Repository details

STARK-B

⚠ Caution: This entry is annotated as "Offline: 2025-01". If you believe this is incorrect, please submit a change request.
Name of repository
STARK-B
Repository URL
https://stark-b.obspm.fr/
Subject(s)
Description
<<<!!!<<< This repository is no longer available. >>>!!!>>>
Contact(s)
  • administrative: sylvie.sahal-brechot@obspm.fr
  • administrative: https://stark-b.obspm.fr/index.php/contact
  • administrative: mdimitrijevic@aob.bg.ac.rs
  • administrative: nbennessib@ksu.edu.sa
  • administrative: nicolas.moreau@obspm.fr
Keyword(s)
Persistent identifier(s) of the repository
Repository type(s)
  • disciplinary
Mission statement for designated community
https://stark-b.obspm.fr/index.php/introduction
Research data repository language(s)
  • English
Data and/or service provider
  • dataProvider

Dates

Offline
2025-01

Institutions (2)

Institution name
Astronomical Observatory of Belgrade
Additional name(s)
  • AOB
  • Astronomskoj opservatoriji u Beogradu
Institution identifier(s)
Country
Serbia
Type(s) of responsibility
  • general
  • technical
  • funding
Type of institution
non-profit
Institution name
Observatoire de Paris
Additional name(s)
  • l’Observatoire de Paris
  • Paris Observatory
Institution identifier(s)
Country
France
Type(s) of responsibility
  • general
  • funding
Type of institution
non-profit

Policies (1)

Policy name
Introduction

Database access

Type of access to research data repository
open

Data access (1)

Type of access to data
open

Data licenses (1)

Data license
Copyrights

Data upload (1)

Type of data upload
closed
Persistent identifier system(s)
  • none
Name of the repository software
  • other
Versioning
yes
Enhanced publication
yes

Remarks

Remarks
Description: "STARK-B is a database of calculated widths and shifts of isolated lines of atoms and ions due to electron and ion collisions. This database is devoted to modeling and spectroscopic diagnostics of stellar atmospheres and envelopes. In addition, it is also devoted to laboratory plasmas, laser equipments and technological plasmas. So, the domain of temperatures and densities covered by the tables is wide and depends on the ionization degree of the considered ion. The temperature can vary from several thousands for neutral atoms to several hundred thousands of Kelvin for highly charged ions. The electron or ion density can vary from 1012 (case of stellar atmospheres) to several 1019cm-3 (some white dwarfs and some laboratory plasmas)."
Entry date
2015-04-22
Last update
2025-01-24
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Cite this re3data.org record:

re3data.org: STARK-B; editing status 2025-01-24; re3data.org - Registry of Research Data Repositories. https://doi.org/10.17616/R37P7H last accessed: 2026-07-07