**Table 4:** Best-fit parameters from model solutions of the $\it JHK$ light-curves with 2 spots on the primary component and $\it BV,JHK$ (rectified) light-curves, corresponding to an effective temperature of the Primary component of 5200 K. The quoted uncertainties are formal mean standard errors to the solution.
$\begin{displaymath}{ \begin{tabular}{lcl@{$~\pm~$}r} \hline \hline Parameter & \... ... 0.0011 & \multicolumn{2}{c} {0.0006} \\ \hline \end{tabular}}\end{displaymath}$

Notes to table:
^a Dimensionless, Roche-lobe filling factor, defined as $Rochefil_{1,2} = R_{\rm pole1,2}/R_{\rm lobe1,2}$ .
^b Dimensionless, Roche potential at stellar surface (see Djurasevic 1992).

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