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Article: The radial velocity experiment (RAVE): Fourth data release

TitleThe radial velocity experiment (RAVE): Fourth data release
Authors
Keywordsstars: abundances
techniques: spectroscopic
surveys
stars: fundamental parameters
catalogs
Issue Date2013
Citation
Astronomical Journal, 2013, v. 146, n. 5 How to Cite?
AbstractWe present the stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, individual abundances, and distances determined for 425,561 stars, which constitute the fourth public data release of the RAdial Velocity Experiment (RAVE). The stellar atmospheric parameters are computed using a new pipeline, based on the algorithms of MATISSE and DEGAS. The spectral degeneracies and the Two Micron All Sky Survey photometric information are now better taken into consideration, improving the parameter determination compared to the previous RAVE data releases. The individual abundances for six elements (magnesium, aluminum, silicon, titanium, iron, and nickel) are also given, based on a special-purpose pipeline that is also improved compared to that available for the RAVE DR3 and Chemical DR1 data releases. Together with photometric information and proper motions, these data can be retrieved from the RAVE collaboration Web site and the Vizier database. © 2013. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/208982
ISSN
2023 Impact Factor: 5.1
2023 SCImago Journal Rankings: 1.953
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorKordopatis, Georges-
dc.contributor.authorGilmore, Gerard F.-
dc.contributor.authorSteinmetz, Matthias-
dc.contributor.authorBoeche, Corrado-
dc.contributor.authorSeabroke, George M.-
dc.contributor.authorSiebert, Arnaud-
dc.contributor.authorZwitter, Tomaž-
dc.contributor.authorBinney, James J.-
dc.contributor.authorDe Laverny, Patrick-
dc.contributor.authorRecio-Blanco, Alejandra-
dc.contributor.authorWilliams, Mary E K-
dc.contributor.authorPiffl, Tilmann-
dc.contributor.authorEnke, Harry-
dc.contributor.authorRoeser, Siegfried-
dc.contributor.authorBijaoui, Albert-
dc.contributor.authorWyse, Rosemary F G-
dc.contributor.authorFreeman, Kenneth C.-
dc.contributor.authorMunari, Ulisse-
dc.contributor.authorCarrillo, I.-
dc.contributor.authorAnguiano, Borja-
dc.contributor.authorBurton, Donna M.-
dc.contributor.authorCampbell, Randy D.-
dc.contributor.authorCass, C. J P-
dc.contributor.authorFiegert, Kristin-
dc.contributor.authorHartley, Malcolm-
dc.contributor.authorParker, Quentin A.-
dc.contributor.authorReid, Warren A.-
dc.contributor.authorRitter, Andreas-
dc.contributor.authorRussell, Ken S.-
dc.contributor.authorStupar, Milorad-
dc.contributor.authorWatson, Fred G.-
dc.contributor.authorBienaymé, Olivier-
dc.contributor.authorBland-Hawthorn, Joss Bland-
dc.contributor.authorGerhard, Ortwin E.-
dc.contributor.authorGibson, Brad K.-
dc.contributor.authorGrebel, Eva K.-
dc.contributor.authorHelmi, Amina-
dc.contributor.authorNavarro, Julio F.-
dc.contributor.authorConrad, C.-
dc.contributor.authorFamaey, Benoît-
dc.contributor.authorFauré, Carole-
dc.contributor.authorJust, Andreas-
dc.contributor.authorKos, Janez-
dc.contributor.authorMatijevič, Gal-
dc.contributor.authorMcMillan, Paul J.-
dc.contributor.authorMinchev, Ivan-
dc.contributor.authorScholz, Ralf Dieter-
dc.contributor.authorSharma, Sanjib-
dc.contributor.authorSiviero, Alessandro-
dc.contributor.authorWylie-De Boer, E. C.-
dc.contributor.authorŽerjal, M.-
dc.date.accessioned2015-03-23T02:02:27Z-
dc.date.available2015-03-23T02:02:27Z-
dc.date.issued2013-
dc.identifier.citationAstronomical Journal, 2013, v. 146, n. 5-
dc.identifier.issn0004-6256-
dc.identifier.urihttp://hdl.handle.net/10722/208982-
dc.description.abstractWe present the stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, individual abundances, and distances determined for 425,561 stars, which constitute the fourth public data release of the RAdial Velocity Experiment (RAVE). The stellar atmospheric parameters are computed using a new pipeline, based on the algorithms of MATISSE and DEGAS. The spectral degeneracies and the Two Micron All Sky Survey photometric information are now better taken into consideration, improving the parameter determination compared to the previous RAVE data releases. The individual abundances for six elements (magnesium, aluminum, silicon, titanium, iron, and nickel) are also given, based on a special-purpose pipeline that is also improved compared to that available for the RAVE DR3 and Chemical DR1 data releases. Together with photometric information and proper motions, these data can be retrieved from the RAVE collaboration Web site and the Vizier database. © 2013. The American Astronomical Society. All rights reserved.-
dc.languageeng-
dc.relation.ispartofAstronomical Journal-
dc.subjectstars: abundances-
dc.subjecttechniques: spectroscopic-
dc.subjectsurveys-
dc.subjectstars: fundamental parameters-
dc.subjectcatalogs-
dc.titleThe radial velocity experiment (RAVE): Fourth data release-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1088/0004-6256/146/5/134-
dc.identifier.scopuseid_2-s2.0-84886872374-
dc.identifier.volume146-
dc.identifier.issue5-
dc.identifier.isiWOS:000325976200031-
dc.identifier.issnl0004-6256-

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