J/ApJ/921/118ivo://CDS.VizieR/J/ApJ/921/118doi:10.26093/cds/vizier.19210118CDSNelson T.Ting Y.-S.Hawkins K.Ji A.Kamdar H.El-Badry K.2024-05-29T08:19:44Z2023-03-29T12:16:11ZCDS support team

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

cds-question@unistra.frchemical-abundancesmultiple-starsvisible-astronomyspectroscopyradial-velocityComoving pairs, even at the separations of O(10^6^)au, are a predicted reservoir of conatal stars. We present detailed chemical abundances of 62 stars in 31 comoving pairs with separations of 10^2^-10^7^ au and 3D velocity differences <2km/s. This sample includes both bound comoving pairs/wide binaries and unbound comoving pairs. Observations were taken using the Magellan Inamori Kyocera Echelle (MIKE) spectrograph on board the Magellan/Clay Telescope at high resolution (R~45000) with a typical signal-to-noise ratio of 150pixel^-1^. With these spectra, we measure surface abundances for 24 elements, including Li, C, Na, Mg, Al, Si, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Sr, Y, Zr, Ba, La, Nd, and Eu. Taking iron as the representative element, our sample of wide binaries is chemically homogeneous at the level of 0.05dex, which agrees with prior studies on wide binaries. Importantly, even systems at separations 2x10^5^-10^7^au are homogeneous to 0.09dex, as opposed to the random pairs, which have a dispersion of 0.23dex. Assuming a mixture model of the wide binaries and random pairs, we find that 73+/-22% of the comoving pairs at separations 2x10^5^-10^7^au are conatal. Our results imply that a much larger parameter space of phase space may be used to find conatal stars, to study M-dwarfs, star cluster evolution, exoplanets, chemical tagging, and beyond.2021ApJ...921..118Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/921/118CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVI/10 : Semiempirical gf Values (Kurucz + 1975)I/345 : Gaia DR2 (Gaia Collaboration, 2018)I/350 : Gaia EDR3 (Gaia Collaboration, 2020)J/A+AS/102/435 : Transitions of SI in visible and infra-red (Biemont+ 1993)J/A+AS/130/541 : Co II oscillator strengths (Raassen+ 1998)J/A+A/340/300 : Fe II oscillator strengths (Raassen+ 1998)J/ApJS/167/292 : Laboratory transition prob. for Gd II (Den Hartog+, 2006)J/ApJS/162/227 : Transition probabilities for SmII (Lawler+, 2006)J/ApJS/169/120 : Transition probabilities for HfII and Hf (Lawler+, 2007)J/AJ/133/889 : Faint companions of Hipparcos stars (Lepine+, 2007)J/ApJ/667/1267 : CrI transition probabilities (Sobeck+, 2007)J/ApJS/182/51 : Transition prob. of rare earth elements (Lawler+, 2009)J/A+A/511/A68 : Transitions of CrII (Gurell+, 2010)J/ApJS/194/35 : Atomic transition probabilities of Mn (Den Hartog+, 2011)J/ApJ/737/L32 : Abundances of 16 Cyg A and B (Schuler+, 2011)J/ApJ/756/46 : Lithium abundances in HIP stars (Ramirez+, 2012)J/ApJ/758/133 : Metallicity profile of M31 HII reg. and PNe (Sanders+, 2012)J/MNRAS/429/126 : Atmospheric parameters from Fe lines (Ruchti+, 2013)J/ApJS/208/27 : Sun and HD 84937 