Table 5:
List of lines used in the abundance analysis, with references to the oscillator strengths used. The columns Waals. , Stark. , and Rad. list the van der Waals, Stark, and radiative damping data (for a description of the data sources, see Barklem et al. 2005, Sect. 3.2, paragraph 5). Rad. is the logarithm (base 10) of the FWHM given in
.
Non-zero values of Stark. and negative values of Waals. represent the logarithm of FWHM per unit pertuber number density at 10 000 K, given in
.
Positive values of the van der Waals parameter correspond to the notation of Anstee & O'Mara (1995), where a packed parameter is used for the broadening cross-section (
)
for collisions by neutral hydrogen at 10 km s-1 and its velocity dependence (
). E.g. for the Mg I 5172.684 Å line, Waals. =729.238 means
in atomic units and
.
d
and d
give the extent of the spectral windows used for fitting of each line, blue-wards and red-wards of the central wavelength. Zero values in both columns indicate that the line-contribution is considered in the same window as the one listed directly above.
Ion |
[Å] |
[eV] |
 |
Ref. |
Waals. |
Stark. |
Rad. |
d
[mÅ] |
d
[mÅ] |
Mg I |
5172.684 |
2.712 |
-0.380 |
1 |
729.238 |
0. |
7.990 |
-700 |
700 |
Mg I |
5183.604 |
2.717 |
-0.160 |
1 |
729.238 |
0. |
7.990 |
-700 |
700 |
Ca I |
4434.957 |
1.886 |
-0.007 |
2 |
-7.162 |
-5.602 |
8.021 |
-300 |
100 |
Ca I |
4435.679 |
1.886 |
-0.517 |
2 |
-7.163 |
-5.610 |
8.025 |
-300 |
300 |
Ca I |
4454.779 |
1.899 |
0.258 |
2 |
-7.162 |
-5.596 |
8.017 |
-100 |
100 |
Ca I |
4455.887 |
1.899 |
-0.518 |
2 |
-7.162 |
-5.602 |
8.021 |
-300 |
300 |
Ca I |
5261.704 |
2.521 |
-0.579 |
3 |
-7.416 |
-5.756 |
7.903 |
-300 |
200 |
Ca I |
5265.556 |
2.523 |
-0.113 |
3 |
-7.416 |
-5.755 |
7.903 |
-300 |
50 |
Ca I |
6439.075 |
2.526 |
0.390 |
3 |
-7.704 |
-6.072 |
7.649 |
-300 |
300 |
Ca I |
6462.567 |
2.523 |
0.262 |
3 |
-7.704 |
-6.072 |
7.645 |
-300 |
50 |
Ca I |
6493.781 |
2.521 |
-0.109 |
3 |
-7.704 |
-6.071 |
7.640 |
-300 |
300 |
Ti I |
4533.241 |
0.848 |
0.476 |
4 |
-7.593 |
-5.144 |
8.083 |
-300 |
300 |
Ti I |
4534.776 |
0.836 |
0.280 |
4 |
-7.596 |
-5.313 |
8.079 |
-300 |
300 |
Ti I |
4535.568 |
0.826 |
0.161 |
5 |
-7.840 |
-5.403 |
8.079 |
-300 |
50 |
Ti II |
4394.059 |
1.221 |
-1.780 |
6 |
-7.944 |
-6.601 |
8.471 |
-100 |
300 |
Ti II |
4395.840 |
1.243 |
-1.930 |
6 |
-7.904 |
-6.550 |
8.471 |
-200 |
200 |
Ti II |
4399.765 |
1.237 |
-1.190 |
6 |
-7.946 |
-6.612 |
8.461 |
-300 |
200 |
Ti II |
4417.714 |
1.165 |
-1.190 |
6 |
-7.926 |
-6.665 |
8.225 |
-300 |
300 |
Ti II |
4443.801 |
1.080 |
-0.720 |
6 |
-7.923 |
-6.509 |
8.199 |
-200 |
300 |
Ti II |
4450.482 |
1.084 |
-1.520 |
6 |
-7.920 |
-6.502 |
8.199 |
-300 |
200 |
Ti II |
4468.507 |
1.131 |
-0.600 |
7 |
-7.931 |
-6.723 |
8.207 |
-300 |
