J/AJ/169/279ivo://CDS.VizieR/J/AJ/169/279CDSOu X.Yelland A.Chiti A.Frebel A.Limberg G.Mardini M.K.2026-03-02T06:25:50Z2026-02-19T15:08:55ZCDS support team

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

cds-question@unistra.frchemical-abundancesdwarf-galaxiesradial-velocityphotometryvisible-astronomyinfrared-astronomyspectroscopychemically-peculiar-starsDwarf galaxies like Sagittarius (Sgr) provide a unique window into the early stages of galactic chemical evolution, particularly through their metal-poor stars. By studying the chemical abundances of stars in the Sgr core and tidal streams, we can gain insights into the assembly history of this galaxy and its early heavy element nucleosynthesis processes. We efficiently selected extremely metal-poor candidates in the core and streams for high-resolution spectroscopic analysis using metallicity-sensitive photometry from SkyMapper DR2 and Gaia DR3 XP spectra, and proper motions. We present a sample of 37 Sgr stars with detailed chemical abundances, of which we identify 10 extremely metal-poor ([Fe/H]<=-3.0) stars, 25 very metal-poor ([Fe/H]<=-2.0) stars, and two metal-poor ([Fe/H]<=-1.0) stars. This sample increases the number of extremely metal-poor Sgr stars analyzed with high-resolution spectroscopy by a factor of 5. Of these stars, 15 are identified as members of the Sgr tidal stream, while the remaining 22 are associated with the core. We derive abundances for up to 20 elements and identify no statistically significant differences between the element abundance patterns across the core and stream samples. Intriguingly, we identify stars that may have formed in ultrafaint dwarf galaxies that accreted onto Sgr, in addition to patterns of C and r-process elements distinct from the Milky Way halo. Over half of the sample shows a neutron-capture element abundance pattern consistent with the scaled solar pure r-process pattern, indicating early r-process enrichment in the Sgr progenitor.2025AJ....169..279Ohttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/169/279CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)J/AJ/113/634 : The survival of Sagittarius dwarf galaxy (Ibata+ 1997)J/ApJ/655/492 : Equivalent widths of 26 metal-poor stars (Aoki+, 2007)J/ApJ/701/1053 : Abundances of 8 stars in the Draco dSph (Cohen+, 2009)J/ApJ/724/341 : Nucleosynthesis of massive metal-free stars (Heger+, 2010)J/ApJ/724/975 : Heavy elements abundances of metal-poor stars (Roederer+, 2010)J/AJ/141/175 : Abundances in M15 RGB/RHB stars (Sobeck+, 2011)J/AJ/144/4 : Properties of dwarf gal. in the Local Group (McConnachie+, 2012)J/ApJ/769/57 : Equivalent widths of metal-poor stars (Frebel+, 2013)J/ApJ/779/102 : Metallicities of RGB stars in dwarf galaxies (Kirby+, 2013)J/ApJ/797/21 : Carbon-enhanced metal-poor stars (Placco+, 2014)J/ApJ/847/142 : Ultra-metal-poor stars LTE & NLTE abundances (Ezzeddine+, 2017)J/ApJ/838/44 : Abundances of the brightest member of Tuc III (Hansen+, 2017)J/ApJ/838/11 : Member stars in the MW satellite Tucana III (Simon+, 2017)J/ApJ/855/83 : Abund. of very metal-poor stars in Sagittarius (Hansen+, 2018)J/AJ/156/179 : Highly r-process-enhanced field stars kinem. (Roederer+, 2018)J/ApJ/870/83 : Abund. in the ultra-faint dwarf gal. GruI & TriII (Ji+, 2019)J/ApJ/882/177 : Abundances of 4 member stars of Tucana III (Marshall+, 2019)J/A+A/631/A171 : Neutron-capture elements in dwarf gal. (Skuladottir+, 2019)J/ApJ/898/150 : High-res. MIKE obs. of metal-poor stars (Ezzeddine+, 2020)J/ApJ/897/183 : Chem. abundances of 3 stars in Grus II galaxy (Hansen+, 2020)J/ApJ/889/63 : Properties of Sgr Stars (Hayes+, 2020)J/ApJS/249/30 : R-Process Alliance: metal-poor star spectr. (Holmbeck+, 2020)J/AJ/160/181 : Chemical abundances in red giants with Magellan (Ji+, 2020)J/ApJ/892/137 : Spectroscopy of Grus II, Tuc IV and Tuc V (Simon+, 2020)J/ApJS/254/31 : Phot. metallicities of stars in SkyMapper DR2 (Chiti+, 2021)J/MNRAS/501/2279 : Stars in the Sagittarius stream (Vasiliev+, 2021)J/A+A/666/A64 : Sagittarius stream with eDR3 (Ramos+, 2022)J/A+A/674/A33 : Gaia synthetic phot. cat. of white dwarfs (Gaia Coll., 2023)J/A+A/691/A226 : Abundances of globular cluster stars (Ceccarelli+, 2024)J/A+A/691/A333 : Gaia-Sausage-Enceladus abundances (Ernandes+, 2024)J/A+A/692/A115 : Pristine survey DR1 (Martin+, 2024)J/A+A/690/A333 : Pristine Inner Galaxy Survey. X. (Sestito+, 2024)J/A+A/689/A201 : Pristine Inner Galaxy Survey. IX. (Sestito+, 2024)J/MNRAS/537/1984 : CEMP prediction abundances (Ardern-Arentsen+, 2025)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/169/279https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/169/279http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/169/279https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/169/279https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/169/279http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/169/279GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/169/279/table3 (Chemical abundances for the Sgr sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/169/279/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/169/279/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/169/279/table3?GETtext/xml+votable180.050000true144.000035417.122610.0055555555555555566/4410 4451 5120 5130 25970 26342 26353 26387 26460 26478 26592 27695 27844 28331 28753 28756-28757 31374 47835 47860 47863 47919 48002 48005 48008 48012-48013 48025 48033 48038 48041 48049https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/169/279?format=asciiOpticalInfrareddefaultJ/AJ/169/279/table3Chemical abundances for the Sgr samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordinte_[EuII/H][0.06/0.16]? Uncertainty for [EuII/H]log(Sun)stat.error;phys.abundfloatnullableSimbadSimbad column added by the CDSmeta.ref.urlcharNameShort target name used in this studymeta.idcharl_[C/Fe]Upper limit flag for [C/Fe]meta.code.error;phys.abundcharGaiaDR3Gaia DR3 (I/355) source IDmeta.id;meta.mainRAICRSGaia DR3 right accension (ICRS, J2016)degpos.eq.ra;meta.mainDEICRSGaia DR3 declination (ICRS, J2016)degpos.eq.dec;meta.mainLambdaLongitude in the heliocentric Sgr coordinate system (1)degpos.framefloatBetaLatitude in the heliocentric Sgr coordinate system (1)degpos.framefloatMemClassification of the whether the star belongs to the Sgr core or stream (2)meta.code.membercharRVobs[-198.1/219.9] Observed radial velocitykm/sspect.dopplerVelocfloatcorrRVhel[-28.97/20.37] Heliocentric radial velocity correctionkm/sphys.veloc;arith.difffloatRVhel[-218.0/193.0] Corrected radial velocitykm/sspect.dopplerVelocfloatUTDateUTC date of the observation, YYYY-MM-DDtime.epoch;obsnullableUTTime[876/85938] UTC time stampstime.epochintBin[2x2] Binning during exposure readoutinstr.setupcharExpTime[600/5999] Total exposure timestime.duration;obs.exposureintSlit[1.0] Spectrum slit widtharcsecinstr.setupfloatTeffPh[4280/5274] Photometric effective temperatureKphys.temperature.effectiveintloggPh[0.4/2.6] Photometric surface gravitylog(cm.s**-2)phys.gravityfloatmZPh[-3.3/-1.79] Photometric model metallicitylog(Sun)phys.abund.ZfloatVtPh[1.38/2.51] Photometric microturbulencekm/sphys.veloc.microTurbfloate_TeffPh[122/123] Uncertainty for photometric effective temperatureKstat.error;phys.temperature.effectiveinte_loggPh[0.2/0.21] Uncertainty for photometric surface gravitylog(cm.s**-2)stat.error;phys.gravityfloate_mZPh[0.21/0.34] Uncertainty for photometric model metallicitylog(Sun)stat.error;phys.abund.Z;meta.modelledfloate_VtPh[0.25/0.58] Uncertainty for photometric microturbulencekm/sstat.error;phys.veloc.microTurbfloatTeffSp[4180/5200] Spectroscopic effective temperatureKphys.temperature.effectivefloatloggSp[0.05/2.55] Spectroscopic surface gravitylog(cm.s**-2)phys.gravityfloatVtSp[1.97/4.5] Spectroscopic microturbulencekm/sphys.veloc.microTurbfloatmZSp[-3.7/-2.1] Spectroscopic model metallicitylog(Sun)phys.abund.Zfloat[EuII/MgI][-0.74/0.64]? Relative abundance, [EuII/MgI]log(Sun)phys.abundfloatnullablee_[EuII/MgI][0.13/0.29]? Uncertainty for [EuII/MgI]log(Sun)stat.error;phys.abundfloatnullable[EuII/FeII][-0.58/1.14]? Relative abundance, [EuII/FeII]log(Sun)phys.abundfloatnullablee_[EuII/FeII][0.06/0.19]? Uncertainty for [EuII/FeII]log(Sun)stat.error;phys.abundfloatnullable[SrII/BaII][-0.82/1.66] Relative abundance, [SrII/BaII]log(Sun)phys.abundfloate_[SrII/BaII][0.05/0.4] Uncertainty for [SrII/BaII]log(Sun)stat.error;phys.abundfloat[SrII/MgI][-1.7/1.08] Relative abundance, [SrII/MgI]log(Sun)phys.abundfloate_[SrII/MgI][0.14/0.34] Uncertainty for [SrII/MgI]log(Sun)stat.error;phys.abundfloat[EuII/BaII][0.24/0.78]? Relative abundance, [EuII/BaII]log(Sun)phys.abundfloatnullablee_[EuII/BaII][0.06/0.23]? Uncertainty for [EuII/BaII]log(Sun)stat.error;phys.abundfloatnullable[EuII/SrII][-0.58/0.88]? Relative abundance, [EuII/SrII]log(Sun)phys.abundfloatnullablee_[EuII/SrII][0.12/0.33]? Uncertainty for [EuII/SrII]log(Sun)stat.error;phys.abundfloatnullable[C/Fe][-0.88/0.2] Relative abundance, [C/Fe]log(Sun)phys.abundfloate_[C/Fe][0.15/0.28] Uncertainty for [C/Fe]log(Sun)stat.error;phys.abundfloatcorr[C/Fe][-0.58/0.84] Evolution-corrected (based on Placco+2014, J/ApJ/797/21) relative abundance, [C/Fe]log(Sun)phys.abundfloat[NaI/Fe][-0.56/0.97] Relative abundance, [NaI/Fe]log(Sun)phys.abundfloate_[NaI/Fe][0.04/0.18] Uncertainty for [NaI/Fe]log(Sun)stat.error;phys.abundfloat[MgI/Fe][-0.21/0.5] Relative abundance, [MgI/Fe]log(Sun)phys.abundfloate_[MgI/Fe][0.05/0.16] Uncertainty for [Mg I/Fe]log(Sun)stat.error;phys.abundfloat[AlI/Fe][-1.46/0.15]? Relative abundance, [AlI/Fe]log(Sun)phys.abundfloatnullablee_[AlI/Fe][0.08/0.39]? Uncertainty for [AlI/Fe]log(Sun)stat.error;phys.abundfloatnullable[SiI/Fe][0.02/0.93] Relative abundance, [SiI/Fe]log(Sun)phys.abundfloate_[SiI/Fe][0.04/0.26] Uncertainty for [SiI/Fe]log(Sun)stat.error;phys.abundfloat[CaI/Fe][-0.06/0.48] Relative abundance, [CaI/Fe]log(Sun)phys.abundfloate_[CaI/Fe][0.04/0.13] Uncertainty for [CaI/Fe]log(Sun)stat.error;phys.abundfloat[ScII/Fe][-0.48/0.23] Relative abundance, [ScII/Fe]log(Sun)phys.abundfloate_[ScII/Fe][0.04/0.23] Uncertainty for [ScII/Fe]log(Sun)stat.error;phys.abundfloat[TiII/Fe][-0.01/0.41] Relative abundance, [TiII/Fe]log(Sun)phys.abundfloate_[TiII/Fe][0.06/0.21] Uncertainty for [TiII/Fe]log(Sun)stat.error;phys.abundfloat[CrI/Fe][-0.62/-0.1] Relative abundance, [CrI/Fe]log(Sun)phys.abundfloate_[CrI/Fe][0.05/0.19] Uncertainty for [CrI/Fe]log(Sun)stat.error;phys.abundfloat[CrII/Fe][-0.32/0.2]? Relative abundance, [CrII/Fe]log(Sun)phys.abundfloatnullablee_[CrII/Fe][0.04/0.18]? Uncertainty for [CrII/Fe]log(Sun)stat.error;phys.abundfloatnullable[MnI/Fe][-0.77/-0.18]? Relative abundance, [MnI/Fe]log(Sun)phys.abundfloatnullablee_[MnI/Fe][0.08/0.16]? Uncertainty for [MnI/Fe]log(Sun)stat.error;phys.abundfloatnullable[CoI/Fe][-0.45/0.58]? Relative abundance, [CoI/Fe]log(Sun)phys.abundfloatnullablee_[CoI/Fe][0.05/0.42]? Uncertainty for [CoI/Fe]log(Sun)stat.error;phys.abundfloatnullable[NiI/Fe][-0.27/0.37] Relative abundance, [NiI/Fe]log(Sun)phys.abundfloate_[NiI/Fe][0.03/0.18] Uncertainty for [NiI/Fe]log(Sun)stat.error;phys.abundfloat[ZnI/Fe][-0.3/0.99]? Relative abundance, [ZnI/Fe]log(Sun)phys.abundfloatnullablee_[ZnI/Fe][0.06/0.28]? Uncertainty for [ZnI/Fe]log(Sun)stat.error;phys.abundfloatnullable[SrII/Fe][-1.37/1.03] Relative abundance, [SrII/Fe]log(Sun)phys.abundfloate_[SrII/Fe][0.11/0.36] Uncertainty for [SrII/Fe]log(Sun)stat.error;phys.abundfloat[YII/Fe][-0.77/0.32] Relative abundance, [YII/Fe]log(Sun)phys.abundfloate_[YII/Fe][0.07/0.2]? Uncertainty for [YII/Fe]log(Sun)stat.error;phys.abundfloatnullable[ZrII/Fe][-0.38/0.52] Relative abundance, [ZrII/Fe]log(Sun)phys.abundfloate_[ZrII/Fe][0.04/0.14]? Uncertainty for [ZrII/Fe]log(Sun)stat.error;phys.abundfloatnullable[BaII/Fe][-1.42/0.47] Relative abundance, [BaII/Fe]log(Sun)phys.abundfloate_[BaII/Fe][0.05/0.22] Uncertainty for [BaII/Fe]log(Sun)stat.error;phys.abundfloat[LaII/Fe][-0.49/0.69]? Relative abundance, [LaII/Fe]log(Sun)phys.abundfloatnullablee_[LaII/Fe][0.07/0.18]? Uncertainty for [LaII/Fe]log(Sun)stat.error;phys.abundfloatnullable[EuII/Fe][-0.58/1.14] Relative abundance, [EuII/Fe]log(Sun)phys.abundfloate_[EuII/Fe][0.06/0.19]? Uncertainty for [EuII/Fe]log(Sun)stat.error;phys.abundfloatnullable[DyII/Fe][-0.17/1.49] Relative abundance, [DyII/Fe]log(Sun)phys.abundfloate_[DyII/Fe][0.07/0.17]? Uncertainty for [DyII/Fe]log(Sun)stat.error;phys.abundfloatnullable[C/H][-3.95/-2.33] Relative