Grid/NLTE
Abstract
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).
Fields of Study & Subjects
Distributed and Parallel Computing Systems
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 1 January 2026
- Language
- EN
- Document type
- Dataset