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Table 5

List of “golden” Fe II lines for various groups of stars (see text for definition of groups).

λ [Å] E [eV] log gf Waals Ref MPD (2) MPG (1) FGD (15) FGKG (7) MG (4) KD (1)

4923.93 2.8910 –1.260 175.202 158 0.16/0.25 4/4
4993.36 2.8070 –3.684 172.220 166 0.04 3 0.00/0.21 3/4 0.13/0.64 3/4 0.29 4
5264.81 3.2300 –3.130 186.300 158 0.09 3
5325.55 3.2210 –3.160 179.252 158 0.08 3
5414.07 3.2210 –3.580 185.303 158 0.01/0.07 3/4 0.07/0.24 3/4 0.08 3
5425.26 3.1990 –3.220 178.255 158 0.14 3 0.01/0.14 4/5 0.09/0.35 4/5 0.17/0.50 3/5 0.11 5
5534.85 3.2450 –2.865 178.239 166 0.06 3
5991.38 3.1530 –3.647 172.221 166 0.01/0.12 3/4 0.04 3
6084.11 3.1990 –3.881 173.223 166 0.08/0.20 3/4 0.03 3
6247.56 3.8920 –2.435 186.272 166 0.04 3
6432.68 2.8910 –3.570 169.204 158 0.07 3 0.01/0.32 3/4 0.02/0.07 3/4 0.10/0.19 3/4 0.05 3
6456.38 3.9030 –2.185 185.276 166 0.14 4 0.03/0.19 4/5 0.04/0.38 4/5 0.14/0.24 4/4 0.03 5

Notes. Column descriptions: λ: wavelength. Elow: lower level energy. “Waals”: parameters used to calculate line broadening due to collisions with neutral hydrogen. Integer component: broadening cross-section at a velocity of 104 m s-1 in atomic units. Fractional component: velocity parameter (see Barklem et al. 2000). If zero, the Unsöld approximation was used. “Ref”: reference code for the gf-values (see below). The remaining columns are headed by a label for each group defined in the text and the number of stars in parantheses. The columns give the minimum and maximum standard deviations of the average line abundances and the minimum and maximum number of abundances averaged for each line for each group. 5414.07 Å was not used in μ Cas and 5991.38 Å not in HD 49933. The column marks the lines used for ϵ Eri; of these, only 4993.36 Å and 6456.38 Å were used in 61 Cyg A and Gmb 1830; only 4993.36 Å and 5425.26 Å in 61 Cyg B.

Reference. 158: Meléndez & Barbuy (2009). 166: Raassen & Uylings (1998).

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