\begin{table}%t1
\caption{\label{table:1}Best fit parameters of the SED at different epochs.}      
%\centering
\par
\begin{tabular}{cc cc c}   
\hline\hline  \noalign{\smallskip}                      
Days & Model & $\beta$ & $A(3000~\AA)$ & $A_V$\tablefootmark{a} 
\\
 &&&(mag) & (mag)\\ 
\hline
0.47 & PL & $1.28 \pm 0.11$ & \mbox{\ldots} &  \mbox{\ldots} \\
		& PL+SN & $1.22 \pm 0.24$ & $0.3\pm0.22$ & \mbox{\ldots} \\
		& PL+SMC & $1.23 \pm 0.08$ &  $0.1 \pm 0.07$ & $0.05 \pm 0.04$ \\ 
\hline
1.25 & PL & $1.24 \pm 0.09$ &  \mbox{\ldots} &  \mbox{\ldots} \\
		& PL+SN & $1.27 \pm 0.2$ & $0.05\pm 0.11$ &  \mbox{\ldots} \\
		& PL+SMC & $1.17 \pm 0.51$ & $0.01 \pm 0.04$ & $0.01 \pm 0.02$ \\ 
\hline
3.4 & PL & $1.25 \pm 0.05$ &  \mbox{\ldots} &  \mbox{\ldots} \\
		& PL+SN & $1.23 \pm 0.21$ & $0.22 \pm 0.24$ & \mbox{\ldots} \\
		& PL+SMC & $1.24 \pm 0.07$ & $0.056 \pm 0.059$ & $0.042 \pm 0.044$ \\ 
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{The SN-origin extinction curve has been only computed in the range $\lambda_{\rm{rest}}=1000-4000~\AA$, hence it is not possible to provide~$A_V$.}}
\end{table}