/ftp/cats/vi/73



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VI/73    Atomic Spectral Lines Data OII, Mg, Al, S, Sc (NIST 1993)
The following files can be converted to FITS (extension .fit .fit.Z .fgz)
	lines.dat
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=VI/73
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Beginning of ReadMe : VI/73 Atomic Spectral Lines Data OII, Mg, Al, S, Sc (NIST 1993) ================================================================================ Selected Tables of Atomic Spectra (O II) Martin W.C., Kaufman V. <J. Phys. Chem. Ref. Data, in preparation (1992)> Wavelengths and Energy Level Classifications of Magnesium Spectra for All Stages of Ionization (Mg I through XII) Kaufman V., Martin W.C. <J. Phys. Chem. Ref. Data, Vol. 20, 83 (1991)> Wavelengths and Energy Level Classifications for the Spectra of Aluminum (Al I through Al XIII) Kaufman V., Martin W.C. <J. Phys. Chem. Ref. Data, Vol. 20, No. 5, p. 775 (1991)> Energy Levels of Sulfur, S I through S XVI Martin W.C., Zalubas R., Musgrove A. <J. Phys. Chem. Ref. Data, Vol. 19, 821 (1990)> Wavelength and Energy Level Classifications of Scandium Spectra for All Stages of Ionization Kaufman V., Sugar J. <J. Phys. Chem. Ref. Data, Vol. 17, 1679 (1988)> ================================================================================ ADC_Keywords: Atomic physics - 150 Keywords: NIST, Atomic Spectral Line Data Abstract: Atomic Spectral Lines Data O II, Mg I-XII, Al I-XIII, S I-XVI, Sc I-XXI. Using recent critical compilations of atomic energy levels, the authors calculate wavelengths (or wave numbers) from the differences of the energy levels. Results are given along with the observed values for all classified lines. Unless otherwise noted, the calculated values are in general more accurate than the observed values wherever the two values differ significantly. Some observed lines are classified as unresolved blends of two or more transitions. The calculated wavelength for each of the main components of such a blend is listed, or in some cases the calculated wavelength of the probable strongest component.