\begin{table}%t5
\caption{Solar thorium abundance derived from line profile fitting.
\label{sunth_lf}}
\small%\centerline
{
\begin{tabular}{lrrrrrrr}
\hline\hline
                  & \multicolumn{3}{c}{3D} & \multicolumn{3}{c}{LHD}\\
                  & $A$(Th) & Shift & $V_{\rm br}$& $A$(Th) & SHIFT & $V_{\rm br}$ & 3D-\xx\ \\
                  & dex   & \kms  & \kms    & dex   & \kms  & \kms   & dex \\ 
\hline
Int. (Neckel)      & 0.088 & --0.05 & 1.49    & 0.160 & --0.53 & 2.77 & --0.072  \\ 
Int. (Delbouille)  & 0.080 & +0.01 & 1.86    & 0.168 & --0.47 & 2.99  & --0.088  \\
Flux (Neckel)      & 0.056 & --0.39 & 1.68    & 0.168 & --0.47 & 4.11 & --0.112  \\
Flux (Kurucz)      & 0.067 & --0.38 & 2.82    & 0.175 & --0.46 & 4.71 & --0.108 \\
\noalign{\smallskip}
\hline
\end{tabular}
}
\smallskip
Note:
(2)$-$(4)  results of the fitting: $A$(Th), shift, and
broadening using a 3D~grid;
(5)$-$(7) same for \xx\ grid; 
(8) gives the difference in abundance $A$(Th)$_{\rm 3D}-$$A$(Th)$_{\rm\xx}$.
\end{table}