Published 2026
| Version v8
Dataset
Open
Grid/NLTE
Description
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).
Files
README.md
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