Grid/NLTE
A. M. Amarsi · Zenodo (CERN European Organization for Nuclear Research) · 2026
Non-LTE departure coefficients for late-type stars. For this version, see Ag I model atom and the 3D non-LTE solar silver abundance (Caliskan, Amarsi, Jönsson, Grevesse, and Sahoo, A&A, in press), and references therein. The methods were first presented in Non-LTE departure coefficients for large spectroscopic surveys (Amarsi et al., A&A, 2020, 642, A62).