TiII log(gf) and abundances (Wood+, 2013)J/A+A/566/A98 : The Gaia Benchmark Stars - Library (Blanco-Cuaresma+, 2014)J/ApJS/215/23 : FeI radiative lifetimes (Den Hartog+, 2014)J/A+A/564/A133 : Gaia FGK benchmark stars: metallicity (Jofre+, 2014)J/A+A/571/A47 : Extensive linelist of CH in stellar atm. (Masseron+, 2014)J/MNRAS/441/3127 : FeI oscillator strengths for Gaia-ESO (Ruffoni+, 2014)J/ApJS/211/20 : NiI transition probability measurements (Wood+, 2014)J/ApJ/815/63 : SDSS wide double white dwarfs spectroscopy (Andrews+, 2015)J/AJ/151/144 : ASPCAP weights for APOGEE chemical elements (Garcia+, 2016)J/A+A/588/A81 : Line list & abundances of the binary zet2 Ret (Saffe+, 2016)J/ApJ/819/19 : Equivalent widths of WASP-94A and WASP-94B (Teske+, 2016)J/MNRAS/472/675 : Wide binaries in Tycho-Gaia: search method (Andrews+, 2017)J/AJ/153/257 : Comoving stars in Gaia DR1 (Oh+, 2017)J/A+A/604/L4 : HAT-P-4 & TYC 2569-744-1 abundances & spectra (Saffe+, 2017)J/MNRAS/479/1332 : Binaries with F, G or K primaries & M dwarfs (Montes+, 2018)J/AJ/158/122 : Star formation history of the MW (Kounkel+, 2019)J/A+A/633/A99 : Gaia DR2 open clusters in the MW. II (Cantat-Gaudin+, 2020)J/MNRAS/496/2422 : Abund. of 42 Pisces-Eridanus stream stars (Hawkins+, 2020)J/MNRAS/492/1164 : Abundances of Gaia DR2 wide binaries (Hawkins+, 2020)J/A+A/645/A106 : Atomic data for the Gaia-ESO Survey (Heiter+, 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/921/118https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/921/118http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/921/118https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/921/118https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/921/118http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/921/118GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/921/118/table1 (Target list for the 33 comoving pairs investigated in this study)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/921/118/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/921/118/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/921/118/table1?GETtext/xml+votable180.050000true191.8605-30.89860.0055555555555555566/16565 18464 24663 25675 25698 25860 25921 29152 29562 29658 29914 29987 30096 30983 41055-41056 41082 41204 41266 41415 41759 41905-41906 42253 42468 42662 42884 43338 43473 43773 44117 44157 44228 45340 45621 46170 46313 46654 47206 47215 47366 47416 47676 47896 479111.9867573869263685e-19 3.916500758235022e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/921/118?format=asciiOpticaldefaultJ/ApJ/921/118/table1Target list for the 33 comoving pairs investigated in this studyrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGaiaGaia EDR3 identifiermeta.id;meta.mainRA_ICRS[189.8/356.1] Gaia EDR3 Right Ascension (ICRS) at Ep=2016.0degpos.eq.ra;meta.mainDE_ICRS[-81/-1.6] Gaia EDR3 Declination (ICRS) at Ep=2016.0degpos.eq.dec;meta.mainPlx[4/25.2] Gaia EDR3 parallaxmaspos.parallaxfloate_Plx[0.01/0.2] Uncertainty in