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Table 3

Line data and equivalent widths measured for the two standard stars (HD 22879 and HD 76932), the solar flux, and the prototypes of low-, and high-α stars, CD−45   3283 and G 159-50.

Element Wavelength exc.pot. log (gf)a HD 22879 HD 76932 Solar flux CD  − 45   3283 G 159-50 etc.
[Å] [eV] EW [mÅ] EW [mÅ] EW [mÅ] EW [mÅ] EW [mÅ]

Na i 4982.82 2.10 −1.00 25.4 22.1 9.9 21.5 ...
Na i 5682.64 2.10 −0.77 38.2 35.3 19.4 34.2 ...
Na i 5688.21 2.10 −0.48 59.8 55.8 32.5 54.1 ...
Na i 6154.22 2.10 −1.59 7.4 7.6 37.8 3.6 7.1 ...
Na i 6160.74 2.10 −1.30 14.0 13.2 56.9 5.4 11.8 ...
Mg i 4730.03 4.34 −2.33 ...
Mg i 5711.09 4.34 −1.74 71.0 66.4 115.5 55.9 76.2 ...
Si i 5684.48 4.95 −1.68 27.6 26.0 60.7 18.6 26.3 ...
Si i 5690.42 4.93 −1.88 20.4 18.2 54.6 13.6 18.5 ...
Si i 5701.10 4.93 −2.06 14.1 13.0 40.3 9.6 13.8 ...
Si i 6142.48 5.62 −1.52 11.2 11.4 34.6 7.4 10.0 ...
Si i 6145.01 5.61 −1.46 13.6 12.5 38.6 9.9 12.5 ...
Si i 6155.13 5.62 −0.89 39.5 36.6 26.4 35.1 ...
Si i 6237.32 5.61 −1.15 24.3 23.8 14.6 21.6 ...
Si i 6243.81 5.61 −1.33 17.3 16.8 46.8 10.2 16.2 ...
Si i 6244.47 5.61 −1.36 16.7 15.5 45.3 9.3 15.3 ...
Si i 6414.98 5.87 −1.08 18.0 15.3 48.3 11.2 17.4 ...
Ca i 5260.38 2.52 −1.79 10.5 9.8 32.1 9.6 11.2 ...
Ca i 5349.46 2.71 −0.45 63.1 60.9 61.9 ...
Ca i 5512.98 2.93 −0.52 47.9 45.1 45.2 49.5 ...
Ca i 5581.97 2.52 −0.63 61.3 59.5 58.9 66.1 ...
Ca i 5590.12 2.52 −0.65 59.7 58.7 59.4 64.1 ...
Ca i 6161.28 2.52 −1.33 26.9 25.8 61.5 25.1 28.7 ...
Ca i 6166.43 2.52 −1.19 34.3 32.1 72.1 32.0 36.3 ...
Ca i 6169.03 2.52 −0.85 55.3 51.8 102.0 55.7 58.5 ...
Ca i 6169.55 2.52 −0.58 74.0 69.1 74.4 ...
Ti i 4820.40 1.50 −0.34 17.2 15.4 45.5 14.9 18.7 ...
Ti i 4913.61 1.87 0.18 23.4 21.1 55.3 19.9 25.4 ...
Ti i 4999.50 0.83 0.27 77.4 75.2 76.3 81.0 ...
Ti i 5016.16 0.85 −0.55 36.0 32.4 33.0 39.6 ...
Ti i 5022.86 0.83 −0.41 44.0 40.0 42.1 46.4 ...
Ti i 5024.84 0.82 −0.55 36.9 33.9 35.0 41.2 ...
Ti i 5039.95 0.02 −1.12 48.5 45.0 46.8 52.3 ...
Ti i 5147.47 0.00 −1.97 13.7 11.3 39.0 13.4 16.6 ...
Ti i 5192.97 0.02 −0.99 56.2 51.9 54.1 58.8 ...
Ti i 5210.38 0.05 −0.85 62.3 57.4 61.5 ...
Ti i 5866.41 1.07 −0.78 18.9 16.0 52.3 15.7 21.5 ...
