\begin{table}%t3
%\centering
\par
\caption{\label{table:3}Summary of GW related quantities\tablefootmark{a}.} 
\begin{tabular}{ccrcrrrrrr}
\hline\hline \noalign{\smallskip}
Model & $t_{f}$[ms]
&$E_{GW} [M_{\odot}c^2]$ & Dir. & $|A_{+,b,\max}|$ & $|A_{\times,b,\max}|$ & 
$|A_{+,pb,\max}|$ & $|A_{\times,pb,\max}|$& $f_{b} [{\rm Hz}]$ & $f_{TW}$[Hz]  \\
\hline
\multirow{2}{*}{R0E1CA}& \multirow{2}{*}{130.8} & \multirow{2}{*}{$2.15\times10^{-11}$}  & I  &  3  &  $<$1 &$3$ & $<$1  & -- & --  \\
          &                 &    & II &  2  &  $<$1    & 5    & $1$ & --& -- \\
%\hline
\multirow{2}{*}{R0E3CA}& \multirow{2}{*}{103.9} & \multirow{2}{*}{$5.72\times10^{-11}$}   & I  & 2   &   $<$1    & 10  & $<$1 & -- &--  \\
          &                &     & II & 2   &   $<$1    & 8 & $<$1 & --& -- \\
%\hline
\multirow{2}{*}{R0STCA} & \multirow{2}{*}{70.3} & \multirow{2}{*}{$1.35\times10^{-11}$} & I  & 3 &$<$1 & 4 &$<$1 & -- & --   \\
         &                  &         & II  & 1 & $<$1  & 3 & $<$1 &--&--\\
%\hline 
\multirow{2}{*}{R1E1CA}& \multirow{2}{*}{112.8} & \multirow{2}{*}{$1.36\times10^{-10}$}  & I  & 3   & $<$1  & 12 & 6 & -- & -- \\
& & & II &  3   & $<$1 & 15  & 1 & -- & --  \\
%\hline
\multirow{2}{*}{R1E3CA}& \multirow{2}{*}{130.4}  &  \multirow{2}{*}{$1.43\times10^{-10}$} & I  & 2   &  $<$1  & 10  & 5 & -- & --\\
&&  & II & 3   & $<$1   & 17 & $<$1& -- & --\\
%\hline
\multirow{2}{*}{R1E1DB}& \multirow{2}{*}{112.8}  & \multirow{2}{*}{$1.24\times10^{-10}$}    & I  &  3  & $<$1 &  12 & 6 & -- &--\\
          &             &        & II &  3  & $<$1 & 15 & 2 & -- & --  \\
%\hline
\multirow{2}{*}{R1STCA}& \multirow{2}{*}{45.8}    &\multirow{2}{*}{$2.01\times10^{-11}$}    & I  &  2  &  $ <$1   &  3 &1  & --  & --\\
          &             &        & II &  2  & $<$1 & 6 &$<$1  & -- &-- \\
%\hline
\multirow{2}{*}{R1E1CA$_{L}$} & \multirow{2}{*}{92.9}  & \multirow{2}{*}{$1.04\times10^{-10}$}  & I  & 3 & $<$1  &4 & 2 & -- & -- \\
          &            &         & II & 2 &$<$1 &  10 & 1 & -- & --\\
%\hline
\multirow{2}{*}{R2E1AC} & \multirow{2}{*}{127.3} & \multirow{2}{*}{$5.52\times10^{-9}$} & I  &  2  &  2    & 6 &5 & --& --\\
& & & II & 105 & $<$1  & 1  &3 & 841 & -- \\
%\hline
\multirow{2}{*}{R2E3AC} & \multirow{2}{*}{106.4}    &  \multirow{2}{*}{$5.31\times10^{-9}$} & I  &  2  &  2    & 4  & 4 & -- & -- \\
          &             &         & II & 104 & $<$1  &  1 &$<$1 & 803 & -- \\
%\hline
\multirow{2}{*}{R2STAC} &  \multirow{2}{*}{64.0}     &  \multirow{2}{*}{$7.62\times10^{-9}$}     & I  &  3  &  3   & 6 &6 & -- & --  \\
          &             &         & II & 133  & $<$1  & 2   & 1& 680 & -- \\
%\hline
\multirow{2}{*}{R3E1AC} & \multirow{2}{*}{62.5}    & \multirow{2}{*}{$5.58\times10^{-8}$}        & I  &  2   &  1   &  15 & 16 & -- &725\\ 
&   &  & II &  393 & $<$1 &  10 & 2 & 880 & -- \\
%\hline
\multirow{2}{*}{R3E2AC} & \multirow{2}{*}{45.5}    &  \multirow{2}{*}{$6.53\times10^{-8}$} & I &   2  &    1 &  11  & 13 &-- &     \\
&            &         & II&  409 &   $<$1&  5  &   3  & 882 & -- \\
%\hline
