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Databases Partners


  • / National Institute for Fusion Science

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  • / Institute for Ion Physics and Applied Physics, Innsbruck

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  • / NIST

    NIST ASD Team

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  • / The Electron Scattering and Modelling group at FLINDERS UNIVERSITY

    The Electron Scattering and Modelling group at FLINDERS UNIVERSITY (Australia).

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  • / Departamento de Física, Universidade Federal do Paranà

    Departamento de Física, Universidade Federal do Paranà (Brazil).

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  • / Atomic And Molecular Data Unit IAEA

    Atomic And Molecular Data Unit IAEA.

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  • / Jet Propulsion Laboratory, California Institute of Technology

    Jet Propulsion Laboratory, California Institute of Technology.

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  • / The Harvard Smithsonian Center for Astrophysics

    The Harvard Smithsonian Center for Astrophysics.

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  • / INAF – Cagliari Astronomical Observatory

    The National Institute for Astrophysics is the leading Italian Research Institute for the Study of the Universe.

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  • / INAF-Catania Astrophysical Observatory

    The Catania Astrophysical Observatory (OACT) is one of the twelve observatories which together with some former CNR Institutes.

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  • / Universitaet Wien

    Partners in VAMDC project (, but not yet partners in VAMDC Consortium.

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  • / Corporacion Parque tecnologico de Merida

    Partners in VAMDC project (, but not yet partners in VAMDC Consortium.

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  • / Institute of Atmospheric Optics

    Partners in VAMDC Consortium.

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  • / Russian Federal Nuclear Center- All-Russian Institute of Technical Physics

    Partners in VAMDC Consortium.

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  • / Institute of Spectroscopy RAS

    Institute for Spectroscopy was established in 1968 as a successor of the Commission for Spectroscopy within the General physics and astronomy Branch of the USSR Academy of Sciences.

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  • / Astronomical Observatory Belgrade

    Founded jointly with the Meteorological Observatory on April, 7 1887, Astronomical Observatory of Belgrade (AOB) is one of the oldest scientific institutions in Serbia.

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  • / Queen’s University Belfast

    Queen’s University Belfast is the leading university in Northern Ireland and a member of the Russell Group.

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  • / INASAN

    Institute of Astronomy of the Russian Academy of Sciences (INASAN) has grown from the Astronomical Council of the Academy of Sciences of the USSR.

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  • / Institute of Research in Astrophysics and Planetology (IRAP, Univ. Toulouse III/CNRS)

    The University of Toulouse III Paul Sabatier (UPS; created in 1969) is one of the most important scientific research clusters in France at the heart of a European space and aeronautics capital.

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  • / Laboratoire Interdisciplinaire Carnot de Bourgogne

    The Molecular Spectroscopy and Applications group of the Institut Carnot de Bourgogne is the world leader in the analysis of high-resolution spectra of methane (12CH4, 13CH4 and CH3D).

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  • / Laboratoire de Planétologie Grenoble

    Laboratory of Planetology (laboratoire de Planétologie Grenoble).

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  • / Laboratoire d’Astrophysique de Bordeaux

    The Laboratoire d’Astrophysique de Bordeaux (LAB) is a research institute from the Centre National de la Recherche Scientifique (CNRS) and the University of Bordeaux.

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  • / Groupe de Spectroscopie Moléculaire et Atmosphérique de Reims

    The Group of Molecular and Atmospheric Spectroscopy (Groupe de Spectroscopie Moleculaire et Atmospherique , GSMA, UMR CNRS 7331) of the University of Reims, France.,9553.html?

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  • / Tata Institute of Fundamental Research

    Tata institute of fundamental research.

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  • / University of South Africa

    University of South Africa.

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  • / Korea Atomic Energy Research Institute

    KAERI has been the leading national institute for the research and development of nuclear technologies in KOREA.

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  • / University College London

    University College London is the largest and oldest college of the University of London. It was founded in 1826 to open up education to all on equal terms and to bring the benefits of learning to society.

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  • / Universität zu Köln

    The University of Cologne is one of the largest universities in Germany with about 49000 students and about 6000 employees working in a broad range of disciplines.

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  • / The Open University

    The Open University is a world leader in modern distance learning.

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  • / Uppsala Universitet

    Uppsala University (UU) is the oldest university in Sweden with about 40000 students and over 5000 employees pursuing research and education over a broad range of disciplines.

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  • / Observatoire de Paris

    Founded in 1667, the Observatoire de Paris is the largest national research center for astronomy. 30 % of all French astronomers are working in it five laboratories and its institute.

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  • / University of Cambridge

    The earliest records of the University date back to 1209 – with the first college of the University being founded in 1284.

