J/AJ/141/62ivo://CDS.VizieR/J/AJ/141/62doi:10.26093/cds/vizier.51410062CDSLai D.K.Smith G.H.Bolte M.Johnson J.A.Lucatello S.Kraft R.P.,Sneden C.2017-07-10T06:22:07Z2012-08-17T14:35:05ZCDS support team

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

cds-question@unistra.frglobular-star-clustersline-intensitieschemical-abundancesWe present analysis of high-resolution spectra of a sample of stars in the globular cluster M5 (NGC 5904). The sample includes stars from the red giant branch (RGB; seven stars), the red horizontal branch (two stars), and the asymptotic giant branch (AGB; eight stars), with effective temperatures ranging from 4000K to 6100K. Spectra were obtained with the HIRES spectrometer on the Keck I telescope, with a wavelength coverage from 3700{AA} to 7950{AA} for the HB and AGB sample, and 5300{AA} to 7600{AA} for the majority of the RGB sample.2011AJ....141...62Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/141/62CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/611/323 : BVI photometry of M5 giant branch stars (Sandquist+, 2004)J/ApJ/689/1031 : Heavy element abundances in giant stars (Yong+, 2008)J/ApJ/689/1031 : Heavy element abundances in giant stars (Yong+, 2008)J/AJ/139/2289 : Abundances of five red giants in M5 (Koch+, 2010)J/AJ/141/62 : M5 chemical abundances for evolved stars (Lai+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/141/62https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/141/62http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/141/62https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/141/62https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/141/62http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/141/62GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/141/62/stars (Results for the 17 stars: observations, atmospheric parameters and abundances)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/141/62/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/141/62/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/141/62/stars?GETtext/xml+votable180.050000true229.65570832.10219440.0055555555555555566/31416 31417https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/141/62?format=asciiOpticaldefaultJ/AJ/141/62/starsResults for the 17 stars: observations, atmospheric parameters and abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharprimaryONameAlternative namemeta.idcharVmagV magnitudemagphot.mag;em.opt.VfloatB-VB-V colour indexmagphot.color;em.opt.B;em.opt.VfloatDateObserving datetime.epochnullableTexpTotal exposure timestime.duration;obs.exposureintS/NSignal-to-noise ration at 6035{AA}stat.snrintStage[AGB HB RGB] Evolutionary stagesrc.classcharSNameSimbad namemeta.idcharS04Details from Sandquist et al. 2004, Cat. J/ApJ/611/323meta.ref.urlcharSimbadSimbad column added by the CDSmeta.refcharTeffEffective temperatureKphys.temperature.effectiveintloggSurface gravitylog(cm.s**-2)phys.gravityfloatvtMicroturbulent velocitykm/sphys.velocfloat[A/H]Abundance ([Fe/H]) adopted as stellar parameterlog(Sun)phys.abund.FefloatVelRadial Velocitykm/sphys.velocfloat[Fe/H]Abundance [Fe/H]log(Sun)phys.abund.Fefloate_[Fe/H]rms uncertainty on [Fe/H]log(Sun)stat.error;phys.abund.Fefloato_[Fe/H]Number of lines for [Fe/H]meta.numberint[FeII/H]Abundance [FeII/H]log(Sun)phys.abundfloate_[FeII/H]rms uncertainty on [FeII/H]log(Sun)stat.error;phys.abundfloato_[FeII/H]Number of lines for [FeII/H]meta.numberintLi? Li number abundance (log(Li/H)+12)phys.abundfloatnullablee_Li? rms uncertainty on Listat.errorfloatnullableo_Li? Number of lines for Limeta.numberintnullable12C/13C? ^12^C/^13^C ratiophys.abundfloatnullablee_12C/13C? rms