\begin{table}%t2
%\centering
\par
\caption{\label{solutions}Final ``best-fit'' values of the model parameters of the stars in the HD~5980 binary system for $i = 86^{\circ}$ and prior to the 1994 LBV~outburst.}
\small \begin{tabular}{l c c c}
\hline\hline
& Primary eclipse & \multicolumn{2}{c}{Secondary eclipse} \\
\cline{3-4}
& Ingress & \multicolumn{2}{c}{Ingress \& Egress} \\ 
\hline 
star A  &  \multicolumn{3}{c}{$\rho_1 = 0.158 \pm 0.005$} \\
&  & \multicolumn{2}{c}{$L_1 = 0.398 \pm 0.021$} \\
%\hline
star B  & \multicolumn{3}{c}{$\rho_3 = 0.108 \pm 0.003$}\\
        & \multicolumn{3}{c}{$\rho_2 = 0.269 \pm 0.014$}\\
        & $L_2 = 0.300 \pm 0.016$ & & \\
        & \multicolumn{3}{c}{$y = 0.19 \pm 0.02$} \\
& $u_2 = 0.58 \pm 0.07$ & \multicolumn{2}{c}{$v = 0.52 \pm 0.14$} \\
\hline
\end{tabular}
\end{table}