Plxmasstat.error;pos.parallaxfloatGmag[2/6] Gaia EDR3 G band magnitudemagphot.mag;em.optfloatSimbadSimbad column added by the CDSmeta.ref.urlchar_RA.icrsRight ascension (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.raindexed_DE.icrsDeclination (ICRS) at Epoch=J2000, proper motions taken into accountdegpos.eq.decindexedBp-Rp[0.5/1.1] Gaia EDR3 (blue-red) passband color indexmagphot.color;em.opt.B;em.opt.RfloatRVel[-67/44.3] Radial velocitykm/sphys.veloc;pos.heliocentricfloate_RVel[0.02/0.3] Uncertainty in RVelkm/sstat.error;spect.dopplerVelocfloatSNR-B[73/235] MIKE blue spectrograph SNRstat.snrfloatSNR-R[92/403] MIKE red spectrograph SNRstat.snrfloate_RA_ICRS[0.007/0.07] Uncertainty in RAdegarcsecstat.error;pos.eq.rafloate_DE_ICRS[0.007/0.1] Uncertainty in DEdegarcsecstat.error;pos.eq.decfloatpmRA[-256/207] Gaia EDR3 proper motion along RAmas/yrpos.pm;pos.eq.radoublee_pmRA[0.009/0.1] Uncertainty in pmRAmas/yrstat.error;pos.pm;pos.eq.rafloatpmDE[-253/25] Gaia EDR3 proper motion along DEmas/yrpos.pm;pos.eq.decdoublee_pmDE[0.009/0.2] Uncertainty in pmDEmas/yrstat.error;pos.pm;pos.eq.decfloatRADEcor[-0.6/0.5] RA and DE correlationstat.correlationRAPlxcor[-0.5/0.4] Right Ascension and parallax correlationstat.correlationRApmRAcor[-0.5/0.4] Right Ascension and RA proper motion correlationstat.correlationRApmDEcor[-0.5/0.4] Right Ascension and DE proper motion correlationstat.correlationDEPlxcor[-0.6/0.2] Declination and parallax correlationstat.correlationDEpmRAcor[-0.6/0.5] Declination and RA proper motion correlationstat.correlationDEpmDEcor[-0.8/0.7] Declination and DE proper motion correlationstat.correlationPlxpmRAcor[-0.5/0.4] Parallax and RA proper motion correlationstat.correlationfloatPlxpmDEcor[-0.4/0.5] Parallax and DE proper motion correlationstat.correlationfloatpmRApmDEcor[-0.6/0.4] RA proper motion and DE proper motion correlationstat.correlationfloatIDShort identifiermeta.idcharprimarym_IDID componentmeta.code.multipcharNlNumber of line measurements for this target (link to Table 3)meta.numberintnullableJ/ApJ/921/118/table2The 3D separations and velocity differences between comoving pairsDelV3D[0.26/3.8] Component's 3D velocity differencekm/sphys.veloc;arith.difffloate_DelV3D[0.02/0.2] Uncertainty in DelV3Dkm/sstat.errorfloatSgeo[277/28200]? Geometric separation (2)AUpos.angDistancedoublenullableb_Sgeo[27.2/2770]? Lower 16 percentile boundary on SgeoAUpos.angDistance;stat.mindoublenullableIDShort identifiermeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCompAGaia EDR3 identifier for component Ameta.idCompBGaia EDR3 identifier for component Bmeta.idSep[1220/18700000] The 3D separation (1)AUpos.angDistancedoublee_Sep[7670/178000] Uncertainty in SepAUstat.errordoubleB_Sgeo[121/12300]? Upper 84 percentile boundary on SgeoAUpos.angDistance;stat.maxdoublenullableJ/ApJ/921/118/table3The line list selectionIDShort identifiermeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintm_IDID componentmeta.code.multipcharIonIdentifierphys.atmol.ionStagecharlambda[4205/8933] Wavelength; Angstroms0.1nmem.wlfloatloggf[-10/0.57] log