R-matrix atomic data support W III as the source of the 4.5 μm kilonova emission, yielding W III masses near 1.7e-4 solar masses for AT2017gfo and 9.4e-4 solar masses for AT2023vfi.
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Luminosity predictions for the first three ionisation stages of W, Pt and Au to probe potential sources of emission in kilonova
R-matrix atomic data support W III as the source of the 4.5 μm kilonova emission, yielding W III masses near 1.7e-4 solar masses for AT2017gfo and 9.4e-4 solar masses for AT2023vfi.