J/A+A/660/A88ivo://CDS.VizieR/J/A+A/660/A88doi:10.26093/cds/vizier.36600088CDSLarsen S.S.Eitner P.Magg E.Bergemann M.Moltzer C.A.S.Brodie J.P.,Romanowsky A.J.Strader J.2023-11-07T10:18:54Z2022-04-14T13:09:06ZCDS support team

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

cds-question@unistra.frglobular-star-clusterschemical-abundancesmetallicityspectroscopyvisible-astronomyWe present detailed abundance measurements for 45 globular clusters (GCs) in galaxies in (and, in one case, beyond) the Local Group. The measurements are based on new high-resolution integrated-light spectra of GCs in NGC 185, NGC 205, M31, M33, and NGC 2403, combined with reanalysis of previous observations of GCs in the Fornax dSph, WLM, NGC 147, NGC 6822, and the Milky Way. The GCs cover the range -2.8<[Fe/H]<-0.1 and we determined abundances for Fe, Na, Mg, Si, Ca, Sc, Ti, Cr, Mn, Ni, Cu, Zn, Zr, Ba, and Eu. Corrections for non local thermodynamic equilibrium effects are included for Na, Mg, Ca, Ti, Mn, Fe, Ni, and Ba. For several of the galaxies, our measurements provide the first quantitative constraints on the detailed composition of their metal-poor stellar populations. Overall, the GCs in different galaxies exhibit remarkably uniform abundance patterns of the alpha-, iron-peak, and neutron-capture elements, with a dispersion of less than 0.1dex in [alpha/Fe] for the full sample. There is a hint that GCs in dwarf galaxies are slightly less alpha-enhanced (by about 0.04 dex on average) than those in larger galaxies. One GC in M33 (HM33-B) resembles the most metal-rich GCs in the Fornax dSph (Fornax 4) and NGC 6822 (SC7) by having alpha-element abundances closer to scaled-solar values, possibly hinting at an accretion origin. We find that the alpha-element abundances strongly correlate with those of Na, Sc, Ni, and Zn. Several GCs with [Fe/H]<-1.5 are deficient in Mg compared to other alpha-elements. We find no GCs with strongly enhanced r-process abundances as reported for metal-poor stars in some ultra-faint dwarfs and the Magellanic Clouds. The similarity of the abundance patterns for metal-poor GCs in different environments points to similar early enrichment histories and only allow for minor variations in the initial mass function.2022A&A...660A..88Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/660/A88CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/660/A88https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/660/A88http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/660/A88https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/660/A88https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/660/A88http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/660/A88GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/660/A88/sources (List of studied clusters + Arcturus and the Sun (with data in tablef1.dat))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/660/A88/sources?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/660/A88/sources?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/660/A88/sources?GETtext/xml+votable180.050000true6.023625-72.08127780.0055555555555555566/2153 2155 2622-2623 2665 2708-2709 2774 2777 2779 7743 8767 12405 17165 29718 31019 33321 33330 35969 42314 47125 48434https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/660/A88?format=asciiOpticaldefaultJ/A+A/660/A88/sourcesList of studied clusters + Arcturus and the Sun (with data in tablef1.dat)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDSource IDmeta.id;meta.maincharRAJ2000? Right ascension (J2000)pos.eq.ra;meta.mainnullableDEJ2000? Declination (J2000)pos.eq.dec;meta.mainnullableSNameSimbad Namemeta.idcharAbundIndDisplay the individual abundance measurements (DSEP) in table f1meta.ref.urlcharAbundDisplay the Mean DSEP and BaSTI NLTE abundancesmeta.ref.urlcharJ/A+A/660/A88/tableb1Spectral window definitionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElemElementphys.atmol.elementcharlam-minBlue edge of window in Angstrom0.1nminstr.bandwidthfloatlam-maxRed edge of window in Angstrom0.1nminstr.bandwidthfloatCommentComment (1)meta.notecharJ/A+A/660/A88/tablec1Mean DSEP NLTE abundances: Fe, Na, Mg, Si, Ca, TirecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.mainchar[Fe/H]Mean [Fe/H] valuelog(Sun)phys.abund.Fe;stat.meanfloate_[Fe/H]Uncertainty on [Fe/H] from error propagationlog(Sun)stat.error;phys.abund.Fefloats_[Fe/H]Standard error on [Fe/H] from dispersion of individual measurementslog(Sun)stat.error;phys.abund.Fefloato_[Fe/H]Number of [Fe/H] measurementsmeta.numberint[Na/Fe]? Mean [Na/Fe] valuelog(Sun)phys.abundfloatnullablee_[Na/Fe]? Uncertainty on [Na/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Na/Fe]? Standard error on [Na/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Na/Fe]Number of [Na/Fe] measurementsmeta.numberint[Mg/Fe]Mean [Mg/Fe] valuelog(Sun)phys.abundfloate_[Mg/Fe]Uncertainty on [Mg/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Mg/Fe]Standard error on [Mg/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Mg/Fe]Number of [Mg/Fe] measurementsmeta.numberint[Si/Fe]? Mean [Si/Fe] valuelog(Sun)phys.abundfloatnullablee_[Si/Fe]? Uncertainty on [Si/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Si/Fe]? Standard error on [Si/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Si/Fe]Number of [Si/Fe] measurementsmeta.numberint[Ca/Fe]Mean [Ca/Fe] valuelog(Sun)phys.abundfloate_[Ca/Fe]Uncertainty on [Ca/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ca/Fe]Standard error on [Ca/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ca/Fe]Number of [Ca/Fe] measurementsmeta.numberint[Ti/Fe]Mean [Ti/Fe] valuelog(Sun)phys.abundfloate_[Ti/Fe]Uncertainty on [Ti/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ti/Fe]Standard error on [Ti/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ti/Fe]Number of [Ti/Fe] measurementsmeta.numberintJ/A+A/660/A88/tablec2Mean DSEP NLTE abundances: Sc, Cr, Mn, NiIDCluster IDmeta.id;meta.mainchare_[Ni/Fe]Uncertainty on [Ni/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[Sc/Fe]Mean [Sc/Fe] valuelog(Sun)phys.abundfloate_[Sc/Fe]Uncertainty on [Sc/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Sc/Fe]Standard error on [Sc/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Sc/Fe]Number of [Sc/Fe] measurementsmeta.numberint[Cr/Fe]Mean [Cr/Fe] valuelog(Sun)phys.abundfloate_[Cr/Fe]Uncertainty on [Cr/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Cr/Fe]Standard error on [Cr/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Cr/Fe]Number of [Cr/Fe] measurementsmeta.numberint[Mn/Fe]Mean [Mn/Fe] valuelog(Sun)phys.abundfloate_[Mn/Fe]Uncertainty on [Mn/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Mn/Fe]? Standard error on [Mn/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Mn/Fe]Number of [Mn/Fe] measurementsmeta.numberint[Ni/Fe]Mean [Ni/Fe] valuelog(Sun)phys.abundfloats_[Ni/Fe]Standard error on [Ni/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ni/Fe]Number of [Ni/Fe] measurementsmeta.numberintJ/A+A/660/A88/tablec3Mean DSEP NLTE abundances: Cu, Zn, Zr, Ba, Eu[Zn/Fe]? Mean [Zn/Fe] valuelog(Sun)phys.abundfloatnullablee_[Zn/Fe]? Uncertainty