Ti i 6258.10 1.44 −0.34 22.0 19.7 50.9 20.0 24.9 ...
Ti i 6258.70 1.46 −0.19 27.7 24.4 24.4 30.6 ...
Ti i 6261.10 1.43 −0.46 18.6 15.9 49.1 16.4 21.0 ...
Cr i 4801.02 3.12 −0.19 14.3 12.6 52.0 15.3 14.5 ...
Cr i 4936.33 3.11 −0.32 11.6 10.2 46.4 11.7 13.1 ...
Cr i 5296.69 0.98 −1.52 47.0 43.8 53.3 51.7 ...
Cr i 5300.74 0.98 −2.22 16.2 14.3 20.2 19.2 ...
Cr i 5329.14 2.91 −0.17 22.9 20.9 24.5 23.7 ...
Cr i 5345.80 1.00 −1.08 67.3 66.6 73.1 74.0 ...
Cr i 5348.32 1.00 −1.42 51.3 48.7 57.3 56.0 ...
Mn i 4783.4 2.30 −0.04 70.0 67.7 79.4 77.4 ...
Mn i 4823.5 2.32 0.05 71.7 68.5 77.6 78.4 ...
Mn i 6013.5 3.07 −0.42 13.4 12.9 88.3 15.1 15.3 ...
Mn i 6016.7 3.07 −0.25 19.6 18.0 97.9 21.0 21.2 ...
Mn i 6021.8 3.07 −0.10 24.5 23.0 102.4 27.0 27.5 ...
Fe i 4788.76 3.24 −1.74 28.9 26.2 71.4 30.6 29.2 ...
Fe i 4800.64 4.14 −1.10 20.6 19.3 22.3 21.4 ...
Fe i 4924.77 2.28 −2.17 54.3 51.2 59.2 55.5 ...
Fe i 4939.68 0.86 −3.32 65.6 62.6 ...
Fe i 4950.10 3.42 −1.56 30.6 28.6 34.2 32.0 ...
Fe i 4962.57 4.18 −1.18 17.1 15.4 59.7 17.6 16.4 ...
Fe i 4973.09 3.96 −0.77 44.2 41.7 47.2 45.9 ...
Fe i 5044.21 2.85 −2.07 32.5 29.8 36.2 33.8 ...
Fe i 5054.67 3.64 −2.04 8.6 7.4 44.1 9.0 10.5 ...
Fe i 5067.14 4.22 −0.86 27.7 26.1 31.2 28.9 ...
Fe i 5074.74 4.22 −0.13 67.6 65.5 75.0 71.7 ...
Fe i 5090.77 4.26 −0.49 45.1 42.0 48.6 46.2 ...
Fe i 5109.65 4.30 −0.73 30.5 28.5 84.7 33.3 31.1 ...
Fe i 5126.19 4.26 −0.85 27.3 23.8 28.1 27.7 ...
Fe i 5127.36 0.91 −3.33 62.6 61.7 67.7 66.5 ...
Fe i 5131.47 2.22 −2.46 43.2 39.8 46.1 45.3 ...
Fe i 5141.74 2.42 −2.23 45.4 41.7 49.1 48.0 ...
Fe i 5145.09 2.20 −3.15 15.5 13.2 18.8 18.7 ...
Fe i 5159.05 4.28 −0.81 27.9 25.8 29.3 28.6 ...
Fe i 5187.91 4.14 −1.24 16.7 15.1 17.8 16.7 ...
Fe i 5198.71 2.22 −2.14 58.6 58.0 66.3 61.1 ...
Fe i 5225.52 0.11 −4.75 33.7 30.4 75.0 41.5 37.6 ...
Fe i 5228.37 4.22 −1.05 19.9 18.7 20.2 21.0 ...
Fe i 5242.49 3.63 −0.99 47.9 45.5 50.3 48.7 ...
Fe i 5243.77 4.26 −0.99 20.8 19.6 65.6 22.0 21.6 ...
Fe i 5247.05 0.09 −4.91 27.4 24.0 34.1 32.2 ...