abundance, [C/H]log(Sun)phys.abundfloate_[C/H][0.1/0.33] Uncertainty for [C/H]log(Sun)stat.error;phys.abundfloat[NaI/H][-3.1/-1.7] Relative abundance, [NaI/H]log(Sun)phys.abundfloate_[NaI/H][0.16/0.38] Uncertainty for [NaI/H]log(Sun)stat.error;phys.abundfloat[MgI/H][-3.27/-1.75] Relative abundance, [MgI/H]log(Sun)phys.abundfloate_[MgI/H][0.09/0.29] Uncertainty for [MgI/H]log(Sun)stat.error;phys.abundfloat[AlI/H][-4.07/-2.52]? Relative abundance, [AlI/H]log(Sun)phys.abundfloatnullablee_[AlI/H][0.1/0.5]? Uncertainty for [AlI/H]log(Sun)stat.error;phys.abundfloatnullable[SiI/H][-2.69/-1.51] Relative abundance, [SiI/H]log(Sun)phys.abundfloate_[SiI/H][0.16/0.32] Uncertainty for [SiI/H]log(Sun)stat.error;phys.abundfloat[CaI/H][-3.02/-1.48] Relative abundance, [CaI/H]log(Sun)phys.abundfloate_[CaI/H][0.06/0.21] Uncertainty for [CaI/H]log(Sun)stat.error;phys.abundfloat[ScII/H][-3.1/-1.71] Relative abundance, [ScII/H]log(Sun)phys.abundfloate_[ScII/H][0.07/0.26] Uncertainty for [ScII/H]log(Sun)stat.error;phys.abundfloat[TiII/H][-3.01/-1.27] Relative abundance, [TiII/H]log(Sun)phys.abundfloate_[TiII/H][0.1/0.24] Uncertainty for [TiII/H]log(Sun)stat.error;phys.abundfloat[CrI/H][-3.78/-2.01] Relative abundance, [CrI/H]log(Sun)phys.abundfloate_[CrI/H][0.11/0.38] Uncertainty for [CrI/H]log(Sun)stat.error;phys.abundfloat[CrII/H][-3.13/-1.64]? Relative abundance, [CrII/H]log(Sun)phys.abundfloatnullablee_[CrII/H][0.07/0.2]? Uncertainty for [CrII/H]log(Sun)stat.error;phys.abundfloatnullable[MnI/H][-3.9/-2.32]? Relative abundance, [MnI/H]log(Sun)phys.abundfloatnullablee_[MnI/H][0.05/0.15]? Uncertainty for [MnI/H]log(Sun)stat.error;phys.abundfloatnullable[CoI/H][-3.26/-1.79]? Relative abundance, [CoI/H]log(Sun)phys.abundfloatnullablee_[CoI/H][0.1/0.35]? Uncertainty for [CoI/H]log(Sun)stat.error;phys.abundfloatnullable[NiI/H][-3.38/-1.85] Relative abundance, [NiI/H]log(Sun)phys.abundfloate_[NiI/H][0.09/0.28] Uncertainty for [NiI/H]log(Sun)stat.error;phys.abundfloat[ZnI/H][-3.08/-1.79]? Relative abundance, [ZnI/H]log(Sun)phys.abundfloatnullablee_[ZnI/H][0.03/0.09]? Uncertainty for [ZnI/H]log(Sun)stat.error;phys.abundfloatnullable[SrII/H][-4.51/-1.66] Relative abundance, [SrII/H]log(Sun)phys.abundfloate_[SrII/H][0.12/0.46] Uncertainty for [SrII/H]log(Sun)stat.error;phys.abundfloat[YII/H][-3.66/-2.01] Relative abundance, [YII/H]log(Sun)phys.abundfloate_[YII/H][0.07/0.19]? Uncertainty for [YII/H]log(Sun)stat.error;phys.abundfloatnullable[ZrII/H][-3.16/-1.46] Relative abundance, [ZrII/H]log(Sun)phys.abundfloate_[ZrII/H][0.06/0.19]? Uncertainty for [ZrII/H]log(Sun)stat.error;phys.abundfloatnullable[BaII/H][-4.58/-1.5] Relative abundance, [BaII/H]log(Sun)phys.abundfloate_[BaII/H][0.07/0.24] Uncertainty for [BaII/H]log(Sun)stat.error;phys.abundfloat[LaII/H][-3.13/-1.47]? Relative abundance, [LaII/H]log(Sun)phys.abundfloatnullablee_[LaII/H][0.06/0.15]? Uncertainty for [LaII/H]log(Sun)stat.error;phys.abundfloatnullable[EuII/H][-3.25/-1.11] Relative abundance, [EuII/H]log(Sun)phys.abundfloat[DyII/H][-3.06/-1.07] Relative abundance, [DyII/H]log(Sun)phys.abundfloate_[DyII/H][0.07/0.18]? Uncertainty for [DyII/H]log(Sun)stat.error;phys.abundfloatnullable[Fe/H][-3.29/-1.85] Relative abundance, [Fe/H]log(Sun)phys.abundfloate_[Fe/H][0.08/0.24] Uncertainty for [Fe/H]log(Sun)stat.error;phys.abundfloat[alpha/Fe][-0.06/0.52] Relative abundance, [alpha/Fe]log(Sun)phys.abundfloatl_[NaI/Fe]Upper limit flag for [NaI/Fe]meta.code.error;phys.abundcharl_[MgI/Fe]Upper limit flag for [MgI/Fe]meta.code.error;phys.abundcharl_[AlI/Fe]Upper limit flag for [AlI/Fe]meta.code.error;phys.abundcharl_[SiI/Fe]Upper limit flag for [SiI/Fe]meta.code.error;phys.abundcharl_[CaI/Fe]Upper limit flag for [CaI/Fe]meta.code.error;phys.abundcharl_[ScII/Fe]Upper limit flag for [ScII/Fe]meta.code.error;phys.abundcharl_[TiII/Fe]Upper limit flag for [TiII/Fe]meta.code.error;phys.abundcharl_[CrI/Fe]Upper limit flag for [CrI/Fe]meta.code.error;phys.abundcharl_[CrII/Fe]Upper limit flag for [CrII/Fe]meta.code.error;phys.abundcharl_[MnI/Fe]Upper limit flag for [MnI/Fe]meta.code.error;phys.abundcharl_[CoI/Fe]Upper limit flag for [CoI/Fe]meta.code.error;phys.abundcharl_[NiI/Fe]Upper limit flag for [NiI/Fe]meta.code.error;phys.abundcharl_[ZnI/Fe]Upper limit flag for [ZnI/Fe]meta.code.error;phys.abundcharl_[SrII/Fe]Upper limit flag for [SrII/Fe]meta.code.error;phys.abundcharl_[YII/Fe]Upper limit flag for [YII/Fe]meta.code.error;phys.abundcharl_[ZrII/Fe]Upper limit flag for [ZrII/Fe]meta.code.error;phys.abundcharl_[BaII/Fe]Upper limit flag for [BaII/Fe]meta.code.error;phys.abundcharl_[LaII/Fe]Upper limit flag for [LaII/Fe]meta.code.error;phys.abundcharl_[EuII/Fe]Upper limit flag for [EuII/Fe]meta.code.error;phys.abundcharl_[DyII/Fe]Upper limit flag for [DyII/Fe]meta.code.error;phys.abundcharl_[C/H]Upper limit flag for [C/H]meta.code.error;phys.abundcharl_[NaI/H]Upper limit flag for [NaI/H]meta.code.error;phys.abundcharl_[MgI/H]Upper limit flag for [MgI/H]meta.code.error;phys.abundcharl_[AlI/H]Upper limit flag for [AlI/H]meta.code.error;phys.abundcharl_[SiI/H]Upper limit flag for [SiI/H]meta.code.error;phys.abundcharl_[CaI/H]Upper limit flag for [CaI/H]meta.code.error;phys.abundcharl_[ScII/H]Upper limit flag for [ScII/H]meta.code.error;phys.abundcharl_[TiII/H]Upper limit flag for [TiII/H]meta.code.error;phys.abundcharl_[CrI/H]Upper limit flag for [CrI/H]meta.code.error;phys.abundcharl_[CrII/H]Upper limit flag for [CrII/H]meta.code.error;phys.abundcharl_[MnI/H]Upper limit flag for [MnI/H]meta.code.error;phys.abundcharl_[CoI/H]Upper limit flag for [CoI/H]meta.code.error;phys.abundcharl_[NiI/H]Upper limit flag for [NiI/H]meta.code.error;phys.abundcharl_[ZnI/H]Upper limit flag for [ZnI/H]meta.code.error;phys.abundcharl_[SrII/H]Upper limit flag for [SrII/H]meta.code.error;phys.abundcharl_[YII/H]Upper limit flag for [YII/H]meta.code.error;phys.abundcharl_[ZrII/H]Upper limit flag for [ZrII/H]meta.code.error;phys.abundcharl_[BaII/H]Upper limit flag for [BaII/H]meta.code.error;phys.abundcharl_[LaII/H]Upper limit flag for [LaII/H]meta.code.error;phys.abundcharl_[EuII/H]Upper limit flag for [EuII/H]meta.code.error;phys.abundcharl_[DyII/H]Upper limit flag for [DyII/H]meta.code.error;phys.abundcharl_[alpha/Fe]Upper limit flag for [alpha/Fe]meta.code.error;phys.abundchar