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Fully relativistic many-body perturbation energies, transition properties, and lifetimes of lithium-like iron Fe XXIV
Shuang 双 Li 李, Min 敏 Zhao 赵, Guo-Qing 国庆 Liu 刘, Chang-Bao 昌宝 Hu 胡 and Guo-Zhu 国柱 Pan 潘 Chinese Physics B 32(10) 103101 (2023) https://doi.org/10.1088/1674-1056/acef01
Optical Excitation of Ultra‐Relativistic Partially Stripped Ions
NIST program of spectroscopic data for light elements of fusion interest
Joseph Reader, Alexander Kramida, Yuri Ralchenko, Wolfgang Wiese and Jeffrey Fuhr Journal of Physics: Conference Series 576 012007 (2015) https://doi.org/10.1088/1742-6596/576/1/012007
Fine Structure Calculations of Atomic Data for Ar XVI
Comparative analysis and variability of the Jovian X-ray spectra detected by the Chandra and XMM-Newton observatories
Yawei Hui, David R. Schultz, Vasili A. Kharchenko, et al. Journal of Geophysical Research: Space Physics 115(A7) (2010) https://doi.org/10.1029/2009JA014854
Energy levels, radiative rates and electron impact excitation rates for transitions in Li-like N V, F VII, Ne VIII and Na IX
Electron‐Ion Recombination Rate Coefficients and Photoionization Cross Sections for Astrophysically Abundant Elements. XII. Na
ix
, Na
x
, Mg
x
, and Mg
xi
for Ultraviolet and X‐Ray Modeling
Electron‐Ion Recombination Rate Coefficients and Photoionization Cross Sections for Astrophysically Abundant Elements. XI. N
v
–
vi
and F
vii
–
viii
for Ultraviolet and X‐Ray Modeling
Electron‐Ion Recombination Rate Coefficients and Photoionization Cross Sections for Astrophysically Abundant Elements. X. Ne
viii
and Ne
ix
for Ultraviolet and X‐Ray Modeling
Sultana N. Nahar and Anil K. Pradhan The Astrophysical Journal Supplement Series 162(2) 417 (2006) https://doi.org/10.1086/498453
Excitation Energies of 1
s
2
ns
(6 $\leq$
n
$\leq$ 9) States for Lithium-Like Systems from
Z
=11 to 20
Electron‐Ion Recombination Rate Coefficients and Photoionization Cross Sections for Astrophysically Abundant Elements. IX. Ni
xxvi
and Ni
xxvii
for Ultraviolet and X‐Ray Modeling