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Ref. ID | | | |
Reference | |
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BGKZ82 | E. Biémont, M. Grevesse, M. Kwiatowski, and P. Zimmerman, Astron. Astrophys. 108, 127 (1982). |
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CHR88a | C. L. Callender, P. A. Hackett, and D. M. Rayner, J. Opt. Soc. Am. B 5, 614 (1988). |
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ELLW98 | R. Engelman, Jr., U. Litzén, H. Lundberg, and J.-F. Wyart, Phys. Scr. 57, 345 (1998). |
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LLJ94 | H. Lundberg, U. Litzén, and S. Johansson, Phys. Scr. 50, 110 (1994). |
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LLTL01 | U. Litzén, H. Lundberg, W.-U. L. Tchang-Brillet, F. Launay, and R. Engleman, Jr., Phys. Scr. 64, 63 (2001). The leading eigenvector percentages given for the 4d85p levels indicate that no meaningful LS-coupling names exist for some levels. We have used numerical names for several such levels. |
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M00 | D. C. Morton, Astrophys. J. Suppl. Ser. 130, 403 (2000). |
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M58 | C. E. Moore, Atomic Energy Levels, Natl. Bur. Stand. (U.S.) Circ. 467. Vol. III (1958); reprinted as Natl. Stand. Ref. Data Ser., Natl. Bur. Stand. (U.S.) 35 (1971). |
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Q96 | P. Quinet, Phys. Scr. 54, 483 (1996). |
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