\begin{table}
\caption{\label{table2}Properties of the prompt emission of BeppoSAX
Gamma Ray Bursts reported in Table~\ref{table1}. We indicate the
duration and fluence both in the X-ray (2.0--10.0 keV band) and
the $\gamma$-ray (40.0--700 keV band). An X following the source name
denotes an X-ray-rich GRB~or an X-ray flash.}
\small%\centerline

\begin{tabular}{lccccc}
 \hline\hline
GRB~name & $\rm \gamma$-ray    & X-ray  & $\rm \gamma$-ray & X-ray    & Ref.\\
         & duration &  duration     &  fluence     &  fluence &  \\
         & (T, s) & (T, s) & $\rm 10^{-7}$ erg  cm$^{-2}$ & $\rm 10^{-7}$ erg  cm$^{-2}$\\
\hline
\object{GRB~960720} & 8    & 17   &    $26\pm3$           &    $0.8\pm0.2$          &    1, 2, 3    \\
\object{GRB~970111} & 43   & 60   &  $430\pm30$           &  $16\pm1$               &    4, 2, 3     \\
\object{GRB~970228} & 80   & 80   &  $64.5$               &  $15.4$                 &    5      \\
\object{GRB~970402} & 150  & 150  &  $82\pm9$             &  $4.7\pm1.5$            &    2     \\
\object{GRB~970508} & 15   & 29   &  $14.5$               &  $5.3$                  &    5      \\
\object{GRB~971214} & 35   & 35   &  $64.9$               &  $2.34$                 &    5,3      \\
\object{GRB~971227} & 7    & 7    &  $6.6\pm0.7$          &  1                      &    6,3     \\
\object{GRB~980109} & 20   & 20   &  $32.3\pm3$           &     --                 &    3,7     \\
\object{GRB~980326} & 9    & 9    &  $7.5\pm1.5$          &  $2\pm0.3$              &    5, 3      \\
\object{GRB~980329} & 58   & 68   &  $650\pm50$           &  $9.7\pm0.7$            &    5,      \\
\object{GRB~980425} & 31   & 40   &  $28.5\pm5$           &  $7.8\pm0.2$            &    2, 3     \\
\object{GRB~980515} & 15   & 20   &  $23\pm3$             &  -                      &    7, 3     \\
\object{GRB~980519} & 30   & 190  &  $81\pm5$             &  18                     &    8,9, 3  \\
\object{GRB~980613} & 50   & 50   &  $9.9$                &    $2.3$                &    5, 3      \\
\object{GRB~981226X}& 20   & 260  &  $4\pm1$              &  $5.7\pm1$              &    10,3       \\
\object{GRB~980703} & 90   & --  & $\rm 300\pm100$           &      --                &    11     \\
\object{GRB~990123} & 100  & 100  & $\rm 1790$                &     $22.9$              &    5, 3      \\
\object{GRB~990217} & 25   & 25   & $\rm 12.7\pm1.5$          &      --                &    7, 3     \\
\object{GRB~990510} & 75   & 80   & $\rm 181$                 &  $17.9$                 &    3, 5       \\
\object{GRB~990625} & 11   & 11   &     --               &     --                 &    3        \\
\object{GRB~990627} & 28   & 60   &     --               &   $\sim$$15$              &    3,12       \\
\object{GRB~990704X}& 23   & 40   & $\rm 10\pm1$              & $\rm 15\pm0.8$              &    13, 3     \\
\object{GRB~990705} & 42   & 45   & $\rm 423$                 & $\rm 22.5$                  &    5, 3      \\
\object{GRB~990712} & 30   & 30   & $\rm 65\pm3$              & $\rm 28.6$                  &    5, 3      \\
\object{GRB~990806} & 30   & 30   & $\sim$$42$              & $\sim$$2.5$               &    14, 3     \\
\object{GRB~990907} & 1    & 220  &     --               &     --                 &    3        \\
\object{GRB~990908} & 50   & 130  &     --               &     --                 &    3       \\
\object{GRB~991014} & 3    & 10   & $\rm 9\pm1$               & 1                       &    15,16, 3    \\
\object{GRB~991105} & 13   & 40   &     --               &      --                &    3         \\
