Benchmarking Current Capabilities for the Generation of Excitation and Photoionisation Atomic Data
Autor: | Andrew Conroy, Connor Ballance, Francis P. Keenan, L. Fernández-Menchero, R. T. Smyth, M. Turkington, Catherine Ramsbottom |
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Jazyk: | angličtina |
Rok vydání: | 2018 |
Předmět: |
Computer science
lcsh:Astronomy Fe-peak elements atomic processes Astronomy and Astrophysics Benchmarking collisions 01 natural sciences astronomy_astrophysics Spectral line Computational physics lcsh:QB1-991 Quality (physics) R-matrix 0103 physical sciences atomic data Radiative transition Current (fluid) electron-impact excitation 010306 general physics 010303 astronomy & astrophysics photoionization Excitation Line (formation) Atomic data |
Zdroj: | Galaxies Volume 6 Issue 3 Galaxies, Vol 6, Iss 3, p 90 (2018) Ramsbottom, C, Ballance, C, Smyth, R, Conroy, A, Fernandez Menchero, L, Turkington, M & Keenan, F 2018, ' Benchmarking Current Capabilities for the Generation of Excitation and Photoionisation Atomic Data ', Galaxies, vol. 6, no. 3, pp. 1-11 . https://doi.org/10.3390/galaxies6030090 |
ISSN: | 2075-4434 |
DOI: | 10.3390/galaxies6030090 |
Popis: | The spectra currently emerging from modern ground- and space-based astronomical instruments are of exceptionally high quality and resolution. To meaningfully analyse these spectra, researchers utilise complex modelling codes to replicate the observations. The main inputs to these codes are atomic data such as excitation and photoionisation cross sections, as well as radiative transition probabilities, energy levels, and line strengths. In this publication, the current capabilities of the numerical methods and computer packages used in the generation of these data are discussed. Particular emphasis is given to Fe-peak species and the heavy systems of tungsten and molybdenum. Some of the results presented to highlight certain issues and/or advances have already been published in the literature, while other sections present new recently evaluated atomic data for the first time. |
Databáze: | OpenAIRE |
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