Stellar laboratories - X. New Cu IV–VII oscillator strengths and the first detection of copper and indium in hot white dwarfs

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Table 1

Statistics of the Cu IV - VII, atomic levels and line transitions from Tables A.13–A.16 and of In IV - VI compiled from the literature (Sect. 4).

Ion		Atomic levels	Lines	Super levels	Super lines
Cu	IV	297	8785	7	15
	V	247	5456	7	16
	VI	254	3797	7	9
	VII	217	2253
In	IV	231	564	7	15
	V	396	919	7	16
	VI	167	176	8	9

Notes. The super levels and lines are used in our model-atmosphere calculations.

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