\begin{table}%t4
\caption{\label{tab:bol_lc_paras}Rise times~$t_{\rm peak}$ and peak absolute magnitudes~$M_{\rm peak}^{\rm bol}$ for the UVOIR~bolometric light curves of the~models.}
%\centering
\par
  \begin{tabular}{ccccccc}
    \hline
    \hline\noalign{\smallskip}
    Model & 1 & 2 & 3 & 4 & 5 & 6 \\
    \hline
    $t_{\rm peak}$ [days] & 18.6  & 18.6  & 18.0  & 15.5  & 14.4  & 13.9 \\
    $M_{\rm peak}^{\rm bol}$   & --17.6 & --18.2 & --18.7 & --19.1 & --19.4 & --19.5 \\
    $\Delta m_{15}^{\rm bol}$ & 0.64  & 0.40  & 0.50  & 0.55  & 0.55  & 0.66 \\[2pt]
    \hline
  \end{tabular} 
\tablefoot {$\Delta m_{15}^{\rm bol}$ is the change in bolometric magnitude between maximum light and~15~days thereafter.  Due~to Monte~Carlo noise magnitudes are uncertain by~$\sim$0.1~mag.}
\end{table}