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Table 4

Modified stellar lines in the 6186−6214 Å spectral range.

Ion λori λnew log (gf)ori log (gf)new
(Å) (Å)

Si i 6194.416 ... 2.076 1.800
Si i 6194.884 ... 2.192 2.400
Si i 6195.433 ... 1.490 1.700
Si i 6208.541 ... 1.467 2.000
Ca i 6204.757 ... 0.276 2.000
Sc i 6193.666 ... 2.760 10.000
Sc i 6210.658 6210.648 1.529 ...
Ti i 6186.141 ... 1.270 1.650
Ti i 6200.318 ... 2.300 +0.300
Ti i 6200.227 ... 3.035 2.450
V i 6188.961 6188.940 1.062 2.650
V i 6189.364 6189.342 2.970 2.700
V i 6190.495 ... 2.377 2.600
V i 6199.197 6199.177 1.300 1.500
V i 6207.272 ... 1.370 ...
V i 6213.866 6213.846 2.050 1.850
Fe i 6187.398 ... 4.148 4.700
Fe i 6187.989 ... 1.720 2.600
Fe i 6190.398 ... 1.520 2.200
Fe i 6191.558 6191.563 1.417 1.700
Fe i 6196.968 ... 2.233 2.800
Fe i 6198.042 ... 2.049 2.400
Fe i 6199.506 ... 4.430 4.975
Fe i 6200.312 6200.302 2.437 2.900
Fe i 6202.305 ... 5.191 5.650
Fe i 6205.585 ... 2.219 3.500
Fe i 6207.230 ... 1.969 ...
Fe i 6208.211 ... 1.139 2.500
Fe i 6209.714 ... 3.249 3.800
Fe i 6212.013 ... 4.758 3.300
Fe i 6212.099 ... 2.913 3.400
Fe i 6213.429 6213.419 2.482 2.900
Fe ii ... 6187.996 ... 4.800
Fe ii ... 6199.190 ... 3.941
Co i 6188.996 ... 2.450 2.500
Co i 6197.833 ... 0.510 1.200
Ni i 6191.178 6191.168 2.939 2.300
Ni i 6204.600 ... 1.100 1.060
Y i 6191.718 ... 0.680 ...
Nd ii 6210.680 6210.660 1.540 1.540

Notes.

(∗)

Lines susceptible to finer tuning (see discussion in Sect. 4).

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