Atomic data for x-ray astrophysics

TR Kallman, P Palmeri - Reviews of Modern Physics, 2007 - APS
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 …

Updated atomic data and calculations for X-ray spectroscopy

AR Foster, L Ji, RK Smith… - The Astrophysical …, 2012 - iopscience.iop.org
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 …

CHIANTI—an atomic database for emission lines. VII. New data for X-rays and other improvements

E Landi, G Del Zanna, PR Young… - The Astrophysical …, 2006 - iopscience.iop.org
The CHIANTI atomic database contains atomic energy levels, wavelengths, radiative
transition probabilities, and collisional excitation data for a large number of ions of …

Photoionization modeling and the K lines of iron

TR Kallman, P Palmeri, MA Bautista… - The Astrophysical …, 2004 - iopscience.iop.org
We calculate the efficiency of iron K line emission and iron K absorption in photoionized
models using a new set of atomic data. These data are more comprehensive than those …

Energy levels, radiative rates, and electron impact excitation rates for transitions in Li-like ions with 12≤ Z≤ 20

KM Aggarwal, FP Keenan - Atomic Data and Nuclear Data Tables, 2013 - Elsevier
We report calculations of energy levels, radiative rates, and electron impact excitation rates
for transitions in Li-like ions with 12≤ Z≤ 20. The grasp (general-purpose relativistic atomic …

Atomic data for the K-vacancy states of Fe XXIV

MA Bautista, C Mendoza, TR Kallman… - Astronomy & …, 2003 - aanda.org
As part of a project to compute atomic data for the spectral modeling of iron K lines, we
report calculations and comparisons of atomic data for K-vacancy states in Fe xxiv. The data …

Spectroscopic diagnostics of the non-Maxwellian κ-distributions using SDO/EVE observations of the 2012 March 7 X-class flare

E Dzifčáková, A Zemanová, J Dudík… - The Astrophysical …, 2018 - iopscience.iop.org
Spectroscopic observations made by the Extreme Ultraviolet Variability Experiment (EVE) on
board the Solar Dynamics Observatory (SDO) during the 2012 March 7 X5. 4-class flare …

An absolute sensitivity calibration of the JET VUV SPRED spectrometer

KD Lawson, IH Coffey, J Zacks, MF Stamp… - Journal of …, 2009 - iopscience.iop.org
The determination of a good relative and absolute sensitivity calibration for wideband VUV
spectrometers is challenging. On JET, the possible T and Be contamination of the VUV …

Energy levels, radiative rates and electron impact excitation rates for transitions in He-like Cl XVI, K XVIII, Ca XIX and Sc XX

KM Aggarwal, FP Keenan - Physica Scripta, 2012 - iopscience.iop.org
We report calculations of energy levels, radiative rates and electron impact excitation cross
sections and rates for transitions in He-like Cl XVI, K XVIII, Ca XIX and Sc XX. The GRASP …

Dynamics and radiation of young type-Ia supernova remnants: Important physical processes

EI Sorokina, SI Blinnikov, DI Kosenko, P Lundqvist - Astronomy Letters, 2004 - Springer
We analyze the physical processes that should be taken into account when modeling young
type-Ia supernova remnants (SNRs) with ages of several hundred years in which forward …