300 |
Ti II |
4470.853 |
1.165 |
-2.020 |
6 |
-7.928 |
-6.713 |
8.217 |
-250 |
150 |
Ti II |
4501.270 |
1.116 |
-0.770 |
6 |
-7.931 |
-6.729 |
8.199 |
-300 |
300 |
Ti II |
4533.960 |
1.237 |
-0.530 |
6 |
-7.960 |
-6.661 |
8.225 |
-300 |
100 |
Ti II |
5185.902 |
1.893 |
-1.490 |
6 |
-7.908 |
-6.533 |
8.367 |
-300 |
300 |
Ti II |
5226.538 |
1.566 |
-1.260 |
6 |
-7.953 |
-6.713 |
8.217 |
-300 |
70 |
Fe I |
4375.930 |
0.000 |
-3.031 |
9 |
215.249 |
-6.320 |
4.622 |
-150 |
300 |
Fe I |
4375.986 |
3.047 |
-2.029 |
8 |
-7.800 |
-5.760 |
7.810 |
0 |
0 |
Fe I |
4383.545 |
1.485 |
0.208 |
9 |
295.265 |
-6.200 |
7.936 |
-300 |
300 |
Fe I |
4404.750 |
1.557 |
-0.147 |
9 |
301.263 |
-6.200 |
7.969 |
-250 |
200 |
Fe I |
4415.123 |
1.608 |
-0.621 |
9 |
308.257 |
-0.621 |
7.986 |
-150 |
200 |
Fe I |
4427.310 |
0.052 |
-2.924 |
9 |
-7.880 |
-6.320 |
4.696 |
-100 |
300 |
Fe I |
4430.614 |
2.223 |
-1.728 |
9 |
431.302 |
-6.080 |
8.606 |
-250 |
250 |
Fe I |
4442.339 |
2.198 |
-1.228 |
9 |
424.302 |
-6.080 |
8.599 |
-300 |
300 |
Fe I |
4443.194 |
2.858 |
-1.043 |
9 |
224.263 |
-6.340 |
7.799 |
-150 |
250 |
Fe I |
4443.196 |
3.071 |
-1.905 |
8 |
-7.770 |
-6.020 |
8.010 |
0 |
0 |
Fe I |
4447.717 |
2.223 |
-1.339 |
9 |
429.302 |
-6.080 |
8.604 |
-250 |
200 |
Fe I |
4461.653 |
0.087 |
-3.210 |
7 |
-7.799 |
-6.320 |
4.638 |
-200 |
200 |
Fe I |
4476.019 |
2.845 |
-0.819 |
9 |
-7.830 |
-6.170 |
7.825 |
-300 |
300 |
Fe I |
4476.076 |
3.686 |
-0.175 |
8 |
-7.670 |
-4.730 |
7.935 |
0 |
0 |
Fe I |
4482.170 |
0.110 |
-3.501 |
7 |
-7.799 |
-6.320 |
4.529 |
0 |
0 |
Fe I |
4482.253 |
2.223 |
-1.482 |
9 |
-7.788 |
-6.080 |
8.599 |
0 |
0 |
Fe I |
4489.739 |
0.121 |
-3.899 |
9 |
218.249 |
-6.320 |
4.403 |
-300 |
200 |
Fe I |
4494.563 |
2.198 |
-1.143 |
9 |
416.302 |
-6.080 |
8.600 |
-300 |
300 |
Fe I |
4528.614 |
2.176 |
-0.887 |
9 |
407.301 |
-6.080 |
8.607 |
-100 |
300 |
Fe I |
4531.148 |
1.485 |
-2.155 |
7 |
-7.678 |
-6.200 |
8.083 |
-250 |
300 |
Fe I |
4736.773 |
3.211 |
-0.752 |
9 |
820.231 |
-5.290 |
7.798 |
-200 |
200 |
Fe I |
4871.318 |
2.865 |
-0.363 |
9 |
748.235 |
-5.490 |
8.005 |
-300 |
300 |
Fe I |
4872.138 |
2.882 |
-0.567 |
9 |
754.235 |
-5.490 |
8.004 |
-300 |
300 |
Fe I |
4890.755 |
2.875 |
-0.394 |
9 |
758.236 |
-5.240 |
8.004 |
-350 |
300 |
Fe I |
4891.492 |
2.851 |
-0.112 |
9 |
750.237 |
-5.490 |
8.009 |
-300 |
350 |
Fe I |
4903.310 |
2.882 |
-0.926 |
9 |
-7.259 |
-5.490 |
8.004 |
-300 |
300 |
Fe I |
4918.994 |
2.865 |
-0.342 |
9 |
750.237 |
-5.490 |
8.009 |
-350 |
350 |
Fe I |
4918.954 |
4.154 |
-0.635 |
8 |
-7.510 |
-4.690 |
8.470 |
0 |
0 |
Fe I |
4920.503 |
2.832 |
0.068 |
9 |
739.238 |
-5.490 |
8.009 |
-300 |
300 |
Fe I |
5150.840 |
0.990 |
-3.037 |
9 |
-7.742 |
-6.250 |
7.180 |
-300 |
300 |
Fe I |
5166.282 |
0.000 |
-4.123 |
9 |
-7.826 |
-6.330 |
