X-ray and ultraviolet (UV) observations of the outer solar atmosphere have been used for
many decades to measure the fundamental parameters of the solar plasma. This review …

The available atomic data used for interpreting and modeling x-ray observations are
reviewed. The applications for these data can be divided into several levels of detail …

We describe the latest release of AtomDB, version 2.0. 2, a database of atomic data and a
plasma modeling code with a focus on X-ray astronomy. This release includes several major …

The CHIANTI spectral code consists of an atomic database and a suite of computer
programs to calculate the optically thin spectrum of astrophysical objects and carry out …

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 …

Context. The interstellar and intra-cluster medium (ICM) in giant elliptical galaxies and
clusters of galaxies is often assumed to be in hydrostatic equilibrium. Numerical simulations …

The Hitomi results on the Perseus cluster have led to improvements in our knowledge of
atomic physics that are crucial for the precise diagnostic of hot astrophysical plasma …

The current design plans for the International Thermonuclear Experimental Reactor (ITER)
call for tungsten to be employed for certain plasma facing components in the divertor region …

An emerging theme in modern astrophysics is the connection between astronomical
observations and the underlying physical phenomena that drive our cosmos. Both the …