Fe i 5250.21 0.12 −4.90 26.9 23.4 33.7 31.4 ...
Fe i 5250.64 2.20 −2.09 61.9 61.7 68.1 67.0 ...
Fe i 5253.46 3.28 −1.65 33.2 31.0 38.5 35.4 ...
Fe i 5263.30 3.26 −0.97 73.2 70.5 ...
Fe i 5281.79 3.04 −0.94 87.6 83.4 101.5 ...
Fe i 5288.52 3.69 −1.59 19.0 17.3 57.7 19.7 19.5 ...
Fe i 5307.36 1.61 −2.97 47.6 45.7 51.9 49.8 ...
Fe i 5321.10 4.43 −1.26 9.0 8.4 40.9 10.0 9.3 ...
Fe i 5322.04 2.28 −2.92 20.4 18.1 64.6 24.2 22.4 ...
Fe i 5339.93 3.26 −0.80 86.4 79.5 ...
Fe i 5364.87 4.44 0.11 73.4 68.2 ...
Fe i 5365.40 3.57 −1.25 39.2 36.4 41.3 39.7 ...
Fe i 5367.47 4.41 0.19 79.7 75.5 ...
Fe i 5373.70 4.47 −0.77 22.1 20.6 67.9 24.4 22.4 ...
Fe i 5379.57 3.69 −1.53 21.0 19.3 65.2 22.4 22.0 ...
Fe i 5389.48 4.41 −0.45 39.9 37.4 43.6 40.6 ...
Fe i 5393.17 3.24 −0.80 87.5 79.9 104.5 ...
Fe i 5398.28 4.44 −0.60 30.9 28.5 78.1 32.6 30.5 ...
Fe i 5409.13 4.37 −1.06 15.1 14.5 54.9 16.7 16.7 ...
Fe i 5415.20 4.39 0.42 97.5 92.2 ...
Fe i 5432.95 4.44 −0.63 27.9 28.9 27.8 26.8 ...
Fe i 5445.04 4.39 0.00 67.1 64.7 74.8 70.2 ...
Fe i 5473.90 4.15 −0.78 35.3 33.1 38.5 36.1 ...
Fe i 5501.47 0.96 −3.06 74.8 73.5 80.7 78.1 ...
Fe i 5543.93 4.22 −1.03 21.1 19.6 67.5 22.6 22.0 ...
Fe i 5554.89 4.55 −0.36 38.1 35.8 41.3 39.3 ...
Fe i 5560.21 4.43 −1.04 14.4 13.3 54.5 15.4 14.8 ...
Fe i 5567.39 2.61 −2.66 18.1 17.1 21.7 20.6 ...
Fe i 5569.62 3.42 −0.63 89.0 82.6 ...
Fe i 5576.09 3.43 −0.94 67.2 63.6 75.0 ...
Fe i 5618.63 4.21 −1.27 13.6 12.9 50.3 14.3 13.9 ...
Fe i 5624.55 3.42 −0.82 76.2 70.6 ...
Fe i 5633.94 4.99 −0.23 24.0 22.0 25.3 23.6 ...
Fe i 5638.26 4.22 −0.78 32.1 30.3 83.7 35.0 33.9 ...
Fe i 5679.02 4.65 −0.71 17.6 17.7 63.1 19.4 18.4 ...
Fe i 5686.53 4.55 −0.57 28.2 26.6 31.2 28.4 ...
Fe i 5701.55 2.56 −2.21 40.3 38.3 86.2 45.7 43.4 ...
Fe i 5717.83 4.28 −1.01 19.5 19.6 22.5 20.4 ...
Fe i 5731.76 4.26 −1.11 17.3 16.0 60.7 20.6 18.0 ...
Fe i 5852.22 4.55 −1.15 9.5 8.7 44.1 9.5 9.1 ...
Fe i 5856.09 4.29 −1.52 6.9 6.8 33.2 7.6 7.0 ...
Fe i 5859.59 4.55 −0.58 27.7 26.5 30.3 28.1 ...
