\begin{table}%t1
   %\centering
\par
      \caption{Parameters used for the library of template SEDs.\label{tabBC}}
     $$ 
         \begin{array}{p{0.3\linewidth}l}
            \hline\hline
            \noalign{\smallskip}
            IMF & Salpeter\\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
            SFR $\tau$ (Gyr) & 0.1,0.3,0.6,1,1.5,2,3,4,5,7,9,13,15\\
%
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
            log~(age) (yr) & 7,7.02,7.04...10.2^{b}\\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
            Metallicities & 0.02~Z_{\odot}, 0.2~Z_{\odot}, Z_{\odot}, 2.5~Z_{\odot}^{c} \\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
            $E_{B-V}$ & 0,0.03,0.06,0.1,0.15,0.2,...,1.0\\
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
            Extinction law & SMC  \\
            \noalign{\smallskip}
            \hline
          \end{array}
     $$ 
\begin{list}{}{}
\par
\item[$^{{a}}$] At each $z$, galaxies are forced to have ages lower than the Hubble time at that $z$.
\item[$^{{b}}$] Models with metallicity~=~$0.02~Z_{\odot}$ have been limited 
to log~(age)~$\leq 9$; models with metallicity~=~$2.5~Z_{\odot}$ have been limited 
to log~(age)~$\geq 9$. 
\end{list}
   \end{table}