Published 2026 | Version v8
Dataset Open

Grid/NLTE

Authors/Creators

  • 1. ROR icon Uppsala University

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).

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