REVISED AND EXTENDED ANALYSIS OF FIVE TIMES IONIZED XENON, Xe VI

M. GALLARDO, M. RAINERI, J. REYNA ALMANDOS; C. J. B. PAGAN, AND R. ABRAHÃO

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

IOP PUBLISHING LTD

Año: 2015 vol. 216 p. 11 - 25

0067-0049

A capillary discharge tube was used to record the Xe spectrum in the 400?5500Å region. A set of 243 lines of the Xe vi spectrum was observed, and 146 of them were classified for the first time. For all known lines, we calculated the weighted oscillator strengths (gf ) and weighted transition probabilities (gA) using the configuration interaction in a relativistic Hartree?Fock approach. The energy matrix was calculated using energy parameters adjusted to fit the experimental energy levels. Core polarization effects were taken into account in our calculations. Experimental energy values and calculated lifetimes are also presented for a set of 88 levels. From these levels, 32 were classified for the first time and 33 had their values revised. Our analysis of the 5s5p5d and 5s5p6s configurations was extended in order to clarify discrepancies among previous works.vi spectrum was observed, and 146 of them were classified for the first time. For all known lines, we calculated the weighted oscillator strengths (gf ) and weighted transition probabilities (gA) using the configuration interaction in a relativistic Hartree?Fock approach. The energy matrix was calculated using energy parameters adjusted to fit the experimental energy levels. Core polarization effects were taken into account in our calculations. Experimental energy values and calculated lifetimes are also presented for a set of 88 levels. From these levels, 32 were classified for the first time and 33 had their values revised. Our analysis of the 5s5p5d and 5s5p6s configurations was extended in order to clarify discrepancies among previous works.gf ) and weighted transition probabilities (gA) using the configuration interaction in a relativistic Hartree?Fock approach. The energy matrix was calculated using energy parameters adjusted to fit the experimental energy levels. Core polarization effects were taken into account in our calculations. Experimental energy values and calculated lifetimes are also presented for a set of 88 levels. From these levels, 32 were classified for the first time and 33 had their values revised. Our analysis of the 5s5p5d and 5s5p6s configurations was extended in order to clarify discrepancies among previous works.s5p5d and 5s5p6s configurations was extended in order to clarify discrepancies among previous works.