J/A+A/538/A100ivo://CDS.VizieR/J/A+A/538/A100doi:10.26093/cds/vizier.35380100CDSLemasle B.Hill V.Tolstoy E.Venn K.A.Shetrone M.D.Irwin M.J.,de Boer T.J.L.Starkenburg E.Salvadori S.2017-06-01T08:52:59Z2012-02-09T12:55:12ZCDS support team

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

cds-question@unistra.frgalaxiesgiant-starschemical-abundancesradial-velocityline-intensitiesinfrared-photometryvisible-astronomyWide-band photometryThe ages of individual Red Giant Branch stars can range from 1Gyr old to the age of the Universe, and it is believed that the abundances of most chemical elements in their photospheres remain unchanged with time (those that are not affected by the first dredge-up). This means that they trace the interstellar medium in the galaxy at the time the star formed, and hence the chemical enrichment history of the galaxy. Colour-Magnitude Diagram analysis has shown the Carina dwarf spheroidal to have had an unusually episodic star formation history and this is expected to be reflected in the abundances of different chemical elements.2012A&A...538A.100Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/538/A100CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/AJ/130/2677 : Stars in the Carina dSph galaxy field (Majewski+, 2005)J/ApJ/649/201 : Velocities & Washington photometry in Carina dSph (Munoz+ 2006)J/AJ/135/1580 : Element abundances in ten red giants of Car dSph (Koch+, 2008)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/538/A100https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/538/A100http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/538/A100https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/538/A100https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/538/A100http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/538/A100GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/538/A100/table3 (Photometric information for our FLAMES targets)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/538/A100/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/538/A100/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/538/A100/table3?GETtext/xml+votable180.050000true100.4927917-50.77816670.0055555555555555566/39097 391001.0937653039707433e-19 3.9865436196254505e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/538/A100?format=asciiOpticalInfrareddefaultJ/A+A/538/A100/table3Photometric information for our FLAMES targetsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSpSimbad column added by the CDSmeta.ref.urlcharNameName MKVNNNNmeta.id;meta.maincharprimaryRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainVmagESO-WFI V magnitudemagphot.mag;em.opt.VfloatImagESO-WFI I magnitudemagphot.mag;em.opt.IfloatJmag? ESO-SOFI J magnitude (1)magphot.mag;em.opt.VfloatnullableHmag? ESO-SOFI H magnitude (1)magphot.mag;em.opt.VfloatnullableKmag? ESO-SOFI K magnitude (1)magphot.mag;em.opt.VfloatnullableHRVHeliocentric radial velocity (2)km/sspect.dopplerVeloc;pos.heliocentricfloate_HRVrms uncertainty on HRV (2)km/sstat.errorfloatMembMembershipmeta.code.membercharJ/A+A/538/A100/abunFinal abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.mainchar[Fe1/H]Abundance [FeI/H]phys.abundfloate_[Fe1/H]rms uncertainty on [FeI/H]phys.abundfloato_[Fe1/H]Number of line used for [FeI/H]phys.abundint[Fe2/H]? Abundance [FeII/H]phys.abundfloatnullablee_[Fe2/H]? rms uncertainty on [FeII/H]phys.abundfloatnullableo_[Fe2/H]? Number of line used for [FeII/H]phys.abundintnullable[Mg1/H]? Abundance [MgI/H]phys.abundfloatnullablee_[Mg1/H]? rms uncertainty on [MgI/H]phys.abundfloatnullableo_[Mg1/H]? Number of line used for [MgI/H]phys.abundintnullable[Ca1/H]? Abundance [CaI/H]phys.abundfloatnullablee_[Ca1/H]? rms uncertainty on [CaI/H]phys.abundfloatnullableo_[Ca1/H]? Number of line used for [CaI/H]phys.abundintnullable[Ti1/H]? Abundance [TiI/H]phys.abundfloatnullablee_[Ti1/H]? rms uncertainty on [TiI/H]phys.abundfloatnullableo_[Ti1/H]? Number of line used for [TiI/H]phys.abundintnullable[Ti2/H]? Abundance [TiII/H]phys.abundfloatnullablee_[Ti2/H]? rms uncertainty on [TiII/H]phys.abundfloatnullableo_[Ti2/H]? Number of line used for [TiII/H]phys.abundintnullable[Cr1/H]? Abundance [CrI/H]phys.abundfloatnullablee_[Cr1/H]? rms uncertainty on [CrI/H]phys.abundfloatnullableo_[Cr1/H]? Number of line used for [CrI/H]phys.abundintnullable[Co1/H]? Abundance [CoI/H]phys.abundfloatnullablee_[Co1/H]? rms uncertainty on [CoI/H]phys.abundfloatnullableo_[Co1/H]? Number of line used for [CoI/H]phys.abundintnullable[Ni1/H]? Abundance [NiI/H]phys.abundfloatnullablee_[Ni1/H]? rms uncertainty on [NiI/H]phys.abundfloatnullableo_[Ni1/H]? Number of line used for [NiI/H]phys.abundintnullable[Ba2/H]? Abundance [BaII/H]phys.abundfloatnullablee_[Ba2/H]? rms uncertainty on [BaII/H]phys.abundfloatnullableo_[Ba2/H]? Number of line used for [BaII/H]phys.abundintnullable[Na1/H]? Abundance [NaI/H]phys.abundfloatnullablee_[Na1/H]? rms uncertainty on [NaI/H]phys.abundfloatnullableo_[Na1/H]? Number of line used for [NaI/H]phys.abundintnullable[Si1/H]? Abundance [SiI/H]phys.abundfloatnullablee_[Si1/H]? rms uncertainty on [SiI/H]phys.abundfloatnullableo_[Si1/H]? Number of line used for [SiI/H]phys.abundintnullable[Sc2/H]? Abundance [ScII/H]phys.abundfloatnullablee_[Sc2/H]? rms uncertainty on [ScII/H]phys.abundfloatnullableo_[Sc2/H]? Number of line used for [ScII/H]phys.abundintnullable[Y2/H]? Abundance [YII/H]phys.abundfloatnullablee_[Y2/H]? rms uncertainty on [YII/H]phys.abundfloatnullableo_[Y2/H]? Number of line used for [YII/H]phys.abundintnullable[La2/H]? Abundance [LaII/H]phys.abundfloatnullablee_[La2/H]? rms uncertainty on [LaII/H]phys.abundfloatnullableo_[La2/H]? Number of line used for [LaII/H]phys.abundintnullable[Nd2/H]? Abundance [NdII/H]phys.abundfloatnullablee_[Nd2/H]? rms uncertainty on [NdII/H]phys.abundfloatnullableo_[Nd2/H]? Number of line used for [NdII/H]phys.abundintnullable[Eu2/H]? Abundance [EuII/H]phys.abundfloatnullablee_[Eu2/H]? rms uncertainty on [EuII/H]phys.abundfloatnullableo_[Eu2/H]? Number of line used for [EuII/H]phys.abundintnullableJ/A+A/538/A100/table4List of all spectral lines, their atomic parameters and their measured EWs for all the 35 RGB stars in the Carina dSphElElementphys.atmol.elementcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharlambdaWavelength0.1nmem.wlfloatExPotExcitation potentialeVphys.atmol.excitationfloatloggfOscillator strengthphys.atmol.oscStrengthfloatEW? Equivalent width0.1pmspect.line.eqWidthintnullable