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Cited article:

Computation of Non-Maxwellian Electron Excitation Rates for Ions of Astrophysical Interest: Fe xv – A Test Case

Elena Dzifčáková and Helen Mason
Solar Physics 247 (2) 301 (2008)
https://doi.org/10.1007/s11207-007-9106-3

Soft X‐Ray Emission Lines of Fexvin Solar Flare Observations and theChandraSpectrum of Capella

F. P. Keenan, J. J. Drake, S. Chung, et al.
The Astrophysical Journal 645 (1) 597 (2006)
https://doi.org/10.1086/502639

An investigation of Fe XV emission lines in solar flare spectra

F. P. Keenan, K. M. Aggarwal, D. S. Bloomfield, A. Z. Msezane and K. G. Widing
Astronomy & Astrophysics 449 (3) 1203 (2006)
https://doi.org/10.1051/0004-6361:20054028

Emission lines of Fe xv in spectra obtained with the Solar Extreme-Ultraviolet Research Telescope and Spectrograph

F. P. Keenan, K. M. Aggarwal, R. O. Milligan, et al.
Monthly Notices of the Royal Astronomical Society 356 (4) 1592 (2005)
https://doi.org/10.1111/j.1365-2966.2005.08637.x