J/A+A/586/A120ivo://CDS.VizieR/J/A+A/586/A120doi:10.26093/cds/vizier.35860120CDSOsorio Y.Barklem P.S.2016-02-26T13:20:46Z2016-02-04T09:04:22ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frastronomical-modelsstellar-atmosphereschemical-abundancesline-intensitiesMg is the alpha element of choice for Galactic population and chemical evolution studies as it is easily detectable in all late-type stars. Such studies require precise elemental abundances, and thus departures from LTE need to be accounted for.2016A&A...586A.120Ohttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/586/A120CatalogResearchIsServedByTAP VizieR generic servicerelated-toVI/73 : Atomic Spectral Lines Data OII, Mg, Al, S, Sc (NIST 1993)J/A+AS/117/127 : Solar MgI lines Stark broadening (Dimitrijevic+, 1996)J/A+A/487/1203 : Electron-impact excitation of Be-like Mg (Del Zanna+, 2008)J/MNRAS/414/1227 : Mg/Fe ratio of MILES stars (Milone+, 2011)J/MNRAS/418/863 : NLTE corrections for Mg and Ca lines (Merle+ 2011)J/A+A/554/A24 : Infra-red transitions of Ca and Mg (Civis+, 2013)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/586/A120https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/586/A120http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/586/A120https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/586/A120https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/586/A120http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/586/A120GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/586/A120/mgnlteMg LTE and non-LTE equivalent widths (w) for 19 MgI linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeffEffective temperatureKphys.temperature.effectiveintloggSurface gravitylog(cm.s**-2)phys.gravityfloat[Fe/H]Metallicitylog(Sun)phys.abund.ZfloatVturbMicroturbulent velocitykm/sphys.velocfloatA(Mg)Mg abundance (log[Mg/H]+12)log(Sun)phys.abundfloat3829LTElog(wlte/lambda) for 3829{AA} (1)spect.line.eqWidthdouble3829NLTElog(w/lambda) for 3829{AA} (1)spect.line.eqWidthdouble3832LTElog(wlte/lambda) for 3832{AA} (1)spect.line.eqWidthdouble3832NLTElog(w/lambda) for 3832{AA} (1)spect.line.eqWidthdouble3838LTElog(wlte/lambda) for 3838{AA} (1)spect.line.eqWidthdouble3838NLTElog(w/lambda) for 3838{AA} (1)spect.line.eqWidthdouble4167LTElog(wlte/lambda) for 4167{AA} (1)spect.line.eqWidthdouble4167NLTElog(w/lambda) for 4167{AA} (1)spect.line.eqWidthdouble4571LTElog(wlte/lambda) for 4571{AA} (1)spect.line.eqWidthdouble4571NLTElog(w/lambda) for 4571{AA} (1)spect.line.eqWidthdouble4703LTElog(wlte/lambda) for 4703{AA} (1)spect.line.eqWidthdouble4703NLTElog(w/lambda) for 4703{AA} (1)spect.line.eqWidthdouble5167LTElog(wlte/lambda) for 5167{AA} (1)spect.line.eqWidthdouble5167NLTElog(w/lambda) for 5167{AA} (1)spect.line.eqWidthdouble5172LTElog(wlte/lambda) for 5172{AA} (1)spect.line.eqWidthdouble5172NLTElog(w/lambda) for 5172{AA} (1)spect.line.eqWidthdouble5183LTElog(wlte/lambda) for 5183{AA} (1)spect.line.eqWidthdouble5183NLTElog(w/lambda) for 5183{AA} (1)spect.line.eqWidthdouble5528LTElog(wlte/lambda) for 5528{AA} (1)spect.line.eqWidthdouble5528NLTElog(w/lambda) for 5528{AA} (1)spect.line.eqWidthdouble5711LTElog(wlte/lambda) for 5711{AA} (1)spect.line.eqWidthdouble5711NLTElog(w/lambda) for 5711{AA} (1)spect.line.eqWidthdouble7691LTElog(wlte/lambda) for 7691{AA} (1)spect.line.eqWidthdouble7691NLTElog(w/lambda) for 7691{AA} (1)spect.line.eqWidthdouble8710LTElog(wlte/lambda) for 8710{AA} (1)spect.line.eqWidthdouble8710NLTElog(w/lambda) for 8710{AA} (1)spect.line.eqWidthdouble8712LTElog(wlte/lambda) for 8712{AA} (1)spect.line.eqWidthdouble8712NLTElog(w/lambda) for 8712{AA} (1)spect.line.eqWidthdouble8718LTElog(wlte/lambda) for 8718{AA} (1)spect.line.eqWidthdouble8718NLTElog(w/lambda) for 8718{AA} (1)spect.line.eqWidthdouble8736LTElog(wlte/lambda) for 8736{AA} (1)spect.line.eqWidthdouble8736NLTElog(w/lambda) for 8736{AA} (1)spect.line.eqWidthdouble8806LTElog(wlte/lambda) for 8806{AA} (1)spect.line.eqWidthdouble8806NLTElog(w/lambda) for 8806{AA} (1)spect.line.eqWidthdouble21059LTElog(wlte/lambda) for 21059{AA} (1)spect.line.eqWidthdouble21059NLTElog(w/lambda) for 21059{AA} (1)spect.line.eqWidthdouble21061LTElog(wlte/lambda) for 21061{AA} (1)spect.line.eqWidthdouble21061NLTElog(w/lambda) for 21061{AA} (1)spect.line.eqWidthdoubleJ/A+A/586/A120/listList of individual filesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintfileDownload the filemeta.ref.urlcharFileNameName of the file in data subdirectorymeta.id;meta.filecharTitleTitle of the filemeta.title;meta.filechar