\begin{table}%t2
\par
%\centering
\par
\caption{Synthesized Mass ($M_\odot$) for radioactive species in SN~Ia models.\label{tab2}}
\begin{tabular}{ccccccc}
\hline\hline
 Species & W7$^{(\rm a)}$ & {\it c3\_2d\_512}$^{(\rm b)}$ & {\it c3\_3d\_256}$^{(\rm b)}$ &
{\it c3\_3d\_256}$^{(\rm c)}$ & {\it b5\_3d\_256}$^{(\rm c)}$ & {\it b30\_3d\_768}$^{(\rm
c)}$ \\ \hline
\par
$^{22}$Na & 1.73E-08  & 5.76E-08 & 9.42E-08 & 8.94E-08 & 8.00E-07 & 1.00E-07 \\
$^{26}$Al & 4.93E-07  & 5.98E-07 & 9.82E-07 & 9.11E-07 & 4.53E-05 & 4.47E-06 \\
$^{36}$Cl & 2.58E-06  & 5.56E-07 & 7.62E-07 & 9.73E-07 & 1.99E-06 & 6.32E-07 \\
$^{39}$Ar & 1.20E-08  & 1.68E-09 & 2.34E-09 & 3.24E-09 & 9.41E-09 & 2.24E-09 \\
$^{40}$K  & 8.44E-08  & 7.77E-09 & 1.10E-08 & 1.73E-08 & 4.10E-08 & 1.23E-08 \\
$^{41}$Ca & 6.09E-06  & 9.01E-07 & 1.17E-06 & 2.20E-06 & 6.02E-06 & 2.40E-06 \\
$^{44}$Ti & 7.94E-06  & 1.80E-06 & 2.80E-06 & 3.09E-06 & 4.50E-06 & 3.61E-06 \\
$^{48}$V  & 4.95E-08  & 4.10E-05 & 6.95E-05 & 7.27E-05 & 1.32E-04 & 7.68E-05 \\
$^{49}$V  & 1.52E-07  & 3.28E-06 & 5.22E-06 & 5.62E-06 & 1.10E-05 & 5.78E-06 \\
$^{53}$Mn & 2.77E-04  & 4.77E-04 & 5.16E-04 & 4.78E-04 & 5.09E-04 & 4.79E-04 \\
$^{60}$Fe & 7.52E-07  & 1.44E-14 & 6.57E-12 & 6.57E-12 & 8.54E-13 & 4.52E-10 \\
$^{56}$Co & 1.44E-04  & 9.50E-05 & 1.04E-04 & 9.81E-05 & 1.69E-04 & 1.32E-04 \\
$^{57}$Co & 1.48E-03  & 1.33E-03 & 1.38E-03 & 1.16E-03 & 6.35E-04 & 1.15E-03 \\
$^{60}$Co & 4.22E-07  & 4.00E-10 & 6.82E-09 & 6.77E-09 & 1.12E-09 & 2.66E-08 \\
$^{56}$Ni & 5.86E-01  & 2.16E-01 & 2.95E-01 & 3.08E-01 & 3.27E-01 & 4.18E-01 \\
$^{57}$Ni & 2.27E-02  & 9.17E-03 & 1.21E-02 & 1.25E-02 & 1.22E-02 & 1.74E-02 \\
$^{59}$Ni & 6.71E-04  & 6.62E-04 & 7.40E-04 & 6.60E-04 & 4.47E-04 & 7.11E-04 \\
$^{63}$Ni & 8.00E-07  & 4.15E-11 & 2.10E-09 & 2.10E-09 & 1.98E-10 & 2.22E-08 \\
\hline
\end{tabular}
\smallskip
\begin{list}{}{}
\item[$^{{\rm a}}$] Iwamoto et~al.~(\cite{Iwamoto99}).
\item[$^{{\rm b}}$] This work.
\item[$^{{\rm c}}$] This work. In this run we allow the nucleosynthesis calculations 
for those tracer particles that reach NSE conditions only starting at~90\% of the temperature
peak.
\par
\end{list}
\par
%}
\end{table}