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Table 1.

Spectral line data and equivalent widths.

ID Wavelength χexc log(gf) (a) EW (b) EW (c) Ref.
(Å) (eV) (mÅ) (mÅ) HFS
ScII 5239.82 1.46 −0.75 29.7 31.5 1
ScII 5526.82 1.77 −0.05 52.9 55.9 1
ScII 5657.88 1.51 −0.49 41.7 44.1 1
ScII 5667.15 1.50 −1.19 13.7 13.9 1
ScII 5669.04 1.50 −1.07 16.7 17.8 1
ScII 5684.20 1.51 −1.00 18.4 20.4 1
ScII 6245.62 1.51 −1.11 16.0 17.6 2
ScII 6604.60 1.36 −1.30 15.6 16.3 1
VI 4875.49 0.04 −0.81 12.3 9.7 3
VI 5703.59 1.05 −0.20 5.8 5.3 3
VI 5727.06 1.08 +0.02 8.4 8.7 3
VI 6090.22 1.08 −0.05 7.7 7.4 3
CoI 5342.71 4.02 +0.54 7.7 7.3 2
CoI 5352.05 3.58 −0.10 5.2 4.4 2
CoI 5369.60 1.74 −1.47 11.6 10.3 2
CoI 5483.36 1.71 −1.49 12.1 11.1 4

Notes.

(a)

Astrophysically calibrated as explained in the text.

(b)

Equivalent widths for HD 22879.

(c)

Equivalent widths for HD 76932.

References. (1) Lawler et al. (2019); (2) Prochaska et al. (2000); (3) Lawler et al. (2014); (4) Lawler et al. (2015).

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