One of the most enduring and intensively studied problems of x-ray astronomy is the
disagreement of state-of-the art theory and observations for the intensity ratio of two Fe XVII …

For more than 40 years, most astrophysical observations and laboratory studies of two key
soft x-ray diagnostic 2 p-3 d transitions, 3 C and 3 D, in Fe XVII ions found oscillator strength …

There has been a growing request from the X-ray astronomy community for a quantitative
estimate of systematic uncertainties originating from the atomic data used in plasma codes …

The Hitomi results for the Perseus cluster have shown that accurate atomic models are
essential to the success of X-ray spectroscopic missions and just as important as the store of …

We report measurements of electron-impact excitation cross sections for the strong K-shell
n= 2→ 1 transitions in S xv, using the LLNL EBIT-I electron beam ion trap, two crystal …

The rate coefficients for dielectronic recombination and electron-impact excitation processes
with H-like to Be-like silicon ions (Si 13+-Si 10+) are calculated using relativistic distorted …

The resonance 3C ([(2p^ 5) _1/23d_3/2] _J= 1→[2p^ 6] _J= 0) to intercombination 3D ([(2p^
5) _3/23d_5/2] _J= 1→[2p^ 6] _J= 0) line intensity ratio of neonlike ions has been studied …

The cross sections and rate coefficients for dielectronic recombination (DR) and electron-
impact excitation processes of helium-like isoelectronic sequence are systematically …

Comprehensive Laboratory Measurements Resolving the LMM Dielectronic Recombination
Satellite Lines in Ne-like Fe xvii Ions - IOPscience This site uses cookies. By continuing to use …

We used the monochromatic soft-x-ray beamline P04 at the synchrotron-radiation facility
PETRA III to resonantly excite the strongest 2 p-3 d transitions in neonlike Ni xix ions,[2 p 6] …