Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-25T03:29:46.111Z Has data issue: false hasContentIssue false

The Belgian Repository of fundamental Atomic data and Stellar Spectra (BRASS)

Published online by Cambridge University Press:  12 October 2020

M. Laverick
Affiliation:
Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, box 2401, 3001 Leuven, Belgium Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussels, Belgium email: [email protected]
A. Lobel
Affiliation:
Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussels, Belgium email: [email protected]
P. Royer
Affiliation:
Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, box 2401, 3001 Leuven, Belgium
T. Merle
Affiliation:
Institut d’Astronomie et d’Astrophysique, Université Libre de Bruxelles, Av. Franklin Roosevelt 50, CP 226, 1050 Brussels, Belgium
C. Martayan
Affiliation:
European Organisation for Astronomical Research in the Southern Hemisphere, Alonso de Córdova 3107, Vitacura, 19001 Casilla, Santiago de Chile, Chile
P. van Hoof
Affiliation:
Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussels, Belgium email: [email protected]
M. Van der Swaelmen
Affiliation:
Institut d’Astronomie et d’Astrophysique, Université Libre de Bruxelles, Av. Franklin Roosevelt 50, CP 226, 1050 Brussels, Belgium
M. David
Affiliation:
Onderzoeksgroep Toegepaste Wiskunde, Universiteit Antwerpen, Middelheimlaan 1, 2020 Antwerp, Belgium
H. Hensberge
Affiliation:
Royal Observatory of Belgium, Ringlaan 3, B-1180 Brussels, Belgium email: [email protected]
E. Thienpont
Affiliation:
Vereniging voor Sterrenkunde, Kapellebaan 56, 2811 Leest, Belgium
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Belgian Repository of fundamental Atomic data and Stellar Spectra (BRASS) aims to provide one of the largest systematic and homogeneous quality assessment to date of literature atomic data required for stellar spectroscopy. By comparing state-of-the-art synthetic spectrum calculations with extremely high-quality observed benchmark spectra, we have critically evaluated fundamental atomic data, such as line wavelengths and oscillator strengths, for thousands of astrophysically-relevant transitions found in the literature and across several major atomic data repositories. These proceedings provide a short overview of the BRASS project to date, highlighting our recent efforts to investigate and quality-assess the atomic literature data pertaining to over a thousand atomic transitions present in FGK-type stellar spectra. BRASS provides all quality assessed data, theoretical spectra, and observed spectra in a new interactive database under development at brass.sdf.org.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

Dubernet, M. L., Antony, B. K., Ba, Y. A., et al. 2016, J. phys. B: At. Mol. Opt. Phys., 49, 074003CrossRefGoogle Scholar
Dekker, H. et al. 2000, SPIE, 4008, 534Google Scholar
Kramida, A., Ralchenko, Y., Reader, J., & NIST ASD Team 2018. NIST Atomic Spectra Database (version 5.6.1) [Online]. Available: http://physics.nist.gov/asdGoogle Scholar
Lobel, A., Royer, P., Martayan, C., et al. 2017, Can. J. Phys. 2017, 95, 833CrossRefGoogle Scholar
Laverick, M., Lobel, A., Merle, T., et al. 2018, A&A, 612, A60Google Scholar
Laverick, M., Lobel, A., Royer, P., et al. 2019, A&A, 624, A60Google Scholar
Raskin, G., Van Winckel, H., Hensberge, H., et al. 2011, A&A, 526, A69Google Scholar
Ryabchikova, T., Piskunov, N., Kurucz, R., et al. 2015, PhysS., 90, 5Google Scholar