3.540 |
-180 |
180 |
Fe I |
5171.596 |
1.485 |
-1.721 |
9 |
-7.687 |
-6.200 |
6.330 |
-220 |
220 |
Fe I |
5191.455 |
3.038 |
-0.551 |
9 |
-7.258 |
-5.490 |
8.004 |
-300 |
300 |
Fe I |
5192.344 |
2.998 |
-0.421 |
9 |
-7.266 |
-5.490 |
8.010 |
-300 |
250 |
Fe I |
5194.942 |
1.557 |
-2.021 |
9 |
-7.680 |
-6.200 |
6.290 |
-300 |
200 |
Fe I |
5202.336 |
2.176 |
-1.838 |
7 |
-7.603 |
-6.180 |
8.230 |
-300 |
300 |
Fe I |
5202.256 |
4.256 |
-0.837 |
8 |
-7.765 |
-6.010 |
8.320 |
0 |
0 |
Fe I |
5216.274 |
1.608 |
-2.082 |
9 |
-7.674 |
-6.200 |
6.220 |
-300 |
300 |
Fe I |
5232.940 |
2.940 |
-0.058 |
9 |
-7.280 |
-5.490 |
8.009 |
-300 |
300 |
Fe I |
5266.554 |
2.998 |
-0.386 |
9 |
-7.273 |
-5.489 |
8.009 |
-300 |
300 |
Fe I |
5269.537 |
0.859 |
-1.321 |
7 |
-7.761 |
-6.300 |
7.185 |
-350 |
300 |
Fe I |
5281.790 |
3.038 |
-0.834 |
9 |
-7.266 |
-5.490 |
8.010 |
-200 |
200 |
Fe I |
5283.621 |
3.241 |
-0.524 |
9 |
-7.221 |
-5.450 |
7.880 |
-50 |
250 |
Fe I |
5324.191 |
3.211 |
-0.103 |
10 |
-7.235 |
-5.500 |
7.880 |
-250 |
250 |
Fe I |
5328.039 |
0.915 |
-1.466 |
7 |
-7.757 |
-6.302 |
7.161 |
-300 |
150 |
Fe I |
5328.532 |
1.557 |
-1.850 |
9 |
-7.686 |
-6.228 |
6.848 |
-150 |
300 |
Fe I |
5339.929 |
3.266 |
-0.647 |
10 |
-7.221 |
-5.451 |
7.874 |
-250 |
250 |
Fe I |
6393.601 |
2.433 |
-1.576 |
9 |
-7.622 |
-6.310 |
7.970 |
-250 |
250 |
Fe I |
6400.001 |
3.602 |
-0.290 |
10 |
-7.232 |
-5.500 |
7.900 |
-250 |
200 |
Fe I |
6430.846 |
2.176 |
-1.946 |
9 |
-7.704 |
-6.190 |
8.220 |
-220 |
220 |
Fe I |
6494.981 |
2.404 |
-1.273 |
7 |
-7.629 |
-6.330 |
7.936 |
-300 |
300 |
Fe II |
4416.828 |
2.778 |
-2.540 |
11 |
-7.950 |
-6.670 |
8.614 |
-200 |
300 |
Fe II |
4491.405 |
2.856 |
-2.700 |
12 |
-7.950 |
-6.600 |
8.481 |
-200 |
200 |
Fe II |
4508.288 |
2.856 |
-2.312 |
13 |
-7.950 |
-6.670 |
8.617 |
-250 |
250 |
Fe II |
4515.343 |
2.844 |
-2.362 |
14 |
-7.950 |
-6.600 |
8.487 |
-200 |
200 |
Fe II |
4923.927 |
2.891 |
-1.206 |
14 |
-7.914 |
-6.583 |
8.489 |
-300 |
300 |
Fe II |
5197.577 |
3.230 |
-2.100 |
12 |
-7.824 |
-6.600 |
8.480 |
-200 |
200 |
Fe II |
5234.625 |
3.221 |
-2.270 |
15 |
-7.946 |
-6.600 |
8.490 |
-200 |
200 |
Fe II |
5284.109 |
2.891 |
-3.130 |
11 |
-7.914 |
-6.600 |
8.530 |
-160 |
160 |
Fe II |
5316.615 |
3.153 |
-1.850 |
12 |
-7.950 |
-6.600 |
8.480 |
-300 |
100 |
1 Wiese & Martin (1980); 2 Smith & O'Neill (1975); 3 Smith & Raggett (1981); 4 Blackwell et al. (1982); 5 R. Kurucz, http://cfaku5.cfa.harvard.edu/ATOMS/2200; 6 Pickering et al. (2001); 7 Martin et al. (1988); 8 R. Kurucz, http://cfaku5.cfa.harvard.edu/ATOMS/2600; 9 O'Brian et al. (1991); 10 Bard et al. (1991); 11 Moity (1983); 12 Kroll & Kock (1987); 13 Biemont et al. (1991); 14 Schnabel et al. (2004); 15 Heise & Kock (1990).
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