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Table 6

Iron line selection for the M6 stellar parameter determination (Sect. 3.1.6).

λ E low log(gf) Sourcea
(nm) (eV)

Fe I
843.957 4.549 −0.587 K07
847.174 4.956 −1.037 K07
852.667 4.913 −0.760 BWL
852.785 5.020 −1.625 K07
857.180 5.010 −1.414 K07
859.295 4.956 −1.066 K07
859.883 4.386 −1.089 BWL
860.105 5.112 −1.577 K07
861.394 4.988 −1.247 K07
863.241 4.103 −2.341 K07
869.945 4.955 −0.380 BWL
872.914 3.415 −2.871 K07
874.743 3.018 −3.176 K07
879.052 4.988 −0.586 BWL
879.807 4.985 −1.895 K07
881.451 5.067 −1.793 K07
881.689 4.988 −2.203 K07
883.402 4.218 −2.558 K07
884.674 5.010 −0.777 K07
889.140 5.334 −1.108 K07

Fe II
611.332 3.221 −4.230 RU
614.774 3.889 −2.827 RU
641.692 3.892 −2.877 RU
643.268 10.930 −1.236 RU
645.638 3.903 −2.185 RU
651.608 2.891 −3.432 RU

Notes. For each line, the wavelength λ, the lower level excitation potential Elow, the gf value, and the source for the gf value are given. The full table is available at the CDS.

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