References

[DereDelZannaYoung+19]

K. P. Dere, G. Del Zanna, P. R. Young, E. Landi, and R. S. Sutherland. CHIANTI—An Atomic Database for Emission Lines. XV. Version 9, Improvements for the X-Ray Satellite Lines. Astrophysical Journal, Supplement, 241(2):22, April 2019. arXiv:1902.05019, doi:10.3847/1538-4365/ab05cf.

[DereLandiMason+97]

K. P. Dere, E. Landi, H. E. Mason, B. C. Monsignori Fossi, and P. R. Young. CHIANTI - an atomic database for emission lines. Astronomy & Astrophysics, Supplement, 125:149–173, October 1997. doi:10.1051/aas:1997368.

[LongKnigge02]

Knox S. Long and Christian Knigge. Modeling the Spectral Signatures of Accretion Disk Winds: A New Monte Carlo Approach. Astrophysical Journal, 579(2):725–740, November 2002. arXiv:astro-ph/0208011, doi:10.1086/342879.

[PrzybillaButler04]

Norbert Przybilla and Keith Butler. Non-LTE Line Formation for Hydrogen Revisited. Astrophysical Journal, 609(2):1181–1191, July 2004. arXiv:astro-ph/0406458, doi:10.1086/421316.