on [Zn/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Zn/Fe]? Standard error on [Zn/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Zn/Fe]Number of [Zn/Fe] measurementsmeta.numberint[Zr/Fe]? Mean [Zr/Fe] valuelog(Sun)phys.abundfloatnullablee_[Zr/Fe]? Uncertainty on [Zr/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Zr/Fe]? Standard error on [Zr/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Zr/Fe]Number of [Zr/Fe] measurementsmeta.numberint[Ba/Fe]Mean [Ba/Fe] valuelog(Sun)phys.abundfloate_[Ba/Fe]Uncertainty on [Ba/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ba/Fe]Standard error on [Ba/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ba/Fe]Number of [Ba/Fe] measurementsmeta.numberint[Eu/Fe]? Mean [Eu/Fe] valuelog(Sun)phys.abundfloatnullablee_[Eu/Fe]? Uncertainty on [Eu/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Eu/Fe]? Standard error on [Eu/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Eu/Fe]Number of [Eu/Fe] measurementsmeta.numberintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.mainchar[Cu/Fe]? Mean [Cu/Fe] valuelog(Sun)phys.abundfloatnullablee_[Cu/Fe]? Uncertainty on [Cu/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Cu/Fe]? Standard error on [Cu/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Cu/Fe]Number of [Cu/Fe] measurementsmeta.numberintJ/A+A/660/A88/tabled1Mean DSEP LTE abundances: Fe, Na, Mg, Si, Ca, Tio_[Na/Fe]Number of [Na/Fe] measurementsmeta.numberintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.mainchar[Fe/H]Mean [Fe/H] valuelog(Sun)phys.abund.Fe;stat.meanfloate_[Fe/H]Uncertainty on [Fe/H] from error propagationlog(Sun)stat.error;phys.abund.Fefloats_[Fe/H]Standard error on [Fe/H] from dispersion of individual measurementslog(Sun)stat.error;phys.abund.Fefloato_[Fe/H]Number of [Fe/H] measurementsmeta.numberint[Na/Fe]? Mean [Na/Fe] valuelog(Sun)phys.abundfloatnullablee_[Na/Fe]? Uncertainty on [Na/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Na/Fe]? Standard error on [Na/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullable[Mg/Fe]Mean [Mg/Fe] valuelog(Sun)phys.abundfloate_[Mg/Fe]Uncertainty on [Mg/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Mg/Fe]Standard error on [Mg/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Mg/Fe]Number of [Mg/Fe] measurementsmeta.numberint[Si/Fe]? Mean [Si/Fe] valuelog(Sun)phys.abundfloatnullablee_[Si/Fe]? Uncertainty on [Si/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Si/Fe]? Standard error on [Si/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Si/Fe]Number of [Si/Fe] measurementsmeta.numberint[Ca/Fe]Mean [Ca/Fe] valuelog(Sun)phys.abundfloate_[Ca/Fe]Uncertainty on [Ca/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ca/Fe]Standard error on [Ca/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ca/Fe]Number of [Ca/Fe] measurementsmeta.numberint[Ti/Fe]Mean [Ti/Fe] valuelog(Sun)phys.abundfloate_[Ti/Fe]Uncertainty on [Ti/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ti/Fe]Standard error on [Ti/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ti/Fe]Number of [Ti/Fe] measurementsmeta.numberintJ/A+A/660/A88/tabled2Mean DSEP LTE abundances: Sc, Cr, Mn, NiIDCluster IDmeta.id;meta.mainchar[Mn/Fe]Mean [Mn/Fe] valuelog(Sun)phys.abundfloate_[Mn/Fe]Uncertainty on [Mn/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Mn/Fe]? Standard error on [Mn/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Mn/Fe]Number of [Mn/Fe] measurementsmeta.numberint[Ni/Fe]Mean [Ni/Fe] valuelog(Sun)phys.abundfloate_[Ni/Fe]Uncertainty on [Ni/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ni/Fe]Standard