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  • / RADAM Portal

    RADAM portal is an interface to the network of RADAM (RADiation DAMage) Databases collecting data on interactions of ions, electrons, positrons and photons with biomolecular systems.

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  • / TFMeCaSDa – CF4 Calculated Spectroscopic Database

    Calculated line lists for carbon tetrafluoride (12CF4). The data on CF4 contain the vibration-rotation energy levels, line positions and line intensities in the range from 500 to 1500 cm-1.

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  • / Belgrade electron/atom(molecule) database (BEAMDB)

    Electron interaction cross-sections for elastic scattering, electron excitation, ionization and total scattering.

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  • / SHeCaSDa – SF6 Calculated Spectroscopic Database

    Calculated line lists for sulfur hexafluoride (32SF6, 33SF6, 34SF6). The data on SF6 contain the vibration-rotation energy levels, line positions and line intensities.

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  • / PAH

    The Theoretical Spectral Database of Polycyclic Aromatic Hydrocarbons was developed in collaboration by G. Malloci and G. Mulas.

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  • / ECaSDa – Ethylene Calculated Spectroscopic Database

    Calculated data of ethylene (12C2H4). The data on ethylene contain the vibration-rotation energy levels, line positions.

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  • / VAMDC species-DB

    This Database contains all the species and its VAMDC-Species Ids which are used by VAMDC.

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  • / KIDA

    The KInetic Database for Astrochemistry (KIDA) is a database of chemical reactions used in chemical models for astrophysical environments such as the interstellar medium and planetary atmospheres.

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  • / Water internet Accessible Distributed Information System (W@DIS)

    The W@DIS information system is designed to provide access to data, information, and ontologies relating to quantitative spectroscopy.

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  • / Spectr-W3

    Atomic database Spectr-W3 for plasma spectroscopy and other applications.

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  • / Carbon Dioxide Spectroscopic Databank 1000K

    Carbon Dioxide spectroscopic Data Base for high temperature applications (CDSD-1000) contains spectral line parameters.

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  • / SESAM

    SESAM (SpEctroScopy of Atoms and Molecules) is devoted to the spectroscopic analysis of UV electronic spectra of diatomic molecules.

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  • / Carbon Dioxide Spectroscopic Databank 296K

    Carbon Dioxide spectroscopic Data Base for atmospheric applications (CDSD-296) contains spectral line parameters.

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  • / CDMS

    The Cologne Database for Molecular Spectroscopy (CDMS) contains a catalog of radio frequency.

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  • / TIPbase

    TIPbase lists fine-structure levels, A-values, collision strengths and effective collision strengths for astrophysically.

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  • / IDEADB – Innsbruck Dissociative Electron Attachment Database

    This database contains informations about dissociative electron attachment upon interaction of low energy electrons.

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  • / UMIST Database for Astrochemistry

    Reaction rate coefficients for astrochemical modelling.

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  • / DESIRE database (Moscow mirror)

    The main purpose of D.E.S.I.R.E. is to provide the astrophysicists, but also the physicists, with an updated information.

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  • / TOPbase

    TOPbase lists LS-coupling energy levels, gf-values and photoionization cross sections for astrophysically abundant ions.

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  • / OACT – LASP Database

    Experimental Astrophysics Laboratory at Catania Astrophysical Observatory, Italy.

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  • / VALD3

    VALD is a collection of atomic and molecular transition parameters that are of astrophysical interest.

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  • / MeCaSDa – Methane Calculated Spectroscopic Database

    Methane Calculated Spectroscopic Database.

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  • / ALADDIN2

    A subset of the IAEA ALADDIN database for testing its implementation as a VAMDC node.

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  • / RADAM – Ion Interactions

    Database for Radiation damage of molecules of biological interest induced by ion collisions.

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  • / VALD sub-set in Moscow (obs)

    The Vienna Atomic Line Database (VALD) is a collection of atomic and molecular transition parameters.

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  • / HITRAN database

    HITRAN is an acronym for high-resolution transmission molecular absorption database.

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  • / JPL database

    The JPL database contains a catalog of radio frequency and microwave to far-infrared spectral lines.

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  • / STARK-B

    STARK-B is a database of calculated widths and shifts of isolated lines of neutral and ionized atoms due to electron and ion collisions.

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    BASECOL is devoted to collisional ro-vibrational excitation of molecules by colliders such as atom, ion, molecule.

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    An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas.

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  • / GSMA Reims S&MPO

    Calculated line lists for ozone (16O3, 16O18O16O and 18O3).

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  • / GhoSST

    Grenoble Astrophysics and Planetology Solid Spectroscopy and Thermodynamics database.

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