\begin{table}%t7
\caption {\label{tablines}Abundance ratios derived and atomic parameters adopted.
}
%\centerline
 {\begin{tabular}{llllrrrrrrrrrrrrrrrrr}
\hline\hline
Species & ${\rm \lambda}$     & ${\rm \chi_{ex}}$ &  C$_6$ & log~$gf$ & \multispan8 [X/Fe]    \\
 \cline{6-13}  \\
   & (${\rm \AA}$) & (eV)  & (cm$^6$~s$^{-1}$) &  & {\bf B-8}  &   {\bf B-107} & {\bf B-108}   & {\bf B118} & {\bf B-122}
 &  {\bf B-128} & {\bf B-130} &  {\bf F-121} \\
\noalign{\smallskip} 
\hline
\noalign{\smallskip}
%                                                           8     107     108       118      122   128     130    121
OI & 6300.311 & 0.00 &0.30E-31 & --9.716                & +0.3: & --      & --     & --     & --    & --  & +0.5:& +0.5: \\ 
OI & 6363.79 & 0.00 &0.30E-31 & --10.25                 & +0.2: & +0.5:   & +0.7:  & +0.3: & +0.7: & --   & --   & +0.5: \\
%
NaI & 6154.230 & 2.10 & 0.90E-31 & --1.56            & +0.3  & --0.3:   &  0.0   & +0.1  & +0.1 & +0.1 & +0.1 & --0.1 \\
NaI & 6160.753 & 2.10 & 0.30E-31  &  --1.26          & +0.4  & --0.3:   & --0.2   & +0.1  & +0.2 & +0.1 & +0.2 & --0.1 \\
%
MgI & 6318.720 & 5.11 & 0.30E-31 & --2.10            & +0.1: & +0.20  & +0.4:  & +0.2   & +0.2 & +0.2 & +0.4 & +0.4 \\
MgI & 6319.242 & 5.11 & 0.30E-31  & --2.36           & +0.1: & --    & +0.2:  &  0.0   & +0.2 & +0.2 & +0.4 & +0.4 \\
MgI & 6319.490 & 5.11 & 0.30E-31   & --2.80          & +0.1: & +0.20  & +0.4:  & +0.2   & +0.2 & +0.4 & +0.4 & +0.4 \\
MgI & 6765.450 & 5.75 & 0.30E-31 &  --1.94           & --    & +0.40: & --    & --     &  -- & +0.2:& +0.4:& +0.4: \\
%
SiI & 6142.494 & 5.62 & 0.30E-31  & --1.50           & +0.2  & +0.2   & +0.4   & +0.2   &  0.0 & +0.2 & +0.4 & +0.2 \\
SiI & 6145.020 & 5.61 & 0.30E-31 & --1.45            & +0.4  & +0.2   & +0.2   & +0.2   & +0.2 & +0.2 &  --  & +0.2 \\
SiI & 6155.142 & 5.62 & 0.30E-30 & --0.85            & +0.2  & +0.1   &  0.0   & +0.2   & --0.1 & +0.2 & +0.3 & +0.2 \\
SiI & 6237.328 & 5.61 & 0.30E-30  &  --1.01          & +0.4  & +0.2   & +0.2   & +0.3   & +0.2 & +0.3 & +0.4 & +0.4 \\
SiI & 6243.823 & 5.61 & 0.30E-32  & --1.30           & +0.4  & +0.2   & +0.2   & +0.4   & +0.3 & +0.4 & +0.4 & +0.4 \\
SiI & 6414.987 & 5.87 & 0.30E-30   & --1.13          & +0.4: & +0.2   & +0.2   & +0.4   & +0.2 & +0.2 & +0.2 & +0.2 \\
SiI & 6721.844 & 5.86 & 0.90E-30 & --1.17            & +0.4  & +0.3   & +0.2   & +0.3   &  --  & +0.2: & +0.4:&  --  \\
%
CaI & 6156.030 & 2.52 & 4.0E-31  & --2.39 &  --   & +0.3   & +0.1  &  0.0   &  0.0 & +0.3 & --   &  0.0: \\
CaI & 6161.295 & 2.51 & 4.0E-31  & --1.02 & +0.2  &  0.0   & +0.3  &  0.0   & +0.3 & +0.2 & +0.3 & +0.3 \\
CaI & 6162.167 & 1.89 & 3.0E-31  & --0.09 &  0.0  & +0.2   &  0.0  & +0.2   &  0.0 &  0.0 & +0.1 & +0.3 \\
CaI & 6166.440 & 2.52 & 3.97E-31 & --0.90 &  0.0  &  0.0   & +0.2  & +0.2   & +0.3 &  0.0 & +0.3 & +0.3 \\
CaI & 6169.044 & 2.52 & 3.97E-31 & --0.54 & +0.3  & +0.1   & +0.1  & +0.2   & +0.3 & +0.3 & +0.1 & +0.3 \\
CaI & 6169.564 & 2.52 & 4.0E-31  & --0.27 & +0.1  & +0.2   & +0.1  & +0.3   & +0.3 & +0.3 & +0.2 & +0.3 \\
