Abstract

The Belgian repository of fundamental atomic data and stellar spectra (BRASS) aims to provide the largest systematic and homogeneous quality assessment to-date of input atomic data required for stellar spectral synthesis. In addition to quality-assessed atomic data, BRASS shall also provide of a range of extremely high-quality benchmark stellar spectra spanning late B-type stars to early K-type stars. In this paper, we summarise the project’s progress and available results to-date. We provide a brief comparison between our results and the BRASS project’s compiled and cross-matched atomic literature, with the goal of providing useful feedback to the atomic community on which methods may produce more reliable and accurate atomic data. We hope that the examples presented here stimulate further investigation by the atomic physics community.

Highlights

  • Methods for Producing Atomic DataMike Laverick 1,2, *, Alex Lobel 2 , Pierre Royer 2 , Christophe Martayan 3 , Thibault Merle 4 , Peter A

  • The Belgian repository of fundamental atomic data and stellar spectra (BRASS) aims to take the first, crucial steps towards constraining and removing systematic input errors from quantitative stellar spectroscopy [1]

  • We summarise the status of the BRASS project to-date and we discuss a number of data-products already available to the astronomy and atomic physics communities

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Summary

Methods for Producing Atomic Data

Mike Laverick 1,2, *, Alex Lobel 2 , Pierre Royer 2 , Christophe Martayan 3 , Thibault Merle 4 , Peter A. M. van Hoof 2 , Mathieu Van de Swaelmen 4 , Marc David 5 , Herman Hensberge 2 and Emmanuel Thienpont 6. Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, P.O. Box 2401, 3001 Leuven, Belgium

Introduction
Cross-Matched Literature
High-Quality Stellar Spectra
Interactive Online Viewing
Quality-Assessed Atomic Data
Comparisons Between the BRASS Results and Previously Retrieved Literature
Findings
Summary and Future Plans
Full Text
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