\begin{table}%t7
\caption{\label{linelist}Linelist of metal lines with astrophysical oscillator strengths.}
%\begin{center}
 %{%\centering
\small 
\begin{tabular}{llllcc}
\hline\hline \noalign{\smallskip}
Wavelength [$\AA$] &  $\chi_{\rm exc}$ [eV]  & $\log gf$ & $\Gamma_{\rm rad}$ [rad~s$^{-1}$] 
& van der Waal & Arcturus fit \\
\hline
 Si I  \\
 15330.191 & 6.718 & $-$1.90 & 1.00E+05 &    A   \\
 15338.780 & 6.261 & $-$2.58 & 1.00E+05 &    A   \\
 15342.973 & 7.108 & $-$1.85 & 1.00E+05 &    A   & * \\
 15361.160 & 5.954 & $-$2.12 & 1.00E+05 &    A   \\
 15375.430 & 6.734 & $-$1.53 & 1.00E+05 &    A   \\
 15376.830 & 6.223 & $-$0.66 & 1.00E+05 &    A   \\
 15376.830 & 6.721 & $-$1.13 & 1.00E+05 &    A   \\
 15381.738 & 6.721 & $-$2.03 & 1.00E+05 &    A   \\
 15387.069 & 7.166 & $-$1.64 & 1.00E+05 &    A   & * \\
 15471.964 & 6.726 & $-$2.40 & 1.00E+05 &    A   \\
 15496.964 & 7.006 & $-$2.54 & 1.00E+05 &  1.30  \\
 15506.980 & 6.727 & $-$1.55 & 1.00E+05 &    A   \\
 15520.115 & 7.108 & $-$1.85 & 1.00E+05 &    A   & * \\
 15532.449 & 6.718 & $-$2.18 & 1.00E+05 &    A   \\
 15538.463 & 6.761 & $-$2.36 & 1.00E+05 &    A   & * \\
 15557.790 & 5.964 & $-$0.65 & 1.00E+05 &    A   \\
 15561.251 & 7.040 & $-$1.23 & 1.00E+05 &    A   \\
 15638.472 & 6.734 & $-$1.93 & 1.00E+05 &    A   \\
 15674.653 & 7.064 & $-$1.30 & 1.00E+05 &    A   \\
 S I  \\
 15400.060 & 8.700 &  0.40 & 1.00E+05 &    A   \\
 15403.770 & 8.700 &  0.40 & 1.00E+05 &    A   \\
 15405.979 & 8.700 & $-$1.45 & 1.00E+05 &    A   \\
 15422.260 & 8.701 &  0.55 & 1.00E+05 &    A   \\
 15422.260 & 8.701 & $-$0.62 & 1.00E+05 &    A   \\
 15469.820 & 8.045 & $-$0.45 & 1.00E+05 &    A   \\
 15475.620 & 8.046 & $-$0.75 & 1.00E+05 &    A   \\
 15478.480 & 8.046 & $-$0.10 & 1.00E+05 &    A   \\
 Ti I  \\
 15334.840 & 1.887 & $-$1.05 & 2.93E+06 &    A   \\
 15381.110 & 2.333 & $-$2.29 & 7.13E+07 &    A   & * \\
 15399.285 & 2.334 & $-$2.00 & 7.13E+07 &    A   & * \\
 15426.970 & 1.873 & $-$2.52 & 2.76E+06 &    A   & * \\
 15543.780 & 1.879 & $-$1.15 & 2.76E+06 &    A   \\
 15602.840 & 2.267 & $-$1.60 & 2.31E+06 &    A   \\
 15698.979 & 1.887 & $-$2.14 & 2.76E+06 &    A   & * \\
 Cr I  \\
 15680.081 & 4.697 &  0.10 & 2.04E+08 &    A   \\
 Mn I  \\
 15673.385 & 5.133 & $-$0.57 & 6.68E+07 &    A   \\
 Fe I  \\
 15323.550 & 6.350 & $-$0.99 & 1.00E+05 &    A   \\
 15335.380 & 5.410 &  0.00 & 1.12E+08 &    A   \\
 15343.810 & 5.653 & $-$0.70 & 1.16E+08 &    A   \\
 15348.398 & 5.874 & $-$1.70 & 9.18E+07 &    A   \\
 15348.950 & 5.950 & $-$1.00 & 1.00E+05 &    A   \\
 15360.230 & 4.260 & $-$2.97 & 8.75E+06 &    A   \\
 15381.980 & 3.640 & $-$3.03 & 1.00E+05 &    A   \\
 15394.670 & 5.621 & $-$0.03 & 1.61E+08 &    A   \\
 15395.720 & 5.621 & $-$0.23 & 1.21E+08 &    A   \\
 15451.330 & 6.450 & $-$0.48 & 1.00E+05 &    A   \\
 15475.923 & 5.874 & $-$2.00 & 1.26E+08 &    A   \\
 15485.450 & 6.280 & $-$0.93 & 1.00E+05 &    A   \\
 15490.340 & 2.198 & $-$4.85 & 1.14E+04 &  1.40  \\
 15490.880 & 6.290 & $-$0.57 & 1.00E+05 &    A   \\
 15493.515 & 6.368 & $-$1.45 & 2.34E+08 &    A   \\
 15493.550 & 6.450 & $-$1.25 & 1.00E+05 &    A   \\
 15496.690 & 6.290 & $-$0.30 & 1.00E+05 &    A   \\
 15499.410 & 6.350 & $-$0.32 & 1.00E+05 &    A   \\
 15500.800 & 6.320 & $-$0.12 & 1.00E+05 &    A   \\
