\begin{table}%t2
      %\centering
\par
      \caption {\label{tab:solution}Spectroscopic orbital solutions based on 
          fitting the 
          radial velocities obtained using different
          data fitting methods, explained in Sect.~\ref{sec:rvs}. }
\par
        \begin{tabular}{lrrrrrrrrr}
          \hline\hline
          & LSD+GAU & LSD+MM & IRAF$_{\rm full}$ & IRAF 
          & KOREL & I09 \\%& All\\
\hline
\par
          $e$      &0.27 (0.02)  &0.28 (0.04)  &0.27 (0.08)  
          &0.27 (0.05)  &0.29 (0.01)  & 0.25 (0.04) \\%& 0.29 (0.02) \\
          $\Omega$ ($^{\circ}$) &83.6 (2.0)   &78.6 (4.9)   &80.5 (9.9) 
          &81.1 (6.0)   &76.8 (5.0) & 46.7 (7.6)  \\% & 79.8 (3.1)  \\
          $T_0$ (days)    &--0.07 (0.05) &--0.06 (0.17) &--0.07 (0.41) 
          &--0.12 (0.22) &-0.1 (0.2) & --0.44 (0.27) \\% & --0.1 (0.1) \\
          $\gamma$ (\kms)&--28.1 (0.4) &--30.0 (1.5) &--29.2 (2.8) 
          &--29.2 (1.7) & --  & --27.8 (2.3)\\%&--28.7 (0.9) \\
          $K_A$ (\kms)   & 88.2 (0.9) &84.3 (2.7)    &84.3  (5.1) 
          &91.9 (3.2)  &87.3 (3.5)  & 85.5 (3.9)  \\% & 89.7 (1.7)  \\
          $K_B$ (\kms)   & 94.6 (1.1) &90.7 (2.8) &91.2 (5.6) 
          &100.5 (3.8)&93.0 (4.0) & 95.9 (4.5) \\%   & 95.9 (1.75)   \\
          $M_A\sin^3 i$ (\msol) & 1.67 (0.12) &1.45 (0.11) &1.48 (0.23) 
          &1.96 (0.19) &1.58 (0.15) &1.69 (0.18)\\%& 1.71 (0.08)\\
          $M_B \sin^3 i$ (\msol)&1.55  (0.11) &1.35 (0.11) &1.37 (0.21) 
          & 1.79 (0.16) &1.48 (0.13) &1.51 (0.16) \\%&1.60 (0.07)\\
          $\chi^2_R$ &  2.7   &  & 0.04 & 0.07& 0.86 &0.7\\%&0.4 \\
          \hline
        \end{tabular}
\smallskip
    \end{table}