Non-LTE corrections derived from an updated Eu II model atom eliminate abundance discrepancies between the 4129 Å and 6645 Å lines in the Sun and metal-poor stars and are provided as a public grid for F-G-K stellar parameters.
Kochukhov, Astrophysics Source Code Library, record ascl:1805.015 (2018)
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Non-LTE corrections for determinations of europium abundances in F-G-K stars in a broad metallicity range
Non-LTE corrections derived from an updated Eu II model atom eliminate abundance discrepancies between the 4129 Å and 6645 Å lines in the Sun and metal-poor stars and are provided as a public grid for F-G-K stellar parameters.