  15501.320 & 6.290 &  0.10 & 1.00E+05 &    A   \\
 15502.170 & 6.350 & $-$1.07 & 1.00E+05 &    A   \\
 15514.280 & 6.290 & $-$0.75 & 1.00E+05 &    A   \\
 15522.640 & 6.320 & $-$0.97 & 1.00E+05 &    A   \\
 15524.543 & 5.793 & $-$2.15 & 2.55E+08 &    A   \\
 15531.750 & 5.642 & $-$0.48 & 1.22E+08 &    A   \\
 15534.260 & 5.642 & $-$0.30 & 1.21E+08 &    A   \\
 15537.690 & 6.320 & $-$0.50 & 1.71E+08 &    A   \\
 15554.510 & 6.280 & $-$1.20 & 1.00E+05 &    A   \\
 15560.780 & 6.350 & $-$0.51 & 1.00E+05 &    A   \\
 15566.725 & 6.350 & $-$0.53 & 1.71E+08 &    A   \\
 15579.080 & 6.320 & $-$1.05 & 1.00E+05 &    A   \\
 15588.260 & 5.490 & $-$2.70 & 1.00E+05 &    A   \\
 15588.260 & 6.370 &  0.34 & 1.00E+05 &    A   \\
 15590.050 & 6.240 & $-$0.43 & 1.00E+05 &    A   \\
 15593.740 & 5.033 & $-$1.92 & 5.96E+08 &    A   \\
 15604.220 & 6.240 &  0.49 & 1.00E+05 &    A   \\
 15611.150 & 3.415 & $-$3.12 & 1.57E+07 &    A   \\
 15614.100 & 6.350 & $-$0.42 & 1.00E+05 &    A   \\
 15621.664 & 5.539 &  0.42 & 1.12E+08 &    A   \\
 15629.630 & 4.559 & $-$3.08 & 2.72E+08 &    A   \\
 15631.112 & 3.642 & $-$4.10 & 8.04E+07 &    A   \\
 15631.950 & 5.352 &  0.15 & 1.14E+08 &    A   \\
 15637.965 & 6.361 & $-$2.20 & 2.33E+08 &    A   \\
 15638.919 & 5.814 & $-$1.74 & 1.41E+08 &    A   \\
 15639.480 & 6.410 & $-$0.88 & 1.00E+05 &    A   \\
 15645.010 & 6.310 & $-$0.57 & 1.00E+05 &    A   \\
 15647.410 & 6.330 & $-$1.05 & 1.00E+05 &    A   \\
 15648.535 & 5.426 & $-$0.66 & 1.12E+08 &    A   \\
 15652.870 & 6.250 & $-$0.13 & 1.00E+05 &    A   \\
 15656.669 & 5.874 & $-$1.80 & 1.41E+08 &    A   \\
 15662.010 & 5.830 &  0.25 & 1.00E+05 &    A   \\
 15662.320 & 6.330 & $-$0.80 & 1.00E+05 &    A   \\
 15670.130 & 6.200 & $-$1.02 & 1.00E+05 &    A   \\
 15671.000 & 6.330 & $-$0.57 & 1.00E+05 &    A   \\
 15671.860 & 5.920 & $-$1.40 & 1.00E+05 &    A   \\
 15673.150 & 6.250 & $-$0.73 & 1.00E+05 &    A   \\
 15676.599 & 5.106 & $-$1.85 & 8.13E+07 &    A   \\
 15677.520 & 6.250 &  0.20 & 1.00E+05 &    A   \\
 15682.510 & 6.370 & $-$0.40 & 1.00E+05 &    A   \\
 15686.020 & 6.330 & $-$0.20 & 1.00E+05 &    A   \\
 15686.440 & 6.250 &  0.17 & 1.00E+05 &    A   \\
 15691.850 & 6.250 &  0.61 & 1.00E+05 &    A   \\
 15692.750 & 5.385 & $-$0.50 & 1.14E+08 &    A   \\
 Ni I  \\
 15555.370 & 5.488 &  0.13 & 1.48E+08 &    A   \\
 15556.016 & 5.283 & $-$3.15 & 1.68E+08 &    A   \\
 15605.680 & 5.300 & $-$0.47 & 1.00E+05 &    A   \\
 15605.680 & 5.300 & $-$0.96 & 1.00E+05 &    A   \\
 15632.654 & 5.305 & $-$0.01 & 9.71E+07 &    A   \\
\hline
\end{tabular}%\end{center}
\par
{See text: (1)~the wavelength in air. (2)~The excitation energy of the lower level. (3)~$\log gf$. (4)~The radiation damping parameter (when no
\noindent  value was available the very small value of $1.00$~$\times$ $10^5$ was used). (5)~The van~der~Waals damping marked with an~``A'' when calculated  according
to \citet{anstee}, \citet{barklem:00} and references therein, or Barklem~P., private communication (if~a number is instead given, this is an empirical correction factor to the van~der~Waals damping computed according to \citet{unsold}). (6)~A star~``*'' when the $\log gf$~value was determined from fits to the spectrum of Arcturus rather than from the Solar spectrum.}
\end{table}