oscillator strengthphys.atmol.oscStrengthfloatRefReference(s) (see refs.dat file)meta.ref;pos.framecharExPot[0/14.8] Excitation potentialeVphys.atmol.excitationfloatlogA[0.36/8.76] log absolute abundance (1)phys.abundfloatJ/ApJ/921/118/table4Stellar parameters and elemental abundances derived from BACCHUSe_[Al/H]A[0.01/0.03] Uncertainty in [Al/H]Alog(Sun)stat.error;phys.abundfloatdel[Si/H]t[0.01/0.05] Error from differential stellar parameters in [Si/H]log(Sun)stat.errorfloate_[Cr/H]A[0.02/0.11] Uncertainty in [Cr/H]Alog(Sun)stat.error;phys.abundfloat[Zr/H]B[-0.33/0.3] Component B nLBL method [Zr/H]Blog(Sun)phys.abundfloat[C/H]B[-0.3/0.35] Component B nLBL method [C/H]Blog(Sun)stat.fit;phys.abundfloat[C/H]Bl[0.01/0.03] Statistical line-to-line scatter in [C/H]Blog(Sun)stat.errorfloat[C/H]Bt[0.01/0.08] Error from differential stellar parameters in [C/H]Blog(Sun)stat.errorfloate_[C/H]B[0.02/0.08] Uncertainty in [C/H]Blog(Sun)stat.error;phys.abundfloatIDInternal comoving pair identifiermeta.id;meta.mainchardelRVDifferent radial velocity in Gaia EDR3? True|Falsemeta.codecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCompAComponent A Gaia EDR3 identifiermeta.idCompBComponent B Gaia EDR3 identifiermeta.idTeffA[5157/6787] Component A effective temperatureKphys.temperature.effectiveinte_TeffA[0/70] Uncertainty in TeffAKstat.errorintloggA[3.9/4.7] Component A log surface gravitylog(cm.s**-2)phys.gravityfloate_loggA[0.02/0.4] Uncertainty in log(g)Alog(cm.s**-2)stat.errorfloatxiA[0.65/1.73] Component A microturbulencekm/sphys.veloc.microTurbfloate_xiA[0.03/0.08] Uncertainty in xiAkm/sstat.errorfloatTeffB[5052/6701] Component B effective temperatureKphys.temperature.effectiveinte_TeffB[1/65] Uncertainty in TeffBKstat.errorintloggB[3.8/4.8] Component B log surface gravitylog(cm.s**-2)phys.gravityfloate_loggB[0.05/0.5] Uncertainty in log(g)Blog(cm.s**-2)stat.errorfloatxiB[0.42/1.71] Component B microturbulencekm/sphys.veloc.microTurbfloate_xiB[0.03/0.08] Uncertainty in xiBkm/sstat.errorfloatdel[Fe/H][-0.17/0.15] Differential method [Fe/H] (1)log(Sun)phys.abundfloatdel[Fe/H]l[0/0.01] Statistical line-to-line scatter in [Fe/H]log(Sun)stat.error;phys.abund.Fefloatdel[Fe/H]t[0.01/0.12] Error from differential stellar parameters in [Fe/H]log(Sun)stat.errorfloate_del[Fe/H][0.02/0.12] Uncertainty in del[Fe/H] (2)log(Sun)stat.error;phys.abund.Fefloat[Fe/H]A[-0.35/0.38] Component A nLBL method [Fe/H]Alog(Sun)phys.abundfloat[Fe/H]Al[0.01] Statistical line-to-line scatter in [Fe/H]Alog(Sun)stat.error;phys.abund.Fefloat[Fe/H]At[0.01/0.15] Error from differential stellar parameters in [Fe/H]Alog(Sun)stat.errorfloate_[Fe/H]A[0.01/0.15] Uncertainty in [Fe/H]Alog(Sun)stat.error;phys.abund.Fefloat[Fe/H]B[-0.3/0.34] Component B nLBL method [Fe/H]Blog(Sun)phys.abundfloat[Fe/H]Bl[0.01] Statistical line-to-line scatter in [Fe/H]Blog(Sun)stat.error;phys.abund.Fefloat[Fe/H]Bt[0.01/0.04] Error from differential stellar parameters in [Fe/H]Blog(Sun)stat.errorfloate_[Fe/H]B[0.02/0.05] Uncertainty in [Fe/H]Blog(Sun)stat.error;phys.abund.Fefloatdel[Na/H][-0.2/0.2] Differential method [Na/H] (1)log(Sun)phys.abundfloatdel[Na/H]l[0/0.03] Statistical line-to-line scatter in [Na/H]log(Sun)stat.errorfloatdel[Na/H]t[0.02/0.05] Error from differential stellar parameters in [Na/H]log(Sun)stat.errorfloate_del[Na/H][0.02/0.05] Uncertainty in del[Na/H] (2)log(Sun)stat.error;phys.abundfloat[Na/H]A[-0.25/0.57] Component A nLBL method [Na/H]Alog(Sun)phys.abundfloat[Na/H]Al[0.01/0.06] Statistical line-to-line scatter in [Na/H]Alog(Sun)stat.errorfloat[Na/H]At[0.01/0.07] Error from differential stellar parameters in [Na/H]Alog(Sun)stat.errorfloate_[Na/H]A[0.02/0.07] Uncertainty in [Na/H]Alog(Sun)stat.error;phys.abundfloat[Na/H]B[-0.18/0.53] Component B nLBL method [Na/H]Blog(Sun)phys.abundfloat[Na/H]Bl[0.01/0.05] Statistical line-to-line scatter in [Na/H]Blog(Sun)stat.errorfloat[Na/H]Bt[0.01/0.05] Error from differential stellar parameters in [Na/H]Blog(Sun)stat.errorfloate_[Na/H]B[0.02/0.06] Uncertainty in [Na/H]Blog(Sun)stat.error;phys.abundfloatdel[Mg/H][-0.13/0.14] Differential method [Mg/H] (1)log(Sun)phys.abundfloatdel[Mg/H]l[0/0.1] Statistical line-to-line scatter in [Mg/H]log(Sun)stat.errorfloatdel[Mg/H]t[0.01/0.05] Error from differential stellar parameters in [Mg/H]log(Sun)stat.errorfloate_del[Mg/H][0.01/0.1] Uncertainty in del[Mg/H] (2)log(Sun)stat.error;phys.abundfloat[Mg/H]A[-0.17/0.56] Component A nLBL method [Mg/H]Alog(Sun)phys.abundfloat[Mg/H]Al[0.03/0.09] Statistical line-to-line scatter in [Mg/H]Alog(Sun)stat.error;stat.valuefloat[Mg/H]At[0.01/0.07] Error from differential stellar parameters in [Mg/H]Alog(Sun)stat.errorfloate_[Mg/H]A[0.03/0.11] Uncertainty in [Mg/H]Alog(Sun)stat.error;phys.abundfloat[Mg/H]B[-0.15/0.52] Component B nLBL method [Mg/H]Blog(Sun)phys.abundfloat[Mg/H]Bl[0.04/0.09] Statistical line-to-line scatter in [Mg/H]Blog(Sun)stat.error;stat.valuefloat[Mg/H]Bt[0.01/0.05] Error from differential stellar parameters in [Mg/H]Blog(Sun)stat.errorfloate_[Mg/H]B[0.04/0.09] Uncertainty in [Mg/H]Blog(Sun)stat.error;phys.abundfloatdel[Si/H][-0.13/0.15] Differential method [Si/H] (1)log(Sun)phys.abundfloate_del[Si/H][0.01/0.05] Uncertainty in del[Si/H] (2)log(Sun)stat.error;phys.abundfloatdel[Si/H]l[0/0.03] Statistical line-to-line scatter in [Si/H]log(Sun)stat.errorfloatdel[Al/H][-0.15/0.15] Differential method [Al/H] (1)log(Sun)phys.abundfloatdel[Al/H]l[0/0.1] Statistical line-to-line scatter in [Al/H]log(Sun)stat.errorfloatdel[Al/H]t[0.01/0.02] Error from differential stellar parameters in [Al/H]log(Sun)stat.errorfloate_del[Al/H][0.01/0.1] Uncertainty in del[Al/H] (2)log(Sun)stat.error;phys.abundfloat[Al/H]A[-0.16/0.5] Component A nLBL method [Al/H]Alog(Sun)phys.abundfloat[Al/H]Al[0/0.03] Statistical line-to-line scatter in [Al/H]Alog(Sun)stat.errorfloat[Al/H]At[0/0.03] Error from differential stellar parameters in [Al/H]Alog(Sun)stat.errorfloat[Al/H]B[-0.13/0.45] Component B nLBL method [Al/H]Blog(Sun)phys.abundfloat[Al/H]Bl[0/0.1] Statistical