1988
DOI: 10.1016/0368-2048(88)85020-5
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Electron shake-up and correlation satellites and continuum shake-off distributions in X-Ray photoelectron spectra of the rare gas atoms

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Cited by 281 publications
(217 citation statements)
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“…Furthermore, the present spectrum has been measured at a photon energy much closer to the Kr 3d threshold compared to the photon energy used by Eriksson et al [29,30]. Hence, some of the differences may also be an effect of conjugate shake-up [29,30]. Figure 9 shows the spectra of the slowest electron of the coincidence events corresponding to group III in the same way that Fig.…”
Section: S)mentioning
confidence: 60%
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“…Furthermore, the present spectrum has been measured at a photon energy much closer to the Kr 3d threshold compared to the photon energy used by Eriksson et al [29,30]. Hence, some of the differences may also be an effect of conjugate shake-up [29,30]. Figure 9 shows the spectra of the slowest electron of the coincidence events corresponding to group III in the same way that Fig.…”
Section: S)mentioning
confidence: 60%
“…The spectrum is plotted on a binding energy scale relative to the 3d 9 to the Al Kα-excited Kr 3d 9 shake-up photoelectron spectrum of Eriksson et al [29] (also discussed in Ref. [30]), which is plotted in the lower part of this figure. Generally, the spectra are similar to each other, but there are differences in the relative intensities.…”
Section: S)mentioning
confidence: 99%
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“…The obtained coefficients ͉C 2s ͉ 2 Ϸ 0.8 and ͉C 2p ͉ 2 Ϸ 0.2 seem to be realistic when compared with another indicator of the strength of the intershell correlation: the spectroscopic factor of the 2s 2 shell in Ne. Experimental values of the spectroscopic factor are 0.91 in photoionization [37] and 0.85 in electron impact ionization [38]. A similar amount of the 2s /2p mixing is required to reproduce correctly the 2s ionization potential [39].…”
Section: ͑1͒mentioning
confidence: 99%