Table B.1
List of measured lines.
Species | λ | χexc | log gfadopted | |
(Å) | (eV) | |||
|
||||
Y ii | 4883.682 | 1.084 | 0.000 | c |
Y ii | 5087.416 | 1.084 | –0.330 | c |
Y ii | 5200.406 | 0.992 | –0.730 | c |
Y ii | 5289.815 | 1.033 | –1.900 | c |
Y ii | 5320.782 | 1.084 | –1.950 | d |
Y ii | 5402.774 | 1.839 | –0.640 | c |
Y ii | 5544.611 | 1.738 | –0.980 | c |
Y ii | 5546.009 | 1.748 | –1.120 | c |
Y ii | 5728.887 | 1.839 | –1.300 | c |
Y ii | 6795.414 | 1.738 | –1.620 | c |
Zr i | 4772.310 | 0.623 | 0.040 | d |
Zr i | 6127.440 | 0.154 | –1.060 | d |
Zr i | 6134.550 | 0.000 | –1.280 | d |
Zr i | 6143.200 | 0.071 | –1.100 | d |
Zr ii | 5112.270 | 1.665 | –0.850 | d |
La ii | 4558.460 | 0.321 | –0.970 | d |
La ii | 4574.860 | 0.173 | –1.080 | d |
La ii | 4662.500 | 0.000 | –1.240 | d |
La ii | 4748.730 | 0.927 | –0.540 | d |
La ii | 4804.039* | 0.235 | –1.490 | b |
La ii | 4920.980 | 0.126 | –0.580 | d |
La ii | 5114.560 | 0.235 | –1.030 | d |
La ii | 5290.820 | 0.000 | –1.650 | d |
La ii | 5303.528* | 0.321 | –1.350 | b |
La ii | 5797.570 | 0.244 | –1.360 | d |
La ii | 5880.630 | 0.235 | –1.830 | d |
La ii | 6390.478* | 0.321 | –1.41 | b |
La ii | 6774.268 | 0.126 | –1.820 | b |
Ce ii | 4515.849 | 1.058 | –0.240 | d |
Ce ii | 4523.075 | 0.516 | –0.240 | c |
Ce ii | 4562.359 | 0.478 | 0.210 | b |
Ce ii | 4628.239 | 1.366 | –0.430 | d |
Ce ii | 4773.941 | 0.924 | –0.390 | b |
Ce ii | 5274.229 | 1.044 | –0.170 | c |
Ce ii | 5472.279 | 1.247 | –0.100 | d |
Ce ii | 5975.818 | 1.327 | –0.450 | b |
Ce ii | 6043.373 | 1.206 | –0.480 | a |
Nd ii | 4645.760 | 0.559 | –0.760 | d |
Notes. The table lists: wavelength λ, excitation potential χexc, adopted oscillator strengths log gf, and source: (a) Merle et al. (2016), (b) GES line list v5 (Heiter et al. 2015), (c) adjusted to reproduce solar and/or Arcturus abundances, and (d) VALD. The effective log gf is given for lines whose hyperfine structure was taken into account (identified with an asterisk after the wavelength).
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