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Active databases

NameDescriptionMaintainerAvailables species
BASECOL: VAMDC-TAP interfaceThis database, called BASECOL is devoted to collisional ro-vibrational excitation of molecules by colliders such as atom, ion, molecule or electron. It is supervised by an international working group of molecular physicists and astrophysicits involved in the calculations and use of ro-vibrational cross-sections, in order to ensure the continuity and the quality of the database.yaye-awa.ba@obspm.fr
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Belgrade electron/atom(molecule) database (BEAMDB)Electron interaction cross-sections for elastic scattering, electron excitation, ionization and total scattering.bratislav.marinkovic@ipb.ac.rs
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CDMSThe Cologne Database for Molecular Spectroscopy (CDMS) contains a catalog of radio frequency and microwave to far-infrared spectral lines of atomic and molecular species that (may) occur in the interstellar or circumstellar medium or in planetary atmospheres. The catalog is continuously updated.endres@ph1.uni-koeln.de
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Carbon Dioxide Spectroscopic Databank 1000K (VAMDC-TAP)Carbon Dioxide spectroscopic Data Base for high temperature applications (CDSD-1000) contains spectral line parameters of 7 most abundant in the Earth's atmosphere isotopologues of the carbon dioxide molecule: 16O12C16O, 16O13C16O, 16O12C18O, 16O12C17O, 16O13C18O, 16O13C17O, 18O12C18O, covers 257 - 9648 cm-1 spectral range and contains more than 3950500 lines. The line parameters (line position, line intensity, energy of lower state, air-broadening coefficient, self pressure induced broadening coefficient and exponent of temperature dependence of air broadening coefficient) have the calculated values. The line list has been generated using intensity cutoff 10-27 cm/molecule at reference temperature 1000 K.vip@lts.iao.ru
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Carbon Dioxide Spectroscopic Databank 296K (VAMDC-TAP)Carbon Dioxide spectroscopic Data Base for atmospheric applications (CDSD-296) contains spectral line parameters of 7 most abundant in the Earth's atmosphere isotopologues of the carbon dioxide molecule: 16O12C16O, 16O13C16O, 16O12C18O, 16O12C17O, 16O13C18O, 16O13C17O, 18O12C18O, covers 5.9 - 12784.1 cm-1 spectral range and contains more than 419600 lines. The line parameters (line position, line intensity, energy of lower state, air-broadening coefficient, self pressure induced broadening coefficient and exponent of temperature dependence of air broadening coefficients) have the calculated values. The line list has been generated using intensity cutoff 10-30 cm/molecule at reference temperature 296 K.vip@lts.iao.ru
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ChiantiChianti consists of a critically evaluated set of up-to-date atomic data, together with user-friendly programs written in Interactive Data Language (IDL), to analyse the spectra from astrophysical plasmas. The VAMDC interface presents just the data from the Chianti-v7 release.gtr@ast.cam.ac.uk
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ECaSDa - Ethene Calculated Spectroscopic DatabaseCalculated data of ethylene (12C2H4). The data on ethylene contain the vibration-rotation energy levels, line positions and line intensities in the range from 500 to 7500 cm-1ludovic.daumont@univ-reims.fr, maud.rotger@univ-reims.fr
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GSMA Reims S&MPOCalculated line lists for ozone (16O3, 16O18O16O and 18O3). The data on methane contain the vibration-rotation energy levels, line positions and line strengths in the range from 0 to 8000 cm-1.ylb@iao.ru, vladimir.tyuterev@univ-reims.fr
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GeCaSDa: Gemane Calculated Spectroscopic DatabaseCalculated line lists for Germane (GeH4)cyril.richard@u-bourgogne.fr
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GhoSSTThe GhoSST database ("Grenoble Astrophysics and Planetology Solid Spectroscopy and Thermodynamics" database service) provides laboratory data on spectra (from UV to FIR) of natural and synthetic solids (ices, molecular solids, minerals, salts, inorganic materials, organic materials, meteorites, adsorbed molecules, hydrated solids,?) of space sciences, Earth sciences and astrophysical interest. It is completed with band list data (NIR to FIR) on molecular solids and adsorbed/hydratation molecules. The GhoSST data come from laboratory experiments performed since 1989 at IPAG (and formerly at LGGE and LPG) with different spectroscopy techniques (transmission, bidirectional reflection, micro-spectroscopy, ATR, Raman, Fluorescence, ...).damien.albert@obs.ujf-grenoble.fr
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HITRANonlineThe HITRAN database, from http://www.cfa.harvard.edu/HITRAN/christian.hill@ucl.ac.uk
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IDEADB - Innsbruck Dissociative Electron Attachment DatabaseThis database contains informations about dissociative electron attachment upon interaction of low energy electrons with molecules.johannes.postler@uibk.ac.at
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JPL database: VAMDC-TAP serviceThe JPL database contains a catalog of radio frequency and microwave to far-infrared spectral lines of atomic and molecular species that (may) occur in the interstellar or circumstellar medium or in planetary atmospheres. The catalog is continuously updated. THIS IS JUST FOR DEVELOPMENTendres@ph1.uni-koeln.de
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KIDA: Kinetic Database for Astrochemistry - TAP serviceKIDA is a database of kinetic data interesting for astrochemical (interstellar medium and planetary atmospheres) studies. In addition to the available referenced data, KIDA provides recommendations over a number of important reactions. Chemists and physicists can add their data to the database.Valentine.Wakelam@obs.u-bordeaux1.fr
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LXcatAn open-access website for collecting, displaying, and downloading electron and ion scattering cross sections, swarm parameters (mobility, diffusion coefficient, etc.), reaction rates, energy distribution functions, etc. and other data required for modeling low temperature plasmas. The available data bases have been contributed by members of the community and are indicated by the contributor's chosen title.lxcat.info@gmail.com