error on [Ni/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ni/Fe]Number of [Ni/Fe] measurementsmeta.numberintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[Sc/Fe]Mean [Sc/Fe] valuelog(Sun)phys.abundfloate_[Sc/Fe]Uncertainty on [Sc/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Sc/Fe]Standard error on [Sc/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Sc/Fe]Number of [Sc/Fe] measurementsmeta.numberint[Cr/Fe]Mean [Cr/Fe] valuelog(Sun)phys.abundfloate_[Cr/Fe]Uncertainty on [Cr/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Cr/Fe]Standard error on [Cr/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Cr/Fe]Number of [Cr/Fe] measurementsmeta.numberintJ/A+A/660/A88/tabled3Mean DSEP LTE abundances: Cu, Zn, Zr, Ba, Eu[Ba/Fe]Mean [Ba/Fe] valuelog(Sun)phys.abundfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.mainchar[Cu/Fe]? Mean [Cu/Fe] valuelog(Sun)phys.abundfloatnullablee_[Cu/Fe]? Uncertainty on [Cu/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Cu/Fe]? Standard error on [Cu/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Cu/Fe]Number of [Cu/Fe] measurementsmeta.numberint[Zn/Fe]? Mean [Zn/Fe] valuelog(Sun)phys.abundfloatnullablee_[Zn/Fe]? Uncertainty on [Zn/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Zn/Fe]? Standard error on [Zn/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullable[Zr/Fe]? Mean [Zr/Fe] valuelog(Sun)phys.abundfloatnullablee_[Zr/Fe]? Uncertainty on [Zr/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Zr/Fe]? Standard error on [Zr/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Zr/Fe]Number of [Zr/Fe] measurementsmeta.numberinte_[Ba/Fe]Uncertainty on [Ba/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ba/Fe]Standard error on [Ba/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ba/Fe]Number of [Ba/Fe] measurementsmeta.numberint[Eu/Fe]? Mean [Eu/Fe] valuelog(Sun)phys.abundfloatnullablee_[Eu/Fe]? Uncertainty on [Eu/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Eu/Fe]? Standard error on [Eu/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Eu/Fe]Number of [Eu/Fe] measurementsmeta.numberinto_[Zn/Fe]Number of [Zn/Fe] measurementsmeta.numberintJ/A+A/660/A88/tablee1Mean BaSTI NLTE abundances: Fe, Na, Mg, Si, Ca, TirecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.mainchar[Fe/H]Mean [Fe/H] valuelog(Sun)phys.abund.Fe;stat.meanfloate_[Fe/H]Uncertainty on [Fe/H] from error propagationlog(Sun)stat.error;phys.abund.Fefloats_[Fe/H]Standard error on [Fe/H] from dispersion of individual measurementslog(Sun)stat.error;phys.abund.Fefloato_[Fe/H]Number of [Fe/H] measurementsmeta.numberint[Na/Fe]? Mean [Na/Fe] valuelog(Sun)phys.abundfloatnullablee_[Na/Fe]? Uncertainty on [Na/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Na/Fe]? Standard error on [Na/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Na/Fe]Number of [Na/Fe] measurementsmeta.numberint[Mg/Fe]Mean [Mg/Fe] valuelog(Sun)phys.abundfloate_[Mg/Fe]Uncertainty on [Mg/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Mg/Fe]Standard error on [Mg/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Mg/Fe]Number of [Mg/Fe] measurementsmeta.numberint[Si/Fe]? Mean [Si/Fe] valuelog(Sun)phys.abundfloatnullablee_[Si/Fe]? Uncertainty on [Si/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Si/Fe]? Standard error on [Si/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Si/Fe]Number of [Si/Fe] measurementsmeta.numberint[Ca/Fe]Mean [Ca/Fe] valuelog(Sun)phys.abundfloate_[Ca/Fe]Uncertainty on [Ca/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ca/Fe]Standard