Table 7:

Linelist of metal lines with astrophysical oscillator strengths.

Wavelength []	[eV]		[rad s-1]	van der Waal	Arcturus fit
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

See text: (1) the wavelength in air. (2) The excitation energy of the lower level. (3) . (4) The radiation damping parameter (when no value was available the very small value of 1.00  10⁵ was used). (5) The van der Waals damping marked with an ``A'' when calculated according to Anstee & O'Mara (1995), Barklem et al. (2000) 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 Unsöld (1955)). (6) A star ``*'' when the  value was determined from fits to the spectrum of Arcturus rather than from the Solar spectrum.