Abstract
The MCDF-EAL method has been applied to predict the wavelengths and radiative transitions rates for the w, x, y, z lines of helium-like ions from Ca to Cu (omitting Sc), and for the stronger satellites of the corresponding lithium-like and beryllium-like ions in the range λ=1.5–3 Å. Some comparisons are made of new data with other methods of calculation and, to a limited extent, with observations.

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