948 & $01^{\rm h}51^{\rm m}13\fs96$ & --$18\degr35\arcmin40\farcs1$  & 2.2 & 15--150     & 3       &
    $\sim$0.4    & $\surd$ & $\times$ & $\times$ & 0.457$^f$  & 21 \\
    070721B & {\it Swift} & 285~654 & $02^{\rm h}12^{\rm m}32\fs95$ & --$02\degr11\arcmin40\farcs6$  & 0.9 & 15--150     & 360     & $\sim$340      & $\surd$ & $\surd$ & $\times$  & 3.626$^g$  & 10 \\
    070721A & {\it Swift} & 285~653 & $00^{\rm h}12^{\rm m}39\fs24$ & --$28\degr22\arcmin00\farcs6$  & 2.3 & 15--150     & 7.1     & 3.868   & $\surd$ & $\surd$ & $.$ & $\cdots$ & 20 \\
    070621  & {\it Swift} & 282~808 & $21^{\rm h}35^{\rm m}10\fs14$ & --$24\degr49\arcmin03\farcs1$  & 2   & 15--150     & 430     & 33      & $\surd$ & $\times$ & $.$ & $\cdots$ & 1  \\
    070612B & {\it Swift} & 282~073 & $17^{\rm h}26^{\rm m}54\fs4$  & --$08\degr45\arcmin08\farcs7$  & 4.7 & 15--150     & 168     & 13.5    & $\surd$ & $\times$ & $.$ & $\cdots$ & 15 \\
    070429A & {\it Swift} & 277~571 & $19^{\rm h}50^{\rm m}48\fs8$  & --$32\degr24\arcmin17\farcs9$  & 2.4 & 15--150     & 91      & 163.3   & $\surd$ & $\surd$ & $.$ & $\cdots$ & 3  \\
    070419B & {\it Swift} & 276~212 & $21^{\rm h}02^{\rm m}49\fs57$ & --$31\degr15\arcmin49\farcs7$  & 3.5 & 15--150     & 736     & 236.4   & $\surd$ & $\surd$ & $.$ & $\cdots$ & 7  \\
    070209  & {\it Swift} & 259~803 & $03^{\rm h}04^{\rm m}50^{\rm s}$  & --$47\degr22\arcmin30\arcsec$  & 168 & 15--150     & 2.2     & 0.09
    & $\times$ & $\times$ & $.$     & 0.314?$^h$ & 22 \\
    061110A & {\it Swift} & 238~108 & $22^{\rm h}25^{\rm m}09\fs9$  & --$02\degr15\arcmin30\farcs7$  & 3.7 & 15--150     & 106     & 40.7    & $\surd$ & $\surd$ & $.$ & 0.758$^i$   & 11 \\
    060526  & {\it Swift} & 211~957 & $15^{\rm h}31^{\rm m}18\fs4$  & +$00\degr17\arcmin11\farcs0$  & 6.8 & 15--150     & 126     & 298.2   & $\surd$ & $\surd$ & $.$ & 3.21$^j$   & 8 \\
    060505  & {\it Swift} & 208~654 & $22^{\rm h}07^{\rm m}04\fs50$ & --$27\degr49\arcmin57\farcs8$  & 4.7 & 15--150     & 94.4    & $\sim$4 & $\surd$ & $\surd$ & $.$ & 0.0889$^k$ & 18 \\
    060403  & {\it Swift} & 203~755 & $18^{\rm h}49^{\rm m}21\fs80$ & +$08\degr19\arcmin45\farcs3$  & 5.5 & 15--150     & 135     & 30.1    & $\surd$ & $\times$ & $.$ & $\cdots$ & 16 \\
    050801  & {\it Swift} & 148~522 & $13^{\rm h}36^{\rm m}35^{\rm s}$ & --$21\degr55\arcmin41\arcsec$ & 1   & 15--150     & 31      & 19.4    & $\surd$ & $\surd$ & $\times$ & 1.56$^l$  & 2  \\
    050726  & {\it Swift} & 147~788 & $13^{\rm h}20^{\rm m}12\fs30$ & --$32\degr03\arcmin50\farcs8$  & 6   & 15--150     & 194     & 49.9    & $\surd$ & $\surd$ & $.$ & $\cdots$ & 13 \\
    050509C & {\it HETE-II}      & H3751  & $12^{\rm h}52^{\rm m}53\fs94$ & --$44\degr50\arcmin04\farcs1$  & 1   & 2--30       & 60      & 25      & $\surd$ & $\surd$ & $\surd$ & $\cdots$ & 19 \\% XRF
