Abstract
Calculations of the photoionization of the $4f$ and $5d$ subshells in the mercury isonuclear sequence have been performed within the framework of a Hartree-Slater central-field model. The results, obtained from the neutral to ${\mathrm{Hg}}^{33+}$, show that removal of outer-shell electrons have virtually no effect on inner-shell cross sections even for subshells with delayed maxima and/or Cooper minima. The general systematics of the variation of $4f$ and $5d$ cross sections in the Hg isonuclear sequence is discussed.
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