\begin{table}%t5 
\par
\caption {\label{ssc-fit-1}SSC best fit results for  2005 March 31~\swf~ observation and using a  log-parabolic electron
distribution as defined in Eq.~(\ref{eq-lpep-elec}).}
%%\centerline

 {\begin{tabular}{llllllllll}
\hline\hline
\noalign{\smallskip}
 Date   &$B$   &$R$   &$\delta$  &$N(*)$       &$r$ &$\gamma_{p}(**)$  &$\gamma_{\rm max}$
&$\gamma_{\rm min}$ &$u_e{}/u_{b}$\\ 
        &G   &cm  &          &$\mbox{cm}^{-3}$ &    &              &\\ 
\hline
31-03-2005  &$0.075$ &$1.5\times10^{15}$ &25 &4   &1.3
&$4.0\times10^{3}$&$2.5\times10^{6}$&$1.1\times10^{3}$& 220\\
\hline
\noalign{\smallskip} 
\end{tabular}
}
\par
 \smallskip
(*)  $N=\int n(\gamma)\rm d\gamma$.\\
(**) Do not confuse $\gamma_{c}$ (the turn-over energy in Eq.~(\ref{lppl-elec}))  with 
$\gamma_{\rm p}$  (the peak energy in Eq.~(\ref{eq-lpep-elec})).\\
(***) $\gamma_{\rm p}^{\rm LP}$ represents $\gamma_{\rm p}$ obtained from extrapolating the log-parabolic branch of the
distribution described by Eq.~(\ref{lppl-elec}). These values can be compared with $\gamma_{\rm p}$ from 2005 March~31.
\end{table}