The Belgian repository of fundamental atomic data and stellar spectra (BRASS) aims to critically evaluate atomic data, from publicly available repositories, by comparing state-of-the-art synthetic spectra against high-quality benchmark stellar spectra. In preparation for our assessment we have cross-matched atomic line transitions from several different databases. Our investigation revealed significant updates in log(gf) values, sometimes as large as 2-4 dex, that fully justify the need for systematic quality assessments of the atomic data. We have also investigated the spectral line blending of an initial subset of 2647 atomic lines using spectral synthesis calculations, for the spectral types BAFGK.SCOPUS: cp.jinfo:eu-repo/semantics/publi...
Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-...
Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-...
Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-...
BRASS is an international networking project of the Federal Government of Belgium for the developmen...
Context. Fundamental atomic parameters, such as oscillator strengths, play a key role in modelling a...
BRASS is an international networking project of the Federal Government of Belgium for the developmen...
BRASS is an international networking project of the Federal Government of Belgium for the developmen...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
The Belgian repository of fundamental atomic data and stellar spectra (BRASS) aims to provide the la...
The Belgian repository of fundamental atomic data and stellar spectra (BRASS) aims to provide the la...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
© 2019 ESO. Context. Fundamental atomic transition parameters, such as oscillator strengths and rest...
Accurate atomic transition data are crucial input parameters for the modelling of stars. The fundame...
11th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Labor...
Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-...
Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-...
Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-...
BRASS is an international networking project of the Federal Government of Belgium for the developmen...
Context. Fundamental atomic parameters, such as oscillator strengths, play a key role in modelling a...
BRASS is an international networking project of the Federal Government of Belgium for the developmen...
BRASS is an international networking project of the Federal Government of Belgium for the developmen...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
The Belgian repository of fundamental atomic data and stellar spectra (BRASS) aims to provide the la...
The Belgian repository of fundamental atomic data and stellar spectra (BRASS) aims to provide the la...
Context. Fundamental atomic transition parameters, such as oscillator strengths and rest wavelengths...
© 2019 ESO. Context. Fundamental atomic transition parameters, such as oscillator strengths and rest...
Accurate atomic transition data are crucial input parameters for the modelling of stars. The fundame...
11th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Labor...
Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-...
Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-...
Context. We describe the atomic and molecular data that were used for the abundance analyses of FGK-...