/ftp/cats/J/A%252bAS/102/269/.



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J/A+AS/102/269   Lab. and solar highly-excited levels of Fe I   (Nave+ 1993)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat
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drwxr-xr-x 18 cats archive 4096 Dec 12 14:24 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:56 [TAR file] -rw-r--r-- 1 cats archive 314 Jul 31 2001 .message -r--r--r-- 1 cats archive 5342 Jul 31 2001 ReadMe -r--r--r-- 1 cats archive 51346 Jul 31 2001 table1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+AS/102/269 Lab. and solar highly-excited levels of Fe I (Nave+ 1993) ================================================================================ Highly-excited levels of Fe I obtained from laboratory and solar Fourier transform and grating spectra. II. Laboratory and solar identifications NAVE G., JOHANSSON S. <Astron. Astrophys. Suppl. Ser. 102, 269 (1993)> =1993A&AS..102..269N ================================================================================ ADC_Keywords: Atomic physics ; Sun Keywords: atomic data - line: identification - infrared: general - ultraviolet: general Abstract: New identifications of about 2200 FeI lines between 170nm and 5mum (59000 to 2000 cm^-1^) due to highly-excited configurations are presented. These have been observed in hollow cathode lamps using Fourier transform and grating spectroscopy. About 1700 if the lines have been observed in the solar spectrum. A companion paper presents the experimental energy levels.

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