\begin{table}%t3
%\centering
\par
\caption{Parameters of Models O310 and T310. The (baryonic) mass of
the inner core, $M_{\rm core}$, that has been excluded from the
simulation, and the final neutron star mass, $M_{\rm ns}$, are given
in solar masses. The initial and final radius of the inner core,
$R_{\rm core}^{0}$ and $R_{\rm core}^{\infty}$, respectively, are
given in km, and its initial velocity of contraction, $\dot R_{\rm
core}^{0}$, in km~s$^{-1}$.  The initial neutrino luminosities of different
flavours, $L_{\nu_{\rm e},52}^0$, $L_{\bar \nu_{\rm e},52}^0$, and
$L_{\nu_x,52}^0$ (see also the main text), are given in units of $\rm
10^{52}~erg/s$, and the energy loss of the inner core, $\Delta
\varepsilon$, in units of ${M_{\odot}} c^2$. The explosion energy,
$E_{\rm exp,51}$, and the explosion time scale, $t_{\rm exp}$, are
given in $\rm 10^{51}~erg$ and in ms, respectively.}
\label{tab:explosion_models}
\begin{tabular}{lccccccccccccc}
\hline
\hline
  Model                     &  Resolution                           &
  $M_{\rm core}$            &  $R_{\rm core}^{0}$                   &
  $\dot R_{\rm core}^{0}$   &  $R_{\rm core}^{\infty}$              &
  $L_{\nu_{\rm e},52}^0$    &  $L_{\bar \nu_{\rm e},52}^0$          & 
  $L_{\nu_x,52}^0$          & 
  $\Delta Y_{\rm L}$        &  $\Delta \varepsilon$                 &  
  $E_{\rm exp,51}$          &  $t_{\rm exp}$                        &
  $M_{\rm ns}$             \\ 
  \noalign{\smallskip}
\hline
  O310 & 400 & 0.848 & 31.7 & 50 & 18.1 & 3.094 & 3.684 & 
         2.613  & 0.0963 & 0.0688 & 1.59 & 70 & $ 1.12$ \\
  T310 & $400\times 192$ & 0.848 & 31.7 & 50 & 18.1 & 3.094  & 3.684 &
         2.613 & 0.0963 & 0.0688 & 1.77 & 62 &  $1.09$ \\
\hline
\end{tabular}
\end{table}