line-to-line scatter in [Al/H]Blog(Sun)stat.errorfloat[Al/H]Bt[0/0.03] Error from differential stellar parameters in [Al/H]Blog(Sun)stat.errorfloate_[Al/H]B[0.01/0.1] Uncertainty in [Al/H]Blog(Sun)stat.error;phys.abundfloat[Si/H]A[-0.28/0.43] Component A nLBL method [Si/H]Alog(Sun)phys.abundfloat[Si/H]Al[0.02/0.03] Statistical line-to-line scatter in [Si/H]Alog(Sun)stat.error;stat.valuefloat[Si/H]At[0.01/0.06] Error from differential stellar parameters in [Si/H]Alog(Sun)stat.errorfloate_[Si/H]A[0.02/0.06] Uncertainty in [Si/H]Alog(Sun)stat.error;phys.abundfloat[Si/H]B[-0.23/0.43] Component B nLBL method [Si/H]Blog(Sun)phys.abundfloat[Si/H]Bl[0.02/0.03] Statistical line-to-line scatter in [Si/H]Blog(Sun)stat.error;stat.valuefloat[Si/H]Bt[0.01/0.08] Error from differential stellar parameters in [Si/H]Blog(Sun)stat.errorfloate_[Si/H]B[0.02/0.09] Uncertainty in [Si/H]Blog(Sun)stat.error;phys.abundfloatdel[Ca/H][-0.17/0.13] Differential method [Ca/H] (1)log(Sun)phys.abundfloatdel[Ca/H]l[0/0.03] Statistical line-to-line scatter in [Ca/H]log(Sun)stat.errorfloatdel[Ca/H]t[0.02/0.15] Error from differential stellar parameters in [Ca/H]log(Sun)stat.errorfloate_del[Ca/H][0.03/0.15] Uncertainty in del[Ca/H] (2)log(Sun)stat.error;phys.abundfloat[Ca/H]A[-0.23/0.4] Component A nLBL method [Ca/H]Alog(Sun)phys.abundfloat[Ca/H]Al[0.01/0.03] Statistical line-to-line scatter in [Ca/H]Alog(Sun)stat.errorfloat[Ca/H]At[0.02/0.16] Error from differential stellar parameters in [Ca/H]Alog(Sun)stat.errorfloate_[Ca/H]A[0.03/0.16] Uncertainty in [Ca/H]Alog(Sun)stat.error;phys.abundfloat[Ca/H]B[-0.21/0.34] Component B nLBL method [Ca/H]Blog(Sun)phys.abundfloat[Ca/H]Bl[0.01/0.03] Statistical line-to-line scatter in [Ca/H]Blog(Sun)stat.errorfloat[Ca/H]Bt[0.03/0.09] Error from differential stellar parameters in [Ca/H]Blog(Sun)stat.errorfloate_[Ca/H]B[0.04/0.09] Uncertainty in [Ca/H]Blog(Sun)stat.error;phys.abundfloatdel[Sc/H][-0.21/0.19] Differential method [Sc/H] (1)log(Sun)phys.abundfloatdel[Sc/H]l[0/0.06] Statistical line-to-line scatter in [Sc/H]log(Sun)stat.errorfloatdel[Sc/H]t[0.04/0.1] Error from differential stellar parameters in [Sc/H]log(Sun)stat.errorfloate_del[Sc/H][0.05/0.11] Uncertainty in del[Sc/H] (2)log(Sun)stat.error;phys.abundfloat[Sc/H]A[-0.15/0.57] Component A nLBL method [Sc/H]Alog(Sun)phys.abundfloat[Sc/H]Al[0.02/0.04] Statistical line-to-line scatter in [Sc/H]Alog(Sun)stat.error;stat.valuefloat[Sc/H]At[0.01/0.14] Error from differential stellar parameters in [Sc/H]Alog(Sun)stat.errorfloate_[Sc/H]A[0.03/0.14] Uncertainty in [Sc/H]Alog(Sun)stat.error;phys.abundfloat[Sc/H]B[-0.09/0.51] Component B nLBL method [Sc/H]Blog(Sun)phys.abundfloat[Sc/H]Bl[0.02/0.05] Statistical line-to-line scatter in [Sc/H]Blog(Sun)stat.error;stat.valuefloat[Sc/H]Bt[0.01/0.11] Error from differential stellar parameters in [Sc/H]Blog(Sun)stat.errorfloate_[Sc/H]B[0.03/0.12] Uncertainty in [Sc/H]Blog(Sun)stat.error;phys.abundfloatdel[Ti/H][-0.14/0.18] Differential method [Ti/H] (1)log(Sun)phys.abundfloatdel[Ti/H]l[0/0.02] Statistical line-to-line scatter in [Ti/H]log(Sun)stat.errorfloatdel[Ti/H]t[0.02/0.06] Error from differential stellar parameters in [Ti/H]log(Sun)stat.errorfloate_del[Ti/H][0.03/0.06] Uncertainty in del[Ti/H] (2)log(Sun)stat.error;phys.abundfloat[Ti/H]A[-0.31/0.39] Component A nLBL method [Ti/H]Alog(Sun)phys.abundfloat[Ti/H]Al[0.01/0.03] Statistical line-to-line scatter in [Ti/H]Alog(Sun)stat.error;stat.valuefloat[Ti/H]At[0.01/0.09] Error from differential stellar parameters in [Ti/H]Alog(Sun)stat.errorfloate_[Ti/H]A[0.02/0.09] Uncertainty in [Ti/H]Alog(Sun)stat.error;phys.abundfloat[Ti/H]B[-0.22/0.31] Component Bdifferential method [Ti/H]log(Sun)phys.abundfloat[Ti/H]Bl[0.01/0.03] Statistical line-to-line scatter in [Ti/H]Blog(Sun)stat.error;stat.valuefloat[Ti/H]Bt[0.02/0.07] Error from differential stellar parameters in [Ti/H]Blog(Sun)stat.errorfloate_[Ti/H]B[0.02/0.08] Uncertainty in [Ti/H]Blog(Sun)stat.error;phys.abundfloatdel[V/H][-0.17/0.22] Differential method [V/H] (1)log(Sun)phys.abundfloatdel[V/H]l[0/0.06] Statistical line-to-line scatter in [V/H]log(Sun)stat.errorfloatdel[V/H]t[0.02/0.04] Error from differential stellar parameters in [V/H]log(Sun)stat.errorfloate_del[V/H][0.03/0.06] Uncertainty in del[V/H] (2)log(Sun)stat.error;phys.abundfloat[V/H]A[-0.47/0.36] Component A nLBL method [V/H]Alog(Sun)phys.abundfloat[V/H]Al[0.02/0.06] Statistical line-to-line scatter in [V/H]Alog(Sun)stat.error;stat.valuefloat[V/H]At[0.01/0.23] Error from differential stellar parameters in [V/H]Alog(Sun)stat.errorfloate_[V/H]A[0.02/0.24] Uncertainty in [V/H]Alog(Sun)stat.error;phys.abundfloat[V/H]B[-0.4/0.27] Component B nLBL method [V/H]Blog(Sun)phys.abundfloat[V/H]Bl[0.01/0.05] Statistical line-to-line scatter in [V/H]Blog(Sun)stat.error;stat.valuefloat[V/H]Bt[0.01/0.15] Error from differential stellar parameters in [V/H]Blog(Sun)stat.errorfloate_[V/H]B[0.02/0.16] Uncertainty in [V/H]Blog(Sun)stat.error;phys.abundfloatdel[Cr/H][-0.14/0.14] Differential method [Cr/H] (1)log(Sun)phys.abundfloatdel[Cr/H]l[0.01/0.05] Statistical line-to-line scatter in [Cr/H]log(Sun)stat.errorfloatdel[Cr/H]t[0.02/0.04] Error from differential stellar parameters in [Cr/H]log(Sun)stat.errorfloate_del[Cr/H][0.03/0.06] Uncertainty in del[Cr/H] (2)log(Sun)stat.error;phys.abundfloat[Cr/H]A[-0.39/0.29] Component A nLBL method [Cr/H]Alog(Sun)phys.abundfloat[Cr/H]Al[0.01/0.05] Statistical line-to-line scatter in [Cr/H]Alog(Sun)stat.errorfloat[Cr/H]At[0.01/0.11] Error from differential stellar parameters in [Cr/H]Alog(Sun)stat.errorfloat[Cr/H]B[-0.37/0.25] Component B nLBL method [Cr/H]Blog(Sun)phys.abundfloat[Cr/H]Bl[0.01/0.05] Statistical line-to-line scatter in [Cr/H]Blog(Sun)stat.errorfloat[Cr/H]Bt[0.01/0.06] Error from differential stellar parameters in [Cr/H]Blog(Sun)stat.errorfloate_[Cr/H]B[0.02/0.08] Uncertainty in [Cr/H]Blog(Sun)stat.error;phys.abundfloatdel[Mn/H][-0.24/0.22] Differential method [Mn/H] (1)log(Sun)phys.abundfloatdel[Mn/H]l[0/0.05] Statistical line-to-line scatter