\begin{table}%[t]%t2
%\centering
\par
\caption{\label{t2}Final parameters resulting from  the best $\chi_{\rm red}^2$ fit
to the NIR flare observed on 30 july 2005.}
\begin{tabular}{lccccccccccr}\hline \hline\noalign{\smallskip}
Model  &  $a$  & $\eta$ & $\psi$ & $r_0$ & $r_{\rm spot}$ & $R$  & $\Pi_{\rm L}$ & $i$ & $\Theta$ & $\chi^2_{\rm red}\pm1$ \\
       &        & [deg]  & [deg]  &  $[r_{\rm g}]$ & $[r_{\rm mso}]$  &  & [\%] & [deg] &  [deg] &  &  \\
\hline \noalign{\smallskip}
 I     & 0.5   &   $90$  &  $90$ &  4 & 1.1 & 5 & $50\pm10$ & $60\pm15$ & $15\pm20$ & $1.63\pm1$ \\
 II    & 0.5   &   $0$  &  $0$ &  4 & 1.1 & 5  & $50\pm10$ & $65\pm10$ & $110\pm15$ & $2.95\pm1$\\
III    & 0.5   &   $78.56\pm12$  &  $72\pm18$ &  4 & 1.1 & 5 & $60\pm10$ & $50\pm20$ & $30$ & $1.54\pm1$\\
\hline 
\end{tabular}
\vspace*{9mm}\end{table}