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Table 2

Lines of Cr i and Cr ii selected for solar and stellar abundance calculations.

Id. (a) λ Mult. E low Lower Upper log gf log C6 log (gfε)
   [Å] [eV] level level
Cr i
bl 4254.35(b)  1 0.00  −0.090  −31.54  −
bl 4274.80(b)  1 0.00  −0.220  −31.55  −
bl 4289.72(b)  1 0.00  −0.370  −31.55  −
bl 4373.25 22 0.98  −2.300  −31.72 3.46
4492.31 197 3.38  −0.390  −31.34 5.34
bl. w 4496.86 10 0.94  −1.140  −31.62 4.61
4535.15 33 2.54  −1.020  −31.59 4.74
4541.07 33 2.54  −1.150  −31.59 4.58
4545.96 10 0.94  −1.370  −31.63 4.39
bl. w 4591.39 21 0.97  −1.740  −31.75 4.01
bl 4600.75 21 1.00  −1.250  −31.74 4.49
bl. w 4613.37 21 0.96  −1.650  −31.76 4.13
4616.14 21 0.98  −1.190  −31.75 4.54
4626.19 21 0.97  −1.330  −31.76 4.42
4633.29 186 3.13  −1.110  −31.18 4.62
4646.17 21 1.03  −0.740  −31.74 5.01
bl. w 4651.28 21 0.98  −1.460  −31.75 4.30
bl. w 4652.16 21 1.00  −1.040  −31.75 4.71
4700.61 62 2.71  −1.255  −31.61 4.51
bl 4708.04 186 3.17 0.07  −31.18 5.83
bl. w 4745.31 61 2.71  −1.380  −31.17 4.33
4801.03 168 3.12  −0.131  −31.35 5.62
bl 4885.78(b)  30 2.54  −1.055  −31.3  −
4936.33 166 3.11  −0.25  −31.37 5.47
4953.72 166 3.12  −1.48  −31.37 4.23
bl 5204.52(b)  7 0.94  −0.19  −31.36  −
bl 5206.04 7 0.94 0.02  −31.36 5.67
bl 5208.44 7 0.94 0.17  −31.36 5.83
5241.46 59 2.71  −1.920  −31.3 3.74
bl. w 5243.40 201 3.40  −0.580  −31.22 5.17
5247.56 18 0.96  −1.590  −31.41 4.28
5272.01 225 3.45  −0.420  −31.2 5.31
5287.19 225 3.44  −0.870  −31.21 4.84
5296.69 18 0.98  −1.360  −31.41 4.49
5300.75 18 0.98  −2.000  −31.41 3.73
bl. w 5304.21 225 3.46  −0.670  −31.2 5.04
5312.88 225 3.45  −0.550  −31.21 5.17
5318.78 225 3.44  −0.670  −31.22 5.04
5340.44 225 3.44  −0.730  −31.22 5.02
5345.81 18 1.00  −0.95  −31.41 4.87
5348.32 18 1.00  −1.21  −31.41 4.60
bl. w 5409.79 18 1.03  −0.670  −31.41 5.15
5628.64 203 3.42  −0.740  −31.34 4.99
Cr ii
4555.00 44 4.07  −1.25  −32.4 4.42
4558.66 44 4.07  −0.66  −32.4 5.30
bl 4588.22 44 4.07  −0.83  −32.4 5.08
4592.09 44 4.07  −1.42  −32.4 4.47
bl 4634.11 44 4.07  −0.98  −32.4 4.69
bl 4812.35 30 3.86  −2.10  −32.46 3.73
bl 4824.14 30 3.87  −0.92  −32.46 5.01
bl 5237.34 43 4.07  −1.16  −32.4 4.51
bl 5308.44 43 4.07  −1.81  −32.4 3.84
5313.59 43 4.07  −1.65  −32.4 4.09

Notes.

(a)

Line identification:  bl – blended (in the line core or inner wing),  bl. w – blended in the wing only.

(b)

Solar log (gfε) value for this line can not be reliably computed due to severe blending. The line is not used in determination of the solar Cr abundance.

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