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FW96 | J. R. Fuhr and W. L. Wiese, NIST Atomic Transition Probability Tables, CRC Handbook of Chemistry & Physics, 77th Edition, D. R. Lide, Ed., CRC Press, Inc., Boca Raton, FL (1996). |
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KM91a | V. Kaufman and W. C. Martin, J. Phys. Chem. Ref. Data 20, 83 (1991). We have quoted Ritz-calculated wavelengths for most Mg II lines from this compilation. These values are much more accurate than the directly measured wavelengths in the region below 2000 Å. |
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M03 | D. C. Morton, Astrophys. J. Suppl. Ser. 149, 205 (2003). |
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MZ80 | W. C. Martin and R. Zalubas, J. Phys. Chem. Ref. Data 9, 1 (1980). |
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PTW98 | J. C. Pickering, A. P. Thorne, and J. K. Webb, Mon. Not. R. Astron Soc. 300, 131 (1998). High-accuracy measurements of Mg I and Mg II resonant lines [PTW98], quoted here, give improved values of 35051.277(1) cm-1 for the Mg I 3s3p 1P° level and 35669.298(2) and 35760.848(2) cm-1 for the Mg II 3p 2P° levels. We have retained the less accurate values from [MZ80] for these levels for consistency with the values of other levels in the tables. |
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WSM69 | W. L. Wiese, M. W. Smith and B. M. Miles, Natl. Stand. Ref. Data Ser., Natl. Bur. Stand. (U.S.) 22 (1969). |
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