uncertainty on ^12^C/^13^C ratiostat.errorfloatnullableo_12C/13C? Number of lines for ^12^C/^13^C ratiometa.numberintnullablel_[C/Fe]Limit flag on [C/Fe]meta.code.error;phys.abundchar[C/Fe]? Abundance [C/Fe]log(Sun)phys.abundfloatnullablee_[C/Fe]? rms uncertainty on [C/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[C/Fe]? Number of lines for [C/Fe]meta.numberintnullablel_[N/Fe]Limit flag on [N/Fe]meta.code.error;phys.abundchar[N/Fe]? Abundance [N/Fe]log(Sun)phys.abundfloatnullablee_[N/Fe]? rms uncertainty on [N/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[N/Fe]? Number of lines for [N/Fe]meta.numberintnullable[O/Fe]? Abundance [O/Fe]log(Sun)phys.abundfloatnullablee_[O/Fe]? rms uncertainty on [O/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[O/Fe]? Number of lines for [O/Fe]meta.numberintnullable[Na/Fe]Abundance [Na/Fe]log(Sun)phys.abundfloate_[Na/Fe]rms uncertainty on [Na/Fe]log(Sun)stat.error;phys.abundfloato_[Na/Fe]Number of lines for [Na/Fe]meta.numberint[Mg/Fe]Abundance [Mg/Fe]log(Sun)phys.abundfloate_[Mg/Fe]rms uncertainty on [Mg/Fe]log(Sun)stat.error;phys.abundfloato_[Mg/Fe]Number of lines for [Mg/Fe]meta.numberint[Al/Fe]? Abundance [Al/Fe]log(Sun)phys.abundfloatnullablee_[Al/Fe]? rms uncertainty on [Al/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[Al/Fe]? Number of lines for [Al/Fe]meta.numberintnullable[Si/Fe]Abundance [Si/Fe]phys.abundfloate_[Si/Fe]rms uncertainty on [Si/Fe]stat.error;phys.abundfloato_[Si/Fe]Number of lines for [Si/Fe]meta.numberint[Ca/Fe]Abundance [Ca/Fe]log(Sun)phys.abundfloate_[Ca/Fe]rms uncertainty on [Ca/Fe]log(Sun)stat.error;phys.abundfloato_[Ca/Fe]Number of lines for [Ca/Fe]meta.numberint[ScII/Fe]Abundance [ScII/Fe]log(Sun)phys.abundfloate_[ScII/Fe]rms uncertainty on [ScII/Fe]log(Sun)stat.error;phys.abundfloato_[ScII/Fe]Number of lines for [ScII/Fe]meta.numberint[TiI/Fe]Abundance [TiI/Fe]log(Sun)phys.abundfloate_[TiI/Fe]rms uncertainty on [TiI/Fe]log(Sun)stat.error;phys.abundfloato_[TiI/Fe]Number of lines for [TiI/Fe]meta.numberint[TiII/Fe]Abundance [TiII/Fe]log(Sun)phys.abundfloate_[TiII/Fe]rms uncertainty on [TiII/Fe]log(Sun)stat.error;phys.abundfloato_[TiII/Fe]Number of lines for [TiII/Fe]meta.numberint[VI/Fe]? Abundance [VI/Fe]log(Sun)phys.abundfloatnullablee_[VI/Fe]? rms uncertainty on [VI/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[VI/Fe]? Number of lines for [VI/Fe]meta.numberintnullable[VII/Fe]? Abundance [VII/Fe]log(Sun)phys.abundfloatnullablee_[VII/Fe]? rms uncertainty on [VII/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[VII/Fe]? Number of lines for [VII/Fe]meta.numberintnullable[CrI/Fe]Abundance [CrI/Fe]phys.abundfloate_[CrI/Fe]rms uncertainty on [CrI/Fe]stat.error;phys.abundfloato_[CrI/Fe]Number of lines for [CrI/Fe]meta.numberint[CrII/Fe]Abundance [CrII/Fe]log(Sun)phys.abundfloate_[CrII/Fe]rms uncertainty on [CrII/Fe]log(Sun)stat.error;phys.abundfloato_[CrII/Fe]Number of lines for [CrII/Fe]meta.numberint[Mn/Fe]Abundance [Mn/Fe]log(Sun)phys.abundfloate_[Mn/Fe]rms uncertainty on [Mn/Fe]log(Sun)stat.error;phys.abundfloato_[Mn/Fe]Number of lines for [Mn/Fe]meta.numberint[Co/Fe]Abundance [Co/Fe]log(Sun)phys.abundfloate_[Co/Fe]rms uncertainty on [Co/Fe]log(Sun)stat.error;phys.abundfloato_[Co/Fe]Number of lines for [Co/Fe]meta.numberint[Ni/Fe]Abundance [Ni/Fe]log(Sun)phys.abundfloate_[Ni/Fe]rms uncertainty on [Ni/Fe]log(Sun)stat.error;phys.abundfloato_[Ni/Fe]Number of lines for [Ni/Fe]meta.numberint[Zn/Fe]? Abundance [Zn/Fe]log(Sun)phys.abundfloatnullablee_[Zn/Fe]? rms uncertainty on [Zn/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[Zn/Fe]? Number of lines for [Zn/Fe]meta.numberintnullablel_[Cu/Fe]Limit