error on [Ca/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ca/Fe]Number of [Ca/Fe] measurementsmeta.numberint[Ti/Fe]Mean [Ti/Fe] valuelog(Sun)phys.abundfloate_[Ti/Fe]Uncertainty on [Ti/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ti/Fe]Standard error on [Ti/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ti/Fe]Number of [Ti/Fe] measurementsmeta.numberintJ/A+A/660/A88/tablee3Mean BaSTI NLTE abundances: Cu, Zn, Zr, Ba, Eu[Zr/Fe]? Mean [Zr/Fe] valuelog(Sun)phys.abundfloatnullablee_[Cu/Fe]? Uncertainty on [Cu/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.mainchar[Cu/Fe]? Mean [Cu/Fe] valuelog(Sun)phys.abundfloatnullables_[Cu/Fe]? Standard error on [Cu/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Cu/Fe]Number of [Cu/Fe] measurementsmeta.numberint[Zn/Fe]? Mean [Zn/Fe] valuelog(Sun)phys.abundfloatnullablee_[Zn/Fe]? Uncertainty on [Zn/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Zn/Fe]? Standard error on [Zn/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Zn/Fe]Number of [Zn/Fe] measurementsmeta.numberinte_[Zr/Fe]? Uncertainty on [Zr/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Zr/Fe]? Standard error on [Zr/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Zr/Fe]Number of [Zr/Fe] measurementsmeta.numberint[Ba/Fe]Mean [Ba/Fe] valuelog(Sun)phys.abundfloate_[Ba/Fe]Uncertainty on [Ba/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ba/Fe]Standard error on [Ba/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ba/Fe]Number of [Ba/Fe] measurementsmeta.numberint[Eu/Fe]? Mean [Eu/Fe] valuelog(Sun)phys.abundfloatnullablee_[Eu/Fe]? Uncertainty on [Eu/Fe] from error propagationlog(Sun)stat.error;phys.abundfloatnullables_[Eu/Fe]? Standard error on [Eu/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Eu/Fe]Number of [Eu/Fe] measurementsmeta.numberintJ/A+A/660/A88/tablee2Mean BaSTI NLTE abundances: Sc, Cr, Mn, NirecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster IDmeta.id;meta.mainchar[Sc/Fe]Mean [Sc/Fe] valuelog(Sun)phys.abundfloate_[Sc/Fe]Uncertainty on [Sc/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Sc/Fe]Standard error on [Sc/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Sc/Fe]Number of [Sc/Fe] measurementsmeta.numberint[Cr/Fe]Mean [Cr/Fe] valuelog(Sun)phys.abundfloate_[Cr/Fe]Uncertainty on [Cr/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Cr/Fe]Standard error on [Cr/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Cr/Fe]Number of [Cr/Fe] measurementsmeta.numberint[Mn/Fe]Mean [Mn/Fe] valuelog(Sun)phys.abundfloate_[Mn/Fe]Uncertainty on [Mn/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Mn/Fe]? Standard error on [Mn/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloatnullableo_[Mn/Fe]Number of [Mn/Fe] measurementsmeta.numberint[Ni/Fe]Mean [Ni/Fe] valuelog(Sun)phys.abundfloate_[Ni/Fe]Uncertainty on [Ni/Fe] from error propagationlog(Sun)stat.error;phys.abundfloats_[Ni/Fe]Standard error on [Ni/Fe] from dispersion of individual measurementslog(Sun)stat.error;phys.abundfloato_[Ni/Fe]Number of [Ni/Fe] measurementsmeta.numberintJ/A+A/660/A88/tablef1Individual abundance measurements (DSEP)e_[X/H]LTE? Uncertainty on LTE abundancelog(Sun)stat.error;phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDSource IDmeta.id;meta.maincharlam-minBlue edge of fit range0.1nminstr.bandwidthfloatlam-maxRed edge of fit range0.1nminstr.bandwidthfloat[X/H]LTE? LTE abundance relative to Hlog(Sun)phys.abund;arith.ratiofloatnullableDNLTE? NLTE abundance correctionlog(Sun)arith.factorfloatnullableElementElement measuredphys.atmol.elementchar