A table of semiempirical gf values. Part 1: Wavelengths: 5.2682 NM to 272.3380 NM

Astronomy and Astrophysics – Astronomy

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Atmospheric Models, Line Spectra, Solar Spectra, Stellar Spectra, Astronomical Spectroscopy, Tables (Data), Wave Functions, Wavelengths

Scientific paper

The gf values for 265,587 atomic lines selected from the line data used to calculate line-blanketed model atmospheres are tabulated. These data are especially useful for line identification and spectral synthesis in solar and stellar spectra. The gf values are calculated semiempirically by using scaled Thomas-Fermi-Dirac radial wavefunctions and eigenvectors found through least-squares fits to observed energy levels. Included in the calculation are the first five or six stages of ionization for sequences up through nickel. Published gf values are included for elements heavier than nickel. The tabulation is restricted to lines with wavelengths less than 10 micrometers.

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