flag on [Cu/Fe]meta.code.error;phys.abundchar[Cu/Fe]Abundance [Cu/Fe]log(Sun)phys.abundfloate_[Cu/Fe]? rms uncertainty on [Cu/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[Cu/Fe]Number of lines for [Cu/Fe]meta.numberint[SrI/Fe]? Abundance [SrI/Fe]phys.abundfloatnullablee_[SrI/Fe]? rms uncertainty on [SrI/Fe]stat.error;phys.abundfloatnullableo_[SrI/Fe]? Number of lines for [SrI/Fe]meta.numberintnullable[YII/Fe]? Abundance [YII/Fe]log(Sun)phys.abundfloatnullablee_[YII/Fe]? rms uncertainty on [YII/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[YII/Fe]? Number of lines for [YII/Fe]meta.numberintnullable[ZrI/Fe]? Abundance [ZrI/Fe]log(Sun)phys.abundfloatnullablee_[ZrI/Fe]? rms uncertainty on [ZrI/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[ZrI/Fe]? Number of lines for [ZrI/Fe]meta.numberintnullable[ZrII/Fe]? Abundance [ZrII/Fe]log(Sun)phys.abundfloatnullablee_[ZrII/Fe]? rms uncertainty on [ZrII/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[ZrII/Fe]? Number of lines for [ZrII/Fe]meta.numberintnullable[Mo/Fe]? Abundance [Mo/Fe]log(Sun)phys.abundfloatnullablee_[Mo/Fe]? rms uncertainty on [Mo/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[Mo/Fe]? Number of lines for [Mo/Fe]meta.numberintnullable[BaII/Fe]? Abundance [BaII/Fe]log(Sun)phys.abundfloatnullablee_[BaII/Fe]? rms uncertainty on [BaII/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[BaII/Fe]? Number of lines for [BaII/Fe]meta.numberintnullable[LaII/Fe]Abundance [LaII/Fe]log(Sun)phys.abundfloate_[LaII/Fe]rms uncertainty on [LaII/Fe]log(Sun)stat.error;phys.abundfloato_[LaII/Fe]Number of lines for [LaII/Fe]meta.numberint[CeII/Fe]? Abundance [CeII/Fe]phys.abundfloatnullablee_[CeII/Fe]? rms uncertainty on [CeII/Fe]stat.error;phys.abundfloatnullableo_[CeII/Fe]? Number of lines for [CeII/Fe]meta.numberintnullable[PrII/Fe]? Abundance [PrII/Fe]log(Sun)phys.abundfloatnullablee_[PrII/Fe]? rms uncertainty on [PrII/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[PrII/Fe]? Number of lines for [PrII/Fe]meta.numberintnullable[NdII/Fe]? Abundance [NdII/Fe]log(Sun)phys.abundfloatnullablee_[NdII/Fe]? rms uncertainty on [NdII/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[NdII/Fe]? Number of lines for [NdII/Fe]meta.numberintnullable[SmII/Fe]? Abundance [SmII/Fe]log(Sun)phys.abundfloatnullablee_[SmII/Fe]? rms uncertainty on [SmII/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[SmII/Fe]? Number of lines for [SmII/Fe]meta.numberintnullable[EuII/Fe]Abundance [EuII/Fe]log(Sun)phys.abundfloate_[EuII/Fe]rms uncertainty on [EuII/Fe]log(Sun)stat.error;phys.abundfloato_[EuII/Fe]Number of lines for [EuII/Fe]meta.numberint[DyII/Fe]? Abundance [DyII/Fe]phys.abundfloatnullablee_[DyII/Fe]? rms uncertainty on [DyII/Fe]stat.error;phys.abundfloatnullableo_[DyII/Fe]? Number of lines for [DyII/Fe]meta.numberintnullable[ThII/Fe]? Abundance [ThII/Fe]log(Sun)phys.abundfloatnullablee_[ThII/Fe]? rms uncertainty on [ThII/Fe]log(Sun)stat.error;phys.abundfloatnullableo_[ThII/Fe]? Number of lines for [ThII/Fe]meta.numberintnullable_RAPosition, from Sandquist et al. 2004, Cat. J/ApJ/611/323 (right ascension part)degpos.eq.ra;meta.main_DEPosition, from Sandquist et al. 2004, Cat. J/ApJ/611/323 (declination part)degpos.eq.dec;meta.mainJ/AJ/141/62/table2Atomic parameters and equivalent widthsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharlambdaWavelength; in Angstroms0.1nmem.wlfloatIonElement identification (1)phys.atmol.ionStagefloatlog(gf)Log of the oscillator strengthphys.atmol.oscStrengthfloatEPExcitation potentialeVphys.atmol.excitationfloatRefReference (2)meta.ref;pos.frameintEWEquivalent width (m{AA})1e-13mspect.line.eqWidthfloat