Fe i 6003.01 3.88 −1.10 33.5 31.9 38.2 35.5 ...
Fe i 6024.06 4.55 −0.02 59.0 53.8 68.0 59.1 ...
Fe i 6027.05 4.07 −1.13 24.1 21.9 67.0 28.0 24.9 ...
Fe i 6079.01 4.65 −0.99 10.8 10.1 49.0 12.6 10.1 ...
Fe i 6082.71 2.22 −3.58 7.0 5.7 35.0 7.6 8.3 ...
Fe i 6151.61 2.18 −3.31 12.7 11.4 49.9 15.2 15.7 ...
Fe i 6157.72 4.07 −1.20 21.1 19.8 61.9 23.5 21.3 ...
Fe i 6165.35 4.14 −1.49 10.6 10.1 44.3 9.9 ...
Fe i 6173.33 2.22 −2.88 25.5 24.3 71.2 30.5 29.5 ...
Fe i 6180.20 2.73 −2.70 14.3 13.4 55.3 18.6 17.5 ...
Fe i 6200.31 2.61 −2.43 28.8 26.6 76.4 34.3 31.6 ...
Fe i 6213.43 2.22 −2.55 40.9 39.1 86.2 46.1 45.2 ...
Fe i 6219.28 2.20 −2.43 48.7 45.8 96.7 54.0 51.6 ...
Fe i 6246.32 3.60 −0.87 63.9 58.9 74.4 65.7 ...
Fe i 6252.55 2.40 −1.72 75.5 73.2 128.5 82.1 82.2 ...
Fe i 6265.13 2.18 −2.52 45.3 42.5 90.9 49.9 47.5 ...
Fe i 6335.33 2.20 −2.26 57.3 55.2 65.2 62.6 ...
Fe i 6336.82 3.69 −0.93 54.6 51.9 64.5 56.7 ...
Fe i 6355.03 2.84 −2.31 24.5 22.6 29.4 26.1 ...
Fe i 6358.68 0.86 −4.24 26.3 22.9 83.9 32.8 30.3 ...
Fe i 6393.60 2.43 −1.60 80.9 78.2 91.2 88.7 ...
Fe i 6411.65 3.65 −0.69 73.1 68.1 ...
Fe i 6421.35 2.28 −2.02 67.3 63.8 75.2 70.2 ...
Fe i 6430.85 2.18 −2.01 71.3 69.7 78.6 75.6 ...
Fe ii 4993.34 2.81 −3.73 15.2 15.9 41.4 11.2 12.4 ...
Fe ii 5132.66 2.81 −4.17 6.4 6.7 25.6 4.4 6.1 ...
Fe ii 5197.57 3.23 −2.33 56.0 60.8 47.0 48.8 ...
Fe ii 5234.62 3.22 −2.29 58.2 63.6 89.1 49.8 51.7 ...
Fe ii 5264.80 3.23 −3.15 20.8 23.2 45.8 14.7 15.8 ...
Fe ii 5284.10 2.89 −3.20 32.4 34.5 23.4 26.2 ...
Fe ii 5325.55 3.22 −3.25 18.2 19.6 41.4 13.0 13.4 ...
Fe ii 5414.07 3.22 −3.63 8.8 9.5 27.8 6.0 6.0 ...
Fe ii 5425.25 3.20 −3.31 17.1 18.1 44.0 11.5 12.5 ...
Fe ii 5534.84 3.24 −2.88 32.7 35.4 59.1 25.3 26.6 ...
Fe ii 6084.09 3.20 −3.83 6.2 7.0 20.7 3.7 3.8 ...
Fe ii 6149.24 3.89 −2.75 14.7 15.8 36.4 10.1 9.7 ...
Fe ii 6238.38 3.89 −2.63 18.2 19.8 43.8 12.2 12.5 ...
Fe ii 6247.55 3.89 −2.38 27.1 29.6 52.5 19.8 21.2 ...
Fe ii 6416.92 3.89 −2.75 15.1 16.2 40.4 10.2 11.9 ...
