\begin{table}%t3 \caption{\label{summary_table}Summary of the burst properties of five \textit{Fermi}/LAT bursts.} \par %\centering \par \begin{tabular}{lccccccccc} \hline\hline \noalign{\smallskip} Burst & Redshift & $E_{\gamma, \rm{iso}}$$^1$ & $\alpha$ & $\beta_{\rm opt}$ & Template & $A_{V}^{\rm{host}}$ & $\theta_{\rm jet}^{\rm ISM}$ &$E_{\rm{\gamma}}$$^a$ %\footnotemark[a] & SFR$^b$ %\footnotemark[b] \\ & & erg & & & & & {\it $^\circ$} & {(erg)} & {($M_\odot$ yr$^{-1}$)} \\ \hline \noalign{\smallskip} GRB~090323$^c$ %\footnotemark[c] & 3.57$^{1}$ & $5.1\times 10^{54}$ & $1.90\pm0.01$ & $0.65\pm0.13$ & SMC & $0.14^{\rm +0.04}_{-0.03}$ & ${\la}2.1^\circ$ & ${\la}3.3 \times 10^{51}$ & $\cdots$ \\ GRB~090328 & 0.7354 & $1.0\times 10^{53}$ & $2.27\pm{0.04}$ & $1.19^{\rm +0.24}_{-0.21}$ & SMC & $0.22^{\rm +0.06}_{-0.18}$ & ${\la}5.5^\circ$ & ${\la}4.6 \times 10^{50}$ & 4.8 \\ GRB~090902B & 1.822$^{2}$ & $3.5\times 10^{54}$ & $0.94 \pm 0.02$ & $0.79^{\rm +0.05}_{-0.19}$ & SMC/LMC & ${\la}0.34$ & ${\ga}6.4^\circ$ & ${\ga}2.2 \times 10^{52}$ & $\cdots$ \\ GRB~080916C$^{3}$,$^c$%\footnotemark[c] \footnotemark[c] & 4.35$^{3}$ & $8.8\times 10^{54}$ & $ 1.40 \pm 0.05$ & $0.38^{\rm +0.20}_{-0.19}$ & $\cdots$ & $\cdots$ & ${\ga}6^\circ$ & ${\ga}4.8 \times 10^{52}$ & $\cdots$ \\ GRB~090510 & 0.903 & $1.1\times 10^{53}$ & $\cdots$ & $\cdots$ & $\cdots$ & $\leq$1.1 & $\cdots$ & $\cdots$ & 0.30 \\ \hline \end{tabular} \tablebib {(1) \citet{2009GCN..9028....1C}; (2) \citet{Z_090902B}; (3) \citet{2009AetA...498...89G}. } \tablefoot {\tablefoottext{a}{$E_{\gamma, \rm{iso}}$ values are quoted in the energy range 1~keV$-$10~GeV, with the exception of GRB~080916C (10~keV$-$10~GeV: \citealt{2009arXiv0908.1832F}) and GRB~090510 (10~keV$-$30~GeV: \citealt{090902B_PAPER}).} \tablefoottext{b}{The true SFR may be larger than measured because of slit losses.} \tablefoottext{c}{The opening angle and $E_{\rm{\gamma}}$ are lower in a wind medium for GRB~090323 and~080916C.}} \vspace*{2.5mm} \end{table}