VALD: The Meeting Point of Data Producers and Data Users

Vienna Atomic Line Database (VALD) contains data on atomic and molecular energy levels and parameters of spectral lines required for stellar spectra analysis. Hundreds of millions of lines for fine spectral synthesis and for opacity calculations are collected in the present version of VALD (VALD3)....

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Main Authors: Tatiana Ryabchikova, Yury Pakhomov, Nikolai Piskunov
Format: Article
Language:English
Published: MDPI AG 2018-09-01
Series:Galaxies
Subjects:
Online Access:http://www.mdpi.com/2075-4434/6/3/93
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spelling doaj-33729bd670654c93a573b971ef947dcf2020-11-24T23:41:42ZengMDPI AGGalaxies2075-44342018-09-01639310.3390/galaxies6030093galaxies6030093VALD: The Meeting Point of Data Producers and Data UsersTatiana Ryabchikova0Yury Pakhomov1Nikolai Piskunov2Institute of Astronomy, Russian Academy of Sciences, 119017 Moscow, RussiaInstitute of Astronomy, Russian Academy of Sciences, 119017 Moscow, RussiaDepartment of Physics and Astronomy, Division of Astronomy and Space Physics, Uppsala University, 751 20 Uppsala, SwedenVienna Atomic Line Database (VALD) contains data on atomic and molecular energy levels and parameters of spectral lines required for stellar spectra analysis. Hundreds of millions of lines for fine spectral synthesis and for opacity calculations are collected in the present version of VALD (VALD3). Critical evaluation of the data and the diversity of extraction tools support the high popularity of VALD among users. The data model of VALD3 incorporates obligatory links to the bibliography making our database more attractive as a publishing platform for data producers. The VALD data quality and completeness are constantly improving allowing better reproduction of stellar spectra. To illustrate continuous evolution of the data content we present a comparative analysis of the recent experimental and theoretical atomic data for Fe-group elements, which will be included in the next VALD release. This release will also include a possibility for extracting the line data with full isotopic and hyperfine structures.http://www.mdpi.com/2075-4434/6/3/93stellar spectraatomic and molecular datadatabases
collection DOAJ
language English
format Article
sources DOAJ
author Tatiana Ryabchikova
Yury Pakhomov
Nikolai Piskunov
spellingShingle Tatiana Ryabchikova
Yury Pakhomov
Nikolai Piskunov
VALD: The Meeting Point of Data Producers and Data Users
Galaxies
stellar spectra
atomic and molecular data
databases
author_facet Tatiana Ryabchikova
Yury Pakhomov
Nikolai Piskunov
author_sort Tatiana Ryabchikova
title VALD: The Meeting Point of Data Producers and Data Users
title_short VALD: The Meeting Point of Data Producers and Data Users
title_full VALD: The Meeting Point of Data Producers and Data Users
title_fullStr VALD: The Meeting Point of Data Producers and Data Users
title_full_unstemmed VALD: The Meeting Point of Data Producers and Data Users
title_sort vald: the meeting point of data producers and data users
publisher MDPI AG
series Galaxies
issn 2075-4434
publishDate 2018-09-01
description Vienna Atomic Line Database (VALD) contains data on atomic and molecular energy levels and parameters of spectral lines required for stellar spectra analysis. Hundreds of millions of lines for fine spectral synthesis and for opacity calculations are collected in the present version of VALD (VALD3). Critical evaluation of the data and the diversity of extraction tools support the high popularity of VALD among users. The data model of VALD3 incorporates obligatory links to the bibliography making our database more attractive as a publishing platform for data producers. The VALD data quality and completeness are constantly improving allowing better reproduction of stellar spectra. To illustrate continuous evolution of the data content we present a comparative analysis of the recent experimental and theoretical atomic data for Fe-group elements, which will be included in the next VALD release. This release will also include a possibility for extracting the line data with full isotopic and hyperfine structures.
topic stellar spectra
atomic and molecular data
databases
url http://www.mdpi.com/2075-4434/6/3/93
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AT yurypakhomov valdthemeetingpointofdataproducersanddatausers
AT nikolaipiskunov valdthemeetingpointofdataproducersanddatausers
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