Abstract
Our studies at Lawrence Livermore National Laboratory (LLNL) of lanthanide and actinide spectra with the Kitt Peak National Solar Observatory (KPNO) 1 m Fourier transform spectrometer (FTS) have included both intensity for branching ratio (BR) determination (transition probability) and frequency observations using hollow cathodes (HC) and/or electrodeless discharge lamps (EDLs) as sources. The elements we have observed, the purpose of the study and the sources used are given in Table 1.
© 1992 Optical Society of America
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