CaI & 6439.080 & 2.52 & 3.4E-32  & +0.3  &  0.0  & +0.3   & +0.3  & +0.3   & +0.3 & +0.3 & +0.3 &  0.0 \\
CaI & 6455.605 & 2.52 & 3.39E-32 & --1.35     & +0.3  &  0.0   & +0.3  & +0.3   & +0.3 & -0.1 & +0.4:& +0.3 \\
CaI & 6464.679 & 2.52 & 3.4E-32  & --2.10     & +0.3  &  0.0   & +0.3  & +0.3   & +0.3 & +0.3:&  --  & +0.3 \\
CaI & 6471.668 & 2.52 & 3.39E-32 & --0.59     & +0.3  &  0.0   & +0.3  & +0.3   & +0.3 & +0.3 & +0.3 & +0.3 \\
%
CaI & 6493.788 & 2.52 & 3.37E-32    & 0.0    & +0.1  & --0.3   &  0.0  & +0.2   &  0.0 &  0.0 & +0.1 & --0.2 \\
CaI & 6499.654 & 2.52 & 3.37E-32    & --0.85  & +0.2  & --0.3   & +0.2  &  0.0   &  0.0 &  0.0 & +0.1 & -0.1 \\
CaI & 6572.779 & 0.00 & 1.75E-32    & --4.32  & +0.1  &  0.0   & +0.3  & +0.3   & +0.2 &  0.0 & +0.2 &  0.0 \\
CaI & 6717.687 & 2.71 & 4.1E-31     & --0.61  &  0.0  &  0.0   &  0.0  & +0.3   & +0.3 & +0.3 & +0.3 & +0.1\\
%
TiI & 6126.224 & 1.07 & 1.37E-32    & --1.43  & +0.2  & +0.2   & +0.2  &  0.0   & +0.1 & +0.1 & +0.2 &  0.0 \\
TiI & 6258.110 & 1.44 & 3.17E-32    & --0.36  &  0.0  &  0.0   & +0.2  &  0.0   & +0.2 & +0.2 &  0.0 & +0.1 \\
TiI & 6261.106 & 1.43 & 4.68E-32     & --0.48  &  0.0  &  0.0   &  0.0  &  0.0   & +0.3 &  0.0 &  0.0 & +0.2 \\
TiI & 6303.767 & 1.44 & 3.12E-32    & --1.57  &  0.0: &  0.0   &  --   & +0.2   & +0.2:& +0.2:  &  --  & --   \\
TiI & 6336.113 & 1.44 & 1.86E-32    & --1.74  &  --   &  --    & +0.2: & +0.3   & +0.3 &  0.0: &  --  & +0.3: \\
TiI & 6554.238 & 1.44 & 1.81E-32    & --1.22  & +0.2  & +0.2   & +0.2  &  0.0   & +0.2 & +0.2 &  0.0 & +0.2 \\
TiI & 6556.077 & 1.46 & 1.81E-32    & --1.07  &  0.0  & +0.2   & +0.3  &  0.0   &  0.0 & +0.2 & +0.4 & +0.2 \\
TiI & 6599.113 & 0.90 & 1.96E-32    & --2.09  & +0.2: & +0.3   & +0.2: & +0.3   & +0.2 & +0.2::& +0.4: & +0.1 \\
TiI & 6743.127 & 0.90 & 0.30E-31               & --1.73  &  0.0  & +0.1   & +0.2  & --0.2   &  0.0 &  0.0 & +0.2 & +0.2 \\
TiII& 6491.580 & 2.06 & 0.30E-31               & --2.10  & +0.2  & +0.3   & +0.3  & +0.3   & +0.3 & +0.3 & +0.3 & +0.1 \\
TiII& 6559.576 & 2.05 & 0.30E-31               & --2.35  & +0.3  &  0.0   & +0.3  & +0.3   & +0.3 & +0.3 & +0.3 & +0.2 \\
TiII& 6606.970 & 2.06 & 0.30E-31               & --2.85  & +0.2  & +0.2:  & +0.2  & --     & --   & +0.3:& +0.3 & +0.2 \\
%
BaII & 6141.727 & 0.70 & & --0.07$^a$                          & +1.0 & +0.5   & --0.1  & +0.75   & +0.5 & +1.0 & +0.25 &  --0.25  \\
BaII & 6496.908 & 0.60 & & --0.38$^b$                          & +0.9 & +0.5   & +0.15  & +1.2   & +0.75 & +0.75 & +0.25 &  --0.25 \\
LaII & 6390.480 & 0.32 & & --1.41$^c$                      & +0.5 & +0.50   & +0.3  & +0.5   & +0.3:&  --  & --   &  0.0:\\
EuII & 6645.127 & 1.38 & & 0.12$^a$                      & +0.5 & 0.0:  &  +0.5:  & +0.5   & +0.3:&  0.0: & +0.8 & +0.5 \\
 \hline 
\end{tabular}}
\smallskip
Column~5 reports the log gf adopted  as described in Barbuy et~al. (2007).
For the heavy elements~BaII, LaII and EuII, hyperfine structure was taken into account,
and the log gf values reported correspond to the equivalent total $\log gf$, adopted
from a Hill et~al. (2002), b Rutten (1978), c~Lawler et~al. (2001b).
\end{table}