\object{GRB~991106}$^{ a}$ & --  & 5  & $<$$1.2$$^{b}$ &                    &  17      \\
\object{GRB~000210} & 10   & 115  & $\rm 610\pm20$            & $\sim$$15$                &    18, 3    \\
\object{GRB~000214} & 115  & 100  & $\rm 61.7$                & $\rm 11.6$                  &    5, 3      \\
\object{GRB~000528} & 80   & 120  & $\rm 14.4\pm0.4$          &      --                &    19, 20    \\
\object{GRB~000529} & 14   & 30   &     --               &     --                 &    3         \\
\object{GRB~000615X}& 12   & 120  & $\rm 9.8\pm0.9$           & $\rm 17\pm1$                &    21, 3    \\
\object{GRB~000620} & 15   & 20   &    --                &    --                  &    3       \\
\object{GRB~001011} & 31   & 60   &    --                &    --                  &    3          \\
\object{GRB~001109} & 60   & 65   & $\rm 49.7\pm1.9$          & $\rm 6.4\pm0.33$            &    22, 3     \\
\object{GRB~010213} & 23   & 25   &    --                &    --                  &    3          \\
\object{GRB~010214} & 15   & 30   & $\rm 45\pm0.8$            & $\rm 2\pm0.3$               &    23    \\
\object{GRB~010220} & 40   & 150  &    --                &   --                   &    3      \\
\object{GRB~010222} & 170  & 280  & $\rm 753$                 & $\rm 95$                    &    5, 3       \\
\object{GRB~010304} & 15   & 24   &    --                &   --                   &    3     \\
\object{GRB~010501} & 37   & 41   &    --                &   --                   &    3      \\
\object{GRB~010412} & 74   & 90   &    --                &   --                   &    3         \\
\object{GRB~010518} & 25   & 30   &    --                &   --                   &    3         \\
\object{GRB~011121} & 105  & 100  & $\rm 1000\pm20$           & $\rm 140\pm3$               &    24, 3 \\
\object{GRB~011211} & 400  & 400  & $\rm 37\pm4$              & $\rm 11\pm1$                &    24, 3 \\
\object{GRB~020321} & 70   & 90   & 30                    & 0.9                     &    25, 3        \\\hline
\object{GRB~020322} & 15   & 50   & --                   & --                     &    3         \\
\object{GRB~020409} & 40   & 60   & --                   & --                     &    3        \\
\object{GRB~020410} & 1800 &$>$1290& $\sim$$290$            & $>$$47$                   &    26, 3     \\
\object{GRB~020427X}&  -- & 60   &      $<$$2.9$           &  $3.7\pm0.3$            &    27, 3 \\
\hline
\end{tabular}
\smallskip
$^a$ Perhaps not a GRB. See Cornelisse et~al. (2000).\\
$^b$ Conservative $3\sigma$ upper limit based on GCN 448.\\
References:
1:~\citet{piro98}, 
2:~\citet{fro00a},
3:~\citet{fro04}, 
4:~\citet{fer98}, 
5:~\citet{ama02a},
6:~\citet{ant99}, 
7:~\citet{ama99}, 
8:~\citet{nic98}, 
9:~\citet{zan99}, 
10:~\citet{fro00b}, 
11:~\citet{ama98}, 
12:~\citet{mul99b},
13:~\citet{fer01}, 
14:~\citet{mon01}, 
15:~\citet{tas99}, 
16:~\citet{zan00b},
17:~\citet{gan99}, 
18:~\citet{piro02},
19:~\citet{gui00}, 
20:~\citet{zan00a},
21:~\citet{nic01}, 
22:~\citet{gui03}, 
23:~\citet{gui03}, 
24:~\citet{piro05},
25:~\citet{zand03},
26:~\citet{nic04}, 
and 27:~\citet{ama04}.\\
Note 1:  When not available, values of 2--10 keV fluences have been
calculated from the 2--26 keV fluences and assuming the spectral
parameters reported in the references.\\
Note 2: The X-ray and $\gamma$ fluences reported by \citet{ama02a}
have been obtained by reporting the parameters of the WFC
and GRBM spectra fit at $z =0$ (see Table 2 of the same article).
\end{table}