Fe ii 6432.67 2.89 −3.65 16.4 18.1 41.0 11.5 13.1 ...
Ni i 4806.98 3.68 −0.60 21.5 20.2 17.4 20.6 ...
Ni i 4829.02 3.54 −0.33 40.1 38.0 35.3 40.3 ...
Ni i 4831.17 3.61 −0.38 34.1 31.9 77.6 28.3 34.1 ...
Ni i 4904.41 3.54 −0.19 47.8 45.2 43.3 47.8 ...
Ni i 4913.97 3.74 −0.62 18.4 18.1 60.0 15.0 19.1 ...
Ni i 4935.82 3.94 −0.31 23.3 21.7 64.5 19.2 23.3 ...
Ni i 4937.34 3.61 −0.38 35.0 32.4 29.4 34.7 ...
Ni i 4953.20 3.74 −0.61 19.7 17.6 60.0 19.2 ...
Ni i 4998.22 3.61 −0.76 18.2 17.0 14.3 18.1 ...
Ni i 5010.93 3.63 −0.85 15.2 13.9 51.7 10.8 14.4 ...
Ni i 5035.36 3.63 0.12 59.3 60.0 56.0 60.7 ...
Ni i 5081.11 3.85 0.22 54.0 52.5 50.2 55.3 ...
Ni i 5082.34 3.66 −0.55 24.7 23.5 75.4 20.4 25.5 ...
Ni i 5084.09 3.68 −0.04 48.8 47.7 43.1 49.3 ...
Ni i 5099.93 3.68 −0.18 40.7 40.3 35.7 41.0 ...
Ni i 5102.96 1.68 −2.83 12.3 11.6 11.1 14.1 ...
Ni i 5115.39 3.83 −0.14 35.9 34.3 31.4 35.8 ...
Ni i 5155.12 3.90 −0.63 14.3 13.0 53.1 11.5 14.6 ...
Ni i 5155.76 3.90 −0.11 34.2 32.8 30.0 34.8 ...
Ni i 5176.55 3.90 −0.46 19.8 17.9 59.7 14.4 19.4 ...
Ni i 5578.72 1.68 −2.74 15.9 14.4 14.0 17.4 ...
Ni i 5587.86 1.93 −2.41 18.2 17.0 17.8 19.8 ...
Ni i 5682.20 4.10 −0.43 15.0 13.8 53.4 11.0 14.5 ...
Ni i 6086.28 4.26 −0.49 10.3 9.3 44.3 8.3 10.8 ...
Ni i 6108.12 1.68 −2.61 20.8 19.8 67.5 19.5 25.0 ...
Ni i 6175.36 4.09 −0.51 13.3 12.8 49.2 10.6 13.6 ...
Ni i 6176.81 4.09 −0.31 19.5 18.6 67.9 16.6 20.8 ...
Cu i 5105.5 1.39 −1.58 31.3 25.7 95.9 18.2 32.4 ...
Cu i 5218.2 3.82 0.36 13.7 12.2 56.5 6.8 12.1 ...
Cu i 5782.1 1.64 −1.78 ...
Zn i 4722.15 4.03 −0.50 70.8 ...
Zn i 4810.53 4.08 −0.31 48.8 48.5 82.8 37.7 45.7 ...
Y ii 4883.68 1.08 0.01 39.0 40.3 63.9 25.0 35.5 ...
Y ii 5087.42 1.08 −0.28 26.2 27.8 51.0 14.4 23.9 ...
Ba ii 5853.68 0.60 −0.94 38.9 41.9 70.2 32.9 39.6 ...
Ba ii 6141.72 0.70 0.06 84.2 87.7 132.5 81.7 87.5 ...

Notes. 

(a)

The large majority of gf-values are determined from UVES spectra of the two standard stars, HD 22879 and HD 76932, as described in Sect. 2.1. For three lines that are only available in the FIES spectra (Mg i 4730.0, Cu i 5782.1, and Zn i 4722.2), the gf-value is determined so that for the sample of FIES stars, the mean elemental abundance derived from the line agrees with the mean abundance derived from the other lines of the element.

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