Stellar laboratories - IX. New Se v, Sr iv–vii, Te vi, and I vi oscillator strengths and the Se, Sr, Te, and I abundances in the hot white dwarfs G191−B2B and RE 0503−289

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Table 1

Statistics of the Se v, Sr iv–vii, Te vi, and I vi atomic levels and line transitions from Tables A.15–A.21.

Ion	Atomic levels	Lines	Super levels	Super lines

Se v	46	310	7	19
Sr iv	254	7578	7	21
Sr v	130	2022	7	19
Sr vi	22	70	7	10
Sr vii	19	46	7	10
Te vi	30	178	7	12
I vi	38	197	7	15

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