/ftp/cats/6/10



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VI/10              Semiempirical gf Values                       (Kurucz + 1975)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	data.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VI/10
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drwxr-xr-x 141 cats archive 4096 Sep 6 2023 [Up] drwxr-xr-x 2 cats archive 287 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 461 Dec 19 2022 .message -r--r--r-- 1 cats archive 3240 Mar 3 2005 ReadMe -rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 4879835 Aug 19 1996 data.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -rwxr-xr-x 1 cats archive 3217 Sep 14 2000 readme.adc
Beginning of ReadMe : VI/10 Semiempirical gf Values (Kurucz + 1975) ================================================================================ A Table of Semiempirical gf Values Kurucz R.L., Peytremann E. <SAO Spec. Report No. 362 (1975)> =1975SAOSR.362.....K ================================================================================ ADC_Keywords: Abundances; Atomic physics Abstract: This table of gf values for 265,587 atomic lines is selected from the line data used to calculate line-blanketed model atmospheres (Kurucz et al. 1974). The data are especially useful for line identification and spectral synthesis in solar and stellar spectra. Except for 10,100 lines taken from the literature, the gf values have been 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 were the first five or six stages of ionization for sequences up through nickel. Published gf values have been included for elements heavier than nickel. The tabulation is restricted to lines with wavelengths less than 10um.