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 present version 8 of the CHIANTI database. This version includes a large amount of new
data and ions, which represent a significant improvement in the soft X-ray, extreme UV …

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 …

We present version 10 of the CHIANTI package. In this release, we provide updated atomic
models for several helium-like ions and for all the ions of the beryllium, carbon, and …

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 …

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 …

Spectroscopy enables the precise study of astronomical objects and phenomena. Bridging
the gap between physics and astronomy, this is the first integrated graduate-level textbook …

Abstract The Hitomi Soft X-ray Spectrometer spectrum of the Perseus cluster, with∼ 5 eV
resolution in the 2–9 keV band, offers an unprecedented benchmark of the atomic modeling …

Plasma models built on extensive atomic data are essential to interpreting observed cosmic
spectra. H-like Lyman series and He-like triplets observable in the X-ray band are powerful …