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MeCaSDa - Methane Calculated Spectroscopic DatabaseCalculated line lists for methane (12CH4, 13CH4 and 12CH3D). The data on methane contain the vibration-rotation energy levels, line positions and line intensities in the range from 0 to 6200 cm-1.Vincent.Boudon@u-bourgogne.fr
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NIST Atomic Spectra DatabaseThis database provides access and search capability for NIST critically evaluated data on atomic energy levels, wavelengths, and transition probabilitiesyuri.ralchenko@nist.gov
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OACT - LASP Database“Laboratorio di Astrofisica Sperimentale” (Catania-LASp for short) has been active in Catania starting from the eighties. The eldest of the group, after some training at the Physics department of the Catania University, started the activity at the Catania Astrophysical Observatory. Since then and thanks to several funding agencies (Consiglio Nazionale delle Ricerche, Italian CNR; Ministero dell'Istruzione, dell'Universita' e della Ricerca, MIUR; Agenzia Spaziale Italiana, ASI; etc.) and to the help of many colleagues (and directors) of the Observatory the LASp has grown. Today Catania-LASp means a group of 6 people with permanent position plus some students and guests, a laboratory building equipped with high vacuum chambers, facilities for the deposition of ice films, ion and Lyman-alpha irradiation experiments, many spectrometers in the range from 190 nm up to 200 micron, and also raman spectrographs.gle@oact.inaf.it
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Photodissociation - MolD databaseDatabase for photodissociation cross-sections of molecular ions from individual ro-vibrational states and cross-sections and rate coefficients for radiative ion-atom collisional processes.vlada@ipb.ac.rs
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RuCaSDa: Ruthenium tetroxide Calculated Spectroscopic DatabaseLines of Ruthenium Tetroxide (RuO4)cyril.richard@u-bourgogne.fr
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SHeCaSDa - SF6 Calculated Spectroscopic DatabaseCalculated line lists for sulfur hexafluoride (32SF6, 33SF6, 34SF6). The data on SF6 contain the vibration-rotation energy levels, line positions and line intensities in the range from 200 to 3000 cm-1.Vincent.Boudon@u-bourgogne.fr
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SpEctroScopy of Atoms and MoleculesSesam is a project of the LERMA (Laboratoire d'Etudes du Rayonnement et de la Matiere). Its purpose is to provide an atomic and molecular spectral database dedicated more specifically to electronic spectra. The structure of the database has been elaborated with the tools developed in the VAMDC (Virtual Atomic and Molecular Data Center) projectevelyne.roueff@obspm.fr
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Spectr-W3The information accumulated in the SPECTR-W3 ADB contains over 450,000 records and includes factual experimental and theoretical data on ionization potentials, energy levels, wavelengths, radiation transition probabilities, oscillator strengths, and (optionally) the parameters of analytical approximations of electron-collisional cross-sections and rates for atoms and ions. Those data were extracted from publications in physical journals, proceedings of the related conferences, special-purpose publications on atomic data, and provided directly by authors. The information is supplied with references to the original sources and comments, elucidating the details of experimental measurements or calculations, where necessary and available. To date, the SPECTR-W3 ADB is the largest factual database in the world containing the information on spectral properties of multicharged ions.p_a_loboda@mail.ru
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Stark-bDatabase for "Stark" broadening of isolated lines of atoms and ions in the impact approximationsylvie.sahal-brechot@obspm.fr
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TFMeCaSDa - CF4 Calculated Spectroscopic DatabaseCalculated 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.Vincent.Boudon@u-bourgogne.fr
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TIPbase : VAMDC-TAP interfaceTIPbase lists fine-structure levels, A-values, collision strengths and effective collision strengths for astrophysically abundant ions, mainly from the Fe isonuclear sequence computed in the Iron Project.nicolas.moreau@obspm.fr - franck.delahaye@obspm.fr
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TOPbase : VAMDC-TAP interfaceTOPbase lists LS-coupling energy levels, gf-values and photoionization cross sections for astrophysically abundant ions (Z=1,14; Z=16; Z=18; Z=20; Z=26) computed in the Opacity Project.nicolas.moreau@obspm.fr - franck.delahaye@obspm.fr
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Theoretical spectral database of polycyclic aromatic hydrocarbonsThe Cagliari/Toulouse PAH database is a collection of theoretical spectroscopic data about Polycyclic Aromatic Hydrocarbons and carbon clusters. It provides basic geometric characteristics, energetics, harmonic analyses and electronic photoabsorption data. It is maintained by the Astrochemistry group at INAF-Observatory of Cagliari and the Institut de Recherche en Astrophysique et Plan?tologie in Toulouse.gmulas@oa-cagliari.inaf.it
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UMIST Database for AstrochemistryReaction rate coefficients for astrochemical modelling.k.w.smith@qub.ac.uk
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VALD (atoms)The Vienna Atomic Line Database (VALD) is a collection of atomic line parameters (wavelengths, transition energies and quantum numbers, oscillator strengths, Lande factors, radiative and collisional broadening). This resource is the VAMDC-TAP representation of the atomic data in VALD3.thomas.marquart@fysast.uu.se
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VALD sub-set in Moscow (obs)The part of Vienna Atomic Line Database (VALD) with accurate wavelength and energy levels. It also provides laboratory and calculated transition probabilities, Lande factors and broadening parameters. It is used for line identification and spectral synthesis.pakhomov@inasan.ru
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VAMDC species-DBThis Database contains all the species and its VAMDC-Species Ids which are used by VAMDC.nicolas.moreau@obspm.fr
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Water internet Accessible Distributed Information SystemDatabase containing information on water spectras, notably data on H216O, HDO, D2O, H217O and H218O.faz@iao.ru
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