\begin{table}%t2 \caption{\label{tab1.1} The 5 non-\fermi\ GRBs added in this work to the pre-\fermi\ list of 90 GRBs from Ghirlanda et~al. (\cite{Ghirlanda2009}).} \par %%\centerline { \small\begin{tabular}{l l l l l l l l l l} % 7 columns \hline\hline \noalign{\smallskip} % To combine 4 columns into a single one G GRB &$z$ & $\alpha$ & $F$ & $P$ & Range & $L_{\rm iso}$ & $E_{\rm peak}^{\rm rest}$ & $E_{\rm iso}$ & Ref\tablefootmark{**} \\ & & & erg/cm$^{2}$ & ph(erg)/s/cm$^2$ & & erg/s & keV & erg & \\ \hline 080913\tablefootmark{*} & 6.7 & $-0.89\pm 0.52$ & ($8.5\pm 3.5$)e-7 & $1.4 \pm 0.2$ & 15--1000 & ($1.14\pm 0.15$)e53 & $1009 \pm 200$ & ($7.47 \pm 0.9$)e52 & 1 \\ 081028 & 3.038 & $-1.25 \pm 0.38$ & ($3.7 \pm 0.2$)e-6 & $0.5\pm 0.1$ & 15--150 & ($5.0\pm 0.8$)e51 & $234\pm 93$ & ($1.4 \pm 0.22$)e52 & 2 \\ 081121 & 2.512 & $-0.77 \pm 0.15$ & ($1.79\pm 0.34$)e-5 & ($2.6\pm 0.6$)e-6 & 20--7000 & ($1.3\pm 0.13$)e53 & $871\pm 123$ & ($3.2\pm 0.5$)e53 & 3 \\ 090102 & 1.547 & $-0.86\pm 0.14$ & ($3.09\pm 0.27$)e-5 & ($5.1\pm 0.7$)d-6 & 20-2000 & ($8.7\pm 0.56$)e52 & $1149\pm 153$ & ($2.2\pm 0.26$)e53 & 4 \\ 090418A & 1.608 & $-1.3\pm 0.09$ & ($4.6\pm 0.2$)e-6 & $1.9\pm 0.3$ & 15--150 & ($1.1\pm 0.1$)e52 & $1590\pm 604$ & ($1.48\pm 0.15$)e53& 5 \\ \hline \end{tabular}} \tablefoot{\tablefoottext{*}{The peak flux is computed in the 15--150~keV (from gcn 8222).} \tablefoottext{**}{The references of the spectral parameters: (1) Palshin et~al. (\cite{Palshin2008}); (2) Barthelmy et~al. (\cite{Barthelmy2008}); (3) Golenetskii et~al. (\cite{Golenetskiib2008}); (4) Golenetskii et~al. (2009); (5) Palshin et~al. (\cite{Palshin2009}).}} \vspace*{5mm} \end{table}