&                                                  \\
{\rm A_{bs}=T_{bs}/T_d}            & 1.37  \pm 0.04  &                                                   && {\rm A_{bs}=T_{bs}/T_d}           & 1.08  \pm 0.03  &                                                  \\
{\rm \theta_{bs}}{\rm [^{\circ}]}  & 47.2  \pm 8.0   &                                                   && {\rm \theta_{bs}}{\rm [^{\circ}]} & 21.9  \pm 3.0   &                                                  \\
{\rm \lambda_{bs}}{\rm [^{\circ}]} & 66.2  \pm 9.0   &                                                   && {\rm \lambda_{bs}}{\rm [^{\circ}]}& 125.4 \pm 9.0   &                                                  \\
{\Omega_{\rm h}}                   & 17.848\pm 0.02  &                                                   && {\Omega_{\rm h}}                  &17.838 \pm 0.03  &                                                  \\
{\Omega_{\rm c}}                   & 2.282 \pm 0.02  &                                                   && {\Omega_{\rm c}}                  & 2.282 \pm 0.02  &                                                  \\
            \noalign{\smallskip}
            \hline
         \end{array}$$

FIXED PARAMETERS: $q={\cal M}_{\rm c}/{\cal M}_{\rm
h}=0.22$ - mass ratio of the components, ${\rm T_c=4400 K}$ - temperature of the less massive (cooler) donor, ${\rm F_c}=1.0$ - filling factor for the critical Roche lobe of the donor, $f{\rm _{c}}=1.00$ - non-synchronous rotation coefficients of the donor, ${\rm F_h}=R_h/R_{zc}$ - filling factor for the critical non-synchronous lobe of the hotter, more massive gainer (ratio of the stellar polar radius to the critical Roche lobe radius along z-axis for a star in critical non-synchronous rotation regime), ${\rm \beta_h=0.25}$, ${\rm \beta_c=0.08}$ - gravity-darkening coefficients of the components, ${\rm A_h=1.0}$, ${\rm A_c=0.5}$ - albedo coefficients of the components. NOTE: $n$ - number of observations, ${\rm
\Sigma (O-C)^2}$ - 