Table B.1
Some of the data in the used line list.
Wavelength [Å] | Species | Elow [eV] | vdW(This work) | log gf(This work) | log gf(On12) | |
|
||||||
11 681.594 | Fe I | 3.55 | −6.725 | −3.216 | −3.301 | FGK |
11 700.239 | Si I | 6.27 | −7.294 | −0.513 | −0.526 | FGK |
11 712.010 | Ca I | 4.68 | −8.593 | −0.501 | −1.510 | FGK |
11 767.600 | Ca I | 4.532 | −6.621 | −0.666 | −0.635 | FGK, M |
11 780.547 | Ti I | 1.443 | −7.790 | −2.273 | −2.180 | FGK, M |
11 783.267 | Fe I | 2.832 | −8.012 | −1.615 | −1.520 | FGK, M |
11 797.179 | Ti I | 1.430 | −7.790 | −2.250 | −2.250 | FGK, M |
11 797.215 | Fe I | 5.82 | −7.420 | −1.788 | −1.788 | FGK, M |
11 800.657 | Fe I | 6.20 | −7.160 | −1.090 | −1.090 | FGK |
11 828.171 | Mg I | 4.35 | 862.255 | −0.220 | −0.046 | FGK, M |
11 949.545 | Ti I | 1.443 | −7.790 | −1.550 | −1.550 | FGK, M |
11 949.760 | Ca II | 6.470 | −7.743 | +0.218 | −0.040 | FGK |
11 955.955 | Ca I | 4.131 | −7.132 | −0.835 | −0.849 | FGK, M |
11 973.050 | Fe I | 2.176 | −7.881 | −1.566 | −1.405 | FGK, M |
11 955.955 | Ca I | 4.13 | −7.132 | −0.835 | −0.849 | FGK |
11 973.050 | Fe I | 2.18 | −7.881 | −1.566 | −1.405 | FGK |
11 973.854 | Ti I | 1.460 | −7.380 | −1.558 | −1.591 | FGK, M |
11 984.198 | Si I | 4.930 | 677.228 | +0.108 | +0.239 | FGK, M |
11 991.568 | Si I | 4.920 | 674.228 | −0.257 | −0.109 | FGK, M |
12 031.504 | Si I | 4.954 | 685.229 | +0.331 | +0.477 | FGK, M |
12 039.822 | Mg I | 5.753 | −7.239 | −1.525 | −1.530 | FGK |
12 044.055 | Cr I | 3.422 | −6.281 | −1.863 | −1.863 | FGK |
12 044.129 | Fe I | 4.988 | −6.677 | −2.130 | −2.130 | FGK |
12 053.083 | Fe I | 4.559 | −7.439 | −1.535 | −1.543 | FGK |
12 510.520 | Fe I | 4.956 | −7.296 | −1.845 | −1.846 | FGK |
12 532.835 | Cr I | 2.709 | −8.349 | −1.902 | −1.879 | FGK, M |
12 556.999 | Fe I | 2.279 | −8.680 | −3.879 | −3.913 | FGK, M |
12 569.569 | Ti I | 2.175 | −7.810 | −1.867 | −1.867 | FGK, M |
12 569.634 | Co I | 3.409 | −7.730 | −1.605 | −0.992 | FGK, M |
12 600.277 | Ti I | 1.443 | −7.790 | −2.275 | −2.150 | FGK, M |
12 909.070 | Ca I | 4.43 | −7.471 | −0.461 | −0.426 | FGK, M |
12 910.087 | Cr I | 2.708 | −7.509 | −1.821 | −1.863 | FGK, M |
12 919.898 | Ti I | 2.154 | −8.970 | −1.611 | −1.553 | FGK, M |
12 937.016 | Cr I | 2.710 | −7.625 | −1.916 | −1.896 | FGK, M |
12 919.898 | Ti I | 2.15 | −8.970 | −1.611 | −1.553 | FGK, M |
12 975.720–12 976.150 † | Mn I | FGK, M | ||||
13 001.401 | Ca I | 4.441 | −7.396 | −1.273 | −1.139 | FGK, M |
13 006.685 | Fe I | 2.990 | −7.725 | −3.268 | −3.269 | FGK, M |
13 011.892 | Ti I | 1.443 | −6.792 | −2.242 | −2.180 | FGK, M |
13 033.555 | Ca I | 4.441 | −7.462 | −0.194 | −0.064 | FGK, M |
13 057.885 | Ca I | 4.441 | −7.716 | −1.054 | −1.092 | FGK, M |
Notes. Column descriptions: Elow: lower level energy. VdW: parameter(s) used to calculate line broadening due to van der Waals interaction. Negative numbers: logarithm of the line width per perturber at l04 K in rad s-1 cm3 (logγW). Adjusted by fit to a solar spectrum (see Sect. 4.3.1). Positive numbers: integer part: broadening cross-section at a velocity of 104 m s-1 in atomic units, fractional part: velocity parameter (see Barklem et al. 2000). log gf: oscillator strength, adjusted by fit to a solar spectrum (see Sect. 4.3.1 in this paper, and the values adopted by On12). FGK/FGK, M: lines used for the analysis of only the primaries or for both binary components.
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