    050209  & {\it HETE-II}      & U11568 & $08^{\rm h}26^{\rm m}$ & +$19\degr41\arcmin$ & 420 & 30--400     & 200     & 46 & $.$ & $\times$ & $.$ & $\cdots$ & 14 \\
    041211B$^m$  & {\it HETE-II}      & H3622  & $06^{\rm h}43^{\rm m}12^{\rm s}$ & +$20\degr23\arcmin42\arcsec$ & 80  & 30--400     & 1000    & $>$100  & $.$ & $\times$ & $.$  & $\cdots$ & 4  \\
    041006  & {\it HETE-II}      & H3570  & $00^{\rm h}54^{\rm m}50\fs23$ & +$01\degr14\arcmin04\farcs9$  & 0.1 & 30--400       & 713    & $\sim$20 & $\surd$ & $\surd$ & $\surd$ & 0.716$^n$  & 6 \\
    030821  & {\it HETE-II}      & H2814  & $21^{\rm h}42^{\rm m}$  & -$44\degr52$   & $^o$    & 30--400   & 280     & 23      & $.$ & $.$ & $.$       & $\cdots$ & 17 \\
    030329  & {\it HETE-II}      & H2652  & $10^{\rm h}44^{\rm m}49\fs96$ & +$21\degr31\arcmin17\farcs44$ & $10^{-3}$ & 30--400   & 10~760   & 33      & $\surd$ & $\surd$ & $\surd$ & 0.1687$^p$ & 12 \\
    \hline
\end{tabular}}
\par
\smallskip
\par
$^a$  {RA, Dec, and the positional errors (90\% containment) were taken from GCN Reports (\url{http://gcn.gsfc.nasa.gov/report_archive.html}) for GRB~061110A -- GRB~071003 and GCN Circulars otherwise.}
$^b$ {Fluence and $T_{\rm 90}$~data for
        GRB~050726 -- GRB~070612B were taken from~\citet{sakamoto08} except that
        $T_{\rm 90}$ of GRB~060505 was taken
        from~\citet{Palmer06_GCN5076}. Fluence and $T_{\rm 90}$ data of
        GRB~030329 and GRB~030821 were taken from \citet{sakamoto05}, and those of GRB~041006 from \citet{Shirasaki08}. Other data were taken from GCN Circulars and {\it HETE} pages (\url{http://space.mit.edu/HETE/Bursts}).}
$^c$   {X: X-ray, O: optical, R: radio;
        ``$\surd$'' indicates the detection of a counterpart, ``$\times$'' a
        null detection, and ``$.$'' that no measurement was reported in
        the corresponding energy range, from
        \url{http://grad40.as.utexas.edu/grblog.php}}
$^d$   {The
        relative expected VHE flux for each GRB is ranked according to
        the empirical scheme described in Sect.~\ref{sect_rank}.}      
$^e$  {\citet{perley08}}. 
$^f$   {\citet{Cucchiara07_GCN6665}.} 
$^g$  {\citet{Malesani07_GCN6651}}. 
$^h$  {Redshift of a candidate host galaxy~\citet{berger6101}.} 
$^i$ {\citet{Fynbo07_GCN6759}}. 
$^j$  {\citet{berger5170}}. 
$^k$  {\citet{ofek06}}. 
$^l$  {Redshift according to~\citet{pasquale07}, based on afterglow modelling.} 
$^m$   {Although this burst was referred to as GRB~041211 in
      various GCN Circulars, the proper name GRB~041211B~\citep[e.g.,
        in][]{pelangeon06} should be used to distinguish it from another
      burst, GRB~041211A (=H3621) which occurred earlier on the same day
      (P\'elangeon, A., private communication).} 
$^n$ {\citet{soderberg06}.} 
$^o$ {The position error of this burst is large, see Fig.~\ref{030821overlay}.}
$^p$  {\citet{stanek03}.}
\end{table}