\begin{table}%t2
\caption{\label{tabfit}Parameter of the two-component wind model for the best fit of the \ion{C}{iv}~BALs in the selected quasar sample.}
%\centering
\par
\begin{tabular}{l r l r r r r l l l l l l}     
\hline\hline \noalign{\smallskip}
BAL QSO Name & $ z $ & $\tau_{\rm tot_p}$ & $k_{\rm pm}$ & ${v}_{\rm max}^{\rm po}$ ($\rm{km~s}^{-1}$) & ${v}_{\rm max}^{\rm eq}$ ($\rm{km~s}^{-1}$) & ${V}_{\rm rot}$ ($\rm{km~s}^{-1}$) & $\alpha$ & $\beta$ & $\Delta \theta$ ($\degr$) & $i$ ($\degr$) & $f_{\rm e}$ & $\gamma$\\
\hline
 Q1333+2840 & 1.897 & 3.00 & 10.0 & 13~000 & 4000 & 1000 & 3.0 & 0.8 & 10 & 80 & 0.21 & 1.0 \\
 Q1413+1143 & 2.522 & 10.0 & 15.0 & 11~000 & 3500 & 2000 & 3.0 & 0.8 & 10 & 88 & 0.16 & 1.0 \\
 Q0145+0416 & 1.990 & 1.00 & 12.0 & 18~000 & 9600 & 6400 & 2.5 & 1.2 & 15 & 80 & 0.18 & 1.0 \\
 Q0226-1024 & 2.164 & 1.00 & 10.0 & 25~000 & 12500 & 12500 & 2.0 & 1.5 & 15 & 87 & 0.10 & 1.0 \\
 Q0321-3344 & 1.955 & 10.0 & 10.0 & 10~000 & 7500 & 5200 & 2.5 & 1.5 & 15 & 75 & 0.16 & 1.0 \\
 Q0842+3431 & 2.100 & 14.0 & 5.00 & 16~000 & 10000 & 8000 & 3.0 & 1.5 & 15 & 78 & 0.04 & 1.0 \\
 Q1235+1453 & 2.835 & 5.00 & 10.0 & 13~000 & 8000 & 7000 & 2.5 & 1.5 & 15 & 76 & 0.12 & 1.0 \\
 Q1239+0995 & 1.970 & 3.00 & 5.00 & 16~000 & 8000 & 8000 & 3.0 & 1.0 & 15 & 82 & 0.10 & 1.0 \\
 Q0019+0107 M1 & 2.075 & 1.00 & 15.0 & 16~000 & 9000 & 8000 & 2.5 & 1.5 & 15 & 90 & 0.11 & 1.0 \\
 Q0019+0107 M2 & 2.075 & 0.00 & 15.0\tablefootmark{a} & -- & 9000 & 8000 & 2.5 & 1.5 & 15 & 90 & 0.11 & 1.0 \\
 Q0041-4023 M1 & 2.450 & 5.00 & 10.0 & 10~000 & 5000 & 3000 & 2.0 & 1.5 & 15 & 90 & 0.18 & 1.0 \\
 Q0041-4023 M2 & 2.450 & 15.0 & 5.0 & 6000 & 3000 & 3000 & 2.0 & 0.5 & 15 & 0 & 0.07 & 1.0 \\
\hline
\end{tabular}
\tablefoot {\tablefoottext{a}{$k_{\rm pm}$ represents the total equatorial ($i=90 \degr$) optical depth integrated over frequencies since $\tau_{\rm tot_p}=0$.}}
\end{table}