Stellar laboratories - VIII. New Zr iv–vii, Xe iv–v, and Xe vii oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs G191−B2B and RE 0503−289

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Table 5

Identified Xe lines in the UV spectrum of RE 0503−289.

		Wavelength/Å	Comment

Xe	vi	915.163	weak
		928.366^a
		929.131^b
		967.550^a
		970.177	weak
		1017.270^b
		1080.080^a
		1091.630^a
		1101.940^a
		1110.450	weak
		1136.410^a
		1179.540^a
		1181.390^a
		1181.540	blend with Xe viλ 1181.390 Å
		1184.390^a	uncertain
		1228.450
		1280.270
		1298.910^b
		1439.250
Xe	vii	995.516^a
		1077.120^a
		1243.565

Notes. The wavelengths correspond to those given in Gallardo et al. (2015) and in Table B.7 for Xe vi and Xe vii, respectively.

^(a)

Identified by Werner et al. (2012b);

^(b)

identified by Rauch et al. (2015a).

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