Abstract
Considerable extensions of the 4d-absorption spectrum of Ag I have resulted from improvements in experimental technique. All the allowed transitions to 4d
9
5s 5p have now been accounted for, and the weak
n
f series converging on the 4d
9
5s limits have been observed. Double excitations involving the 4d subshell have been detected. A detailed analysis is attempted by comparison with
ab initio
Hartree–Fock calculations.
Reference3 articles.
1. B ro w n C. M. & G in te r M. L . 1977
2. Astrophys;J .,1970
3. C o n n e ra d e J . P . 1978 Contemp. P hys. 19 415. J . opt.Soc.
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