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 research progresses on the investigations of atomic structure and collision dynamics
with highly charged ions based on the heavy ion storage rings and electron ion beam traps …

Aims. The goal of the CHIANTI atomic database is to provide a set of atomic data for the
interpretation of astrophysical spectra emitted by collisionally dominated, high temperature …

We present new computations of the equilibrium and nonequilibrium cooling efficiencies
and ionization states for low-density radiatively cooling gas containing the elements H, He …

Reliably interpreting spectra from electron-ionized cosmic plasmas requires accurate
ionization balance calculations for the plasma in question. However, much of the atomic …

We present a new version of the fully three-dimensional photoionization and dust radiative
transfer code, MOCASSIN, that uses a Monte Carlo approach for the transfer of radiation …

ABSTRACT The C ii $133.5\;\mathrm {nm} $ lines are important observables for the
NASA/SMEX mission Interface Region Imaging Spectrograph. To make three-dimensional …

We analyze and model the infrared spectrum of the Cassiopeia A supernova remnant with
the aim of determining the masses of various elements in the unshocked ejecta. In this way …

Dielectronic (DR) and radiative (RR) recombination rate coefficients for 19 phosphorous-like
ions, between S+ and W 59+, forming sulphur-like ions, have been calculated as part of the …