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Table 1.

Atomic data of the 15 observed spectral lines at VTT.

Element Wavelength (Å) Jl Ju log(gf) χe (eV) geff α
Mn I 5780.1612 5.5 4.5 −1.076 ± 0.235 4.25 1.046 0.249 251
Fe I 5780.2828 4.0 4.0 −2.482 ± 0.118 4.22 1.325 0.271 811
Si I 5780.3838 0.0 1.0 −2.722 ± 0.032 4.20 0.500 0.219 1708
( * )Fe I 5780.5994 3.0 3.0 −2.324 ± 0.034 3.24 1.625 0.244 737
Fe I 5780.8036 2.0 2.0 −2.663 ± 0.038 3.26 1.750 0.244 745
Fe I 5780.8313 4.0 5.0 −2.885 ± 0.413 4.43 2.010 0.269 767
Cr I 5780.9052 3.0 2.0 −1.793 ± 0.357 3.32 1.833 0.288 1098
Cr I 5781.1791 2.0 1.0 −0.619 ± 0.029 3.32 2.000 0.288 1099
( * )Cr I 5781.7512 1.0 0.0 −0.548 ± 0.025 3.32 2.500 0.288 1100
Cu I 5782.0970 1.5 0.5 −1.755 ± 0.088 1.64 0.667 0.287 273
Fe I 5782.1093 3.0 3.0 −0.462 ± 0.065 5.06 1.250 0.332 2338
Cu I 5782.1670 1.5 0.5 −1.839 ± 0.042 1.64 0.667 0.287 273
( * )Cr I 5783.0642 1.0 1.0 −0.184 ± 0.025 3.32 2.000 0.288 1099
( * )Cr I 5783.8498 2.0 2.0 +0.074 ± 0.035 3.32 1.667 0.288 1098
( * )Fe I 5784.6580 3.0 4.0 −2.369 ± 0.031 3.40 1.875 0.244 795

Notes. From left to right: atomic element and ionization state, wavelength, total angular momentum quantum number of the lower Jl and upper Ju levels, the oscillator strength log(gf) and its standard deviation determined in this work, the excitation potential of the lower level χe, Landé g-factor, and the coefficients for collisional broadening (α and σ). The abundances were extracted from Asplund et al. (2009). Lines marked with a star (*) are used as the main lines in the inversions, the others are considered as blends in SIR. Also, a0 is the Bohr radius. Landé g-factors were computed using LS coupling.

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