Indirect X-Ray Line-Formation Processes in Iron L-Shell Ions

By M. Gu. 2003

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CHIANTI—An Atomic Database for Emission Lines. VII. New Data for X-Rays and Other Improvements (2006, methodology): “Collision rates are obtained by summing the distorted-wave collision strengths calculated by Landi & Gu (2006a) at six values of the incident electron energy from threshold to high energies, with the resonant excitation collision rates by Gu (2003) for the n ¼ 3 complex.”
CHIANTI - an atomic database for emission lines. IX. Ionization rates, recombination rates, ionization equilibria for the elements hydrogen through zinc and updated atomic data (2009, methodology): “In this case the 6 parameter formula of Gu (2003b) was used.”
CHIANTI—An Atomic Database for Emission Lines. XV. Version 9, Improvements for the X-Ray Satellite Lines (2019, background): “The 1–160 transition was found to have an anomalously high value at the highest tabulated temperature that was traced to the original data-set of Gu (2003).”
CHIANTI—AN ATOMIC DATABASE FOR EMISSION LINES. XII. VERSION 7 OF THE DATABASE (2012, methodology): “Following the recommendations of Aggarwal et al. (2009), we included theoretical energy levels and A values from their “FAC1” calculation, carried out using the Flexible Atomic Code (FAC;- Gu 2003) on an atomic model which includes up to the n = 5 configuration.”
CHIANTI - An atomic database for Emission Lines. Version 8 (2015, methodology): “They replace those calculated with the DW approximation and the FAC code by Gu (2003).”