A new 3D non-LTE Ag I model atom yields a solar silver abundance of 1.15 ± 0.08, raising the prior value by 0.19 dex and shrinking the meteoritic offset to 0.06 dex.
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3D NLTE sodium abundance corrections relative to 1D LTE are typically negative and larger for saturated lines in giants, reaching -0.7 dex, with a public grid released for use.
PySME v1.0 introduces a revised line-selection framework and updated hydrogen-line physics to enable scalable, high-precision stellar spectrum modeling for large surveys.
citing papers explorer
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Ag I model atom and the 3D non-LTE solar silver abundance
A new 3D non-LTE Ag I model atom yields a solar silver abundance of 1.15 ± 0.08, raising the prior value by 0.19 dex and shrinking the meteoritic offset to 0.06 dex.
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3D NLTE Sodium abundances in late-type stars. Abundance corrections and synthetic spectra
3D NLTE sodium abundance corrections relative to 1D LTE are typically negative and larger for saturated lines in giants, reaching -0.7 dex, with a public grid released for use.
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PySME v1.0: improved modelling of stellar spectra for survey-scale applications
PySME v1.0 introduces a revised line-selection framework and updated hydrogen-line physics to enable scalable, high-precision stellar spectrum modeling for large surveys.