\multirow{2}{*}{R3E3AC} & \multirow{2}{*}{57.5}    &  \multirow{2}{*}{$6.44\times10^{-8}$}       & I &  2   &    2  &   6    & 9  &-- &  \\
&            &         & II&  409 &   $<$1&   6    & 3 & 891 & -- \\   
%\hline
\multirow{2}{*}{R3STAC}  & \multirow{2}{*}{50.2} & \multirow{2}{*}{$1.05\times10^{-7}$} & I   &  5    &   4   &  9  & 11  &-- & 935  \\
&  & & II  &  526  &  $<$1 &   5 &  3 & 854 & -- \\
%\hline
\multirow{2}{*}{R3E1CA}  & \multirow{2}{*}{69.4} & \multirow{2}{*}{$8.05\times10^{-8}$} & I  &  3  &  3   & 9  & 9 &--&--\\
  &     &  & II &  426  & $<$1 &5 &3 &897 & --\\
%\hline
\multirow{2}{*}{R3E1DB}  & \multirow{2}{*}{62.7}  &  \multirow{2}{*}{$7.76\times10^{-8}$} & I  &  8  &   8   & 13 & 11 & -- &-- \\
&  & & II &  425  & $<$1&8 & 3 & 886& --\\
%\hline
\multirow{2}{*}{R3E1AC$_{L}$} & \multirow{2}{*}{196.7}  & \multirow{2}{*}{$2.14\times10^{-7}$}  & I  & 1 & 1  & 136  & 136  & -- & 909 \\
&       &              & II & 437   &$<$1  & 70 & 9 & 909& --  \\
%\hline
\multirow{2}{*}{R4E1AC}& \multirow{2}{*}{98.7}    & \multirow{2}{*}{$7.74\times10^{-8}$}   & I  &  1   &  $<$1   & 37  & 37 & --& 662 \\
          &         &                           & II & 512  &  $<$1  &20 & 6 &385 & -- \\
%\hline
\multirow{2}{*}{R4STAC} &  \multirow{2}{*}{67.2}   & \multirow{2}{*}{$1.91\times10^{-7}$}   & I  & 2    &  1  & 102 & 109 & --&  902\\
&        &            & II &  536   & $<$1    & 53 & 3 & 396 & -- \\
%\hline
\multirow{2}{*}{R4E1EC}& \multirow{2}{*}{100.8}    &  \multirow{2}{*}{$7.51\times10^{-8}$}  & I  & 1   &  1    & 25  & 20 & --  &611\\
&      &               & II &  492  & $<$1 & 15 & 7 & 866 &  \\
%\hline
\multirow{2}{*}{R4E1FC}& \multirow{2}{*}{80.1}    & \multirow{2}{*}{$7.29\times10^{-8}$} & I  &  $<$1    &  $<$1   & 16  & 19 & -- & 828\\
          &        &             & II &  516  & $<$1 & 9 & 3 & 859 & -- \\
%\hline
\multirow{2}{*}{R4E1FC$_{L}$}    & \multirow{2}{*}{97.6} & \multirow{2}{*}{$3.42\times10^{-7}$}   & I  &  2  &  1   & 316  & 298 &  -- &673 \\
&        &             & II & 536 & $<$1 & 157 & 6 & 485 & -- \\
%\hline
\multirow{2}{*}{R4E1CF}    & \multirow{2}{*}{19.1} & \multirow{2}{*}{$6.50\times10^{-8}$}   & I  &    1&   1  & 4 &4 & -- & \\
   &        &             & II & 518 & $<$1 & ring-down & 2 & 370 & -- \\
%\hline
\multirow{2}{*}{R5E1AC} & \multirow{2}{*}{93.2}   & \multirow{2}{*}{$1.20\times10^{-8}$}   & I  &  1 &  1  &  18 & 18 &--& 727 \\
          &          &           & II &  238   & $<$1 & 10 & 11 & 317 &-- \\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{$t_{f}$ is the time after core bounce when the 
simulation was stopped. $E_{GW}$ is the total energy released in gravitational radiation.  We present the maximum amplitudes at different stages of 
their time-evolution in polar (I)~and equatorial (II)~direction. 
The subscripts $b$ and $pb$ stand for bounce and postbounce. $f_{b}$ denotes the peak frequency of the GW burst at bounce,  while $f_{TW}$ stands for the spectral peak from the  narrow band emission caused by a low $T/|W|$ instability. The electronic wave forms of all models are available upon request.}}
\vspace*{2mm}
\end{table}