in [Mn/H]log(Sun)stat.errorfloatdel[Mn/H]t[0.03/0.04] Error from differential stellar parameters in [Mn/H]log(Sun)stat.errorfloate_del[Mn/H][0.03/0.06] Uncertainty in del[Mn/H] (2)log(Sun)stat.error;phys.abundfloat[Mn/H]A[-0.51/0.37] Component A nLBL method [Mn/H]Alog(Sun)phys.abundfloat[Mn/H]Al[0.01/0.03] Statistical line-to-line scatter in [Mn/H]Alog(Sun)stat.error;stat.valuefloat[Mn/H]At[0.01/0.08] Error from differential stellar parameters in [Mn/H]Alog(Sun)stat.errorfloate_[Mn/H]A[0.02/0.08] Uncertainty in [Mn/H]Alog(Sun)stat.error;phys.abundfloat[Mn/H]B[-0.46/0.27] Component B nLBL method [Mn/H]Blog(Sun)phys.abundfloat[Mn/H]Bl[0.01/0.04] Statistical line-to-line scatter in [Mn/H]Blog(Sun)stat.error;stat.valuefloat[Mn/H]Bt[0.01/0.06] Error from differential stellar parameters in [Mn/H]Blog(Sun)stat.errorfloate_[Mn/H]B[0.03/0.07] Uncertainty in [Mn/H]Blog(Sun)stat.error;phys.abundfloatdel[Co/H][-0.29/0.22] Differential method [Co/H] (1)log(Sun)phys.abundfloatdel[Co/H]l[0.01/0.17] Statistical line-to-line scatter in [Co/H]log(Sun)stat.errorfloatdel[Co/H]t[0.02/0.03] Error from differential stellar parameters in [Co/H]log(Sun)stat.errorfloate_del[Co/H][0.03/0.17] Uncertainty in del[Co/H] (2)log(Sun)stat.error;phys.abundfloat[Co/H]A[-0.33/0.31] Component A nLBL method [Co/H]Alog(Sun)phys.abundfloat[Co/H]Al[0.02/0.11] Statistical line-to-line scatter in [Co/H]Alog(Sun)stat.errorfloat[Co/H]At[0.01/0.15] Error from differential stellar parameters in [Co/H]Alog(Sun)stat.errorfloate_[Co/H]A[0.02/0.18] Uncertainty in [Co/H]Alog(Sun)stat.error;phys.abundfloat[Co/H]B[-0.26/0.34] Component B nLBL method [Co/H]Blog(Sun)phys.abundfloat[Co/H]Bl[0.02/0.08] Statistical line-to-line scatter in [Co/H]Blog(Sun)stat.errorfloat[Co/H]Bt[0.01/0.13] Error from differential stellar parameters in [Co/H]Blog(Sun)stat.errorfloate_[Co/H]B[0.03/0.13] Uncertainty in [Co/H]Blog(Sun)stat.error;phys.abundfloatdel[Ni/H][-0.19/0.21] Differential method [Ni/H] (1)log(Sun)phys.abundfloatdel[Ni/H]l[0/0.02] Statistical line-to-line scatter in [Ni/H]log(Sun)stat.errorfloatdel[Ni/H]t[0.02/0.11] Error from differential stellar parameters in [Ni/H]log(Sun)stat.errorfloate_del[Ni/H][0.02/0.11] Uncertainty in del[Ni/H] (2)log(Sun)stat.error;phys.abundfloat[Ni/H]A[-0.43/0.38] Component A nLBL method [Ni/H]Alog(Sun)phys.abundfloat[Ni/H]Al[0.02/0.03] Statistical line-to-line scatter in [Ni/H]Alog(Sun)stat.errorfloat[Ni/H]At[0.01/0.15] Error from differential stellar parameters in [Ni/H]Alog(Sun)stat.errorfloate_[Ni/H]A[0.03/0.15] Uncertainty in [Ni/H]Alog(Sun)stat.error;phys.abundfloat[Ni/H]B[-0.33/0.36] Component B nLBL method [Ni/H]Blog(Sun)phys.abundfloat[Ni/H]Bl[0.02/0.03] Statistical line-to-line scatter in [Ni/H]Blog(Sun)stat.errorfloat[Ni/H]Bt[0.01/0.05] Error from differential stellar parameters in [Ni/H]Blog(Sun)stat.errorfloate_[Ni/H]B[0.03/0.06] Uncertainty in [Ni/H]Blog(Sun)stat.error;phys.abundfloatdel[Cu/H][-0.18/0.21] Differential method [Cu/H] (1)log(Sun)phys.abundfloatdel[Cu/H]l[0/0.04] Statistical line-