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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Volume 606 (October 2017)

A&A, 606 (2017) A105

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Table A.13

Comparison between available experimental and calculated energy levels in Te vi.

E _exp ^a	E _calc ^b	ΔE	J	Leading components (in %) in LS coupling^c

Even parity
0.0	0	0	0.5	99 4d¹⁰5s ²S
238 087.6	238 088	0	1.5	99 4d¹⁰5d ²D
239 736.2	239 736	0	2.5	99 4d¹⁰5d ²D
278 436.2	278 436	0	0.5	100 4d¹⁰6s ²S
480 834.0	480 935	−101	2.5	49 4d⁹5p²⁴D + 13 4d⁹5p²⁴F + 9 4d⁹5p²⁴P
488 295.0	488 184	111	1.5	64 4d⁹5p²⁴D + 10 4d⁹5p²²D + 9 4d⁹5p²⁴F
489 538.0	489 652	−114	0.5	56 4d⁹5p²²S + 19 4d⁹5p²²P + 8 4d⁹5p²⁴D
490 499.0	490 411	88	1.5	59 4d⁹5p²²P + 12 4d⁹5p²²P + 8 4d⁹5s5d ²P
498 636.0	498 676	−40	1.5	47 4d⁹5p²²D + 42 4d⁹5p²⁴F + 5 4d⁹5p²²P
501 898.0	501 788	110	0.5	55 4d⁹5p²²P + 15 4d⁹5p²⁴P + 8 4d⁹5s5d ²P
503 128.0	503 155	−27	1.5	42 4d⁹5p²⁴F + 31 4d⁹5p²²D + 5 4d⁹5p²⁴P
504 027.0	503 990	37	2.5	32 4d⁹5p²⁴F + 24 4d⁹5p²⁴P + 19 4d⁹5p²²F
506 535.0	506 525	10	1.5	49 4d⁹5p²²D + 34 4d⁹5p²⁴P + 8 4d⁹5s5d ²D
510 691.0	510 671	20	2.5	52 4d⁹5p²²D + 30 4d⁹5p²²D + 7 4d⁹5s5d ²D
511 382.0	511 487	−105	0.5	86 4d⁹5p²²P + 6 4d⁹5p²²S
513 098.0	512 913	185	1.5	53 4d⁹5p²²P + 19 4d⁹5p²²P + 8 4d⁹5p²²D
517 679.0	517 850	−171	2.5	43 4d⁹5p²²F + 13 4d⁹5p²²D + 10 4d⁹5p²²F
Odd parity
93 334.6	93 335	0	0.5	99 4d¹⁰5p ²P
105 150.2	105 150	0	1.5	99 4d¹⁰5p ²P
314 198.4	314 198	0	0.5	100 4d¹⁰6p ²P
318 601.4	318 601	0	1.5	100 4d¹⁰6p ²P
376 310.0	376 297	13	1.5	58 4d⁹5s5p ⁴P + 18 4d⁹5s5p ⁴D + 12 4d⁹5s5p ²P
385 045.0	385 062	−17	0.5	75 4d⁹5s5p ⁴P + 13 4d⁹5s5p ⁴D + 11 4d⁹5s5p ²P
388 165.0	388 165	0	1.5	44 4d⁹5s5p ²D + 19 4d⁹5s5p ⁴P + 14 4d⁹5s5p ²P
392 650.0	392 682	−32	1.5	56 4d⁹5s5p ²P + 22 4d⁹5s5p ⁴D + 10 4d⁹5s5p ²P
393 730.0	393 708	22	0.5	63 4d⁹5s5p ²P + 23 4d⁹5s5p ²P + 7 4d⁹5s5p ⁴D
400 015.0	400 008	7	1.5	52 4d⁹5s5p ⁴D + 20 4d⁹5s5p ²D + 10 4d⁹5s5p ⁴P
411 220.0	411 227	−7	1.5	60 4d⁹5s5p ²P + 32 4d¹⁰7p ²P
422 875.0	422 864	11	0.5	75 4d⁹5s5p ²P + 21 4d⁹5s5p ²P

Notes. Energies are given in cm^-1.

^(a)

From Crooker & Joshi (1964), Dunne & O’Sullivan (1992), and Ryabtsev et al. (2007).

^(b)

This work.

^(c)

Only the first three components larger than 5% are given.

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