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By Michael Dance, Ethan Palay, Sultana N. Nahar and Anil K. Pradhan. Monthly Notices of the Royal Astronomical Society 435(2), 1576–1581; published online 26 August 2013.

Cited passages: section 2.3, equations (3)–(4), Maxwellian effective collision strength and excitation coefficient; section 3.1, low-energy resonance structure and its effect on thermal rates. The published title encloses Ne V in square brackets to denote forbidden lines.

Sultana N. Nahar co-investigated atomic collision data for four-times-ionized neon. Resolving near-threshold resonances changed the effective collision strengths needed to interpret temperature-sensitive infrared and optical line ratios.^[ref]