\begin{table}%t5
%\centering
\par
\caption{MORO solutions of the light curve of the eclipsing system
         2MASS J0516288+260738.\label{SOLUTION}}
\begin{tabular}{lllllllll}
\hline\hline\noalign{\smallskip}
Parameter       & a & b & c & d & e & f & g & h     \\[1mm]
\hline\noalign{\smallskip}
$q~(=M_2/M_1)$
                & 0.085 & 0.094 & 0.110 & 0.122 & 0.156 & 0.181 & 0.182 & 0.184          \\
$i$
                & $75\fdg5$ & $74\fdg3$ & $74\fdg0$ & $73\fdg9$
                & $73\fdg5$ & $72\fdg4$ & $72\fdg9$ & $72\fdg3$                                  \\
$T_1/T_2$
                & 1.67 & 1.72 & 1.74 & 1.73 & 1.77 & 1.63 & 1.83 & 1.88                  \\
$r_1/r_2^{~a}$
                & 1.11 & 0.89 & 0.85 & 0.87 & 0.85 & 0.67 & 0.73 & 0.64                  \\
$\Omega_1$
                & 5.138 & 5.350 & 5.510 & 5.520 & 5.598 & 6.123 & 6.001 & 6.220          \\
$\Omega_2$
                & 1.961 & 1.943 & 1.997 & 2.055 & 2.182 & 2.197 & 2.236 & 2.198          \\
$L_1^{b}$
                & 0.998 & 0.998 & 0.999 & 0.998 & 0.999 & 0.993 & 0.999 & 0.999          \\
$x_1^{c}$
                & 0.60$^{*}$   & 0.60$^{*}$   & 0.50$^{*}$   & 0.50$^{*}$
                & 0.60$^{*}$   & 0.60$^{*}$   & 0.488        & 0.60$^{*}$                \\
$x_2^{~c}$
                & 0.50$^{*}$   & 0.50$^{*}$   & 0.50$^{*}$   & 0.50$^{*}$
                & 0.50$^{*}$   & 0.50$^{*}$   & 0.527        & 0.50$^{*}$                \\
$l_3^{d}$
                & 0\%$^{*}$  & 0\%$^{*}$  & 0\%$^{*}$  & 0\%$^{*}$
                & 0\%$^{*}$  & 0\%$^{*}$  & 1.5\%      & 0\%$^{*}$	   \\[1mm]
\hline\noalign{\smallskip}
$1\sigma$ deviation
                &0.00750&0.00750&0.00749&0.00749&0.00749&0.00755&0.00750&0.00749\\%[1mm]
\hline\noalign{\smallskip}
%\end{tabular}
%\noalign{\smallskip}
%$^{a}$ {Ratio of mean Roche radii.}\\
%$^{b}$ {Relative luminosity $L_1/(L_1 + L_2)$; $L_2$ is not
%    independently adjusted, but recomputed from $r_2$ and $T_2$}.\\
%$^{c}$ {Linear limb darkening coefficient; theoretical
%                                 value for $V$ band taken from \citet{1995A&AS..110..329D}.}\\
%$^{d}$ {Fraction of third light at maximum.}\\
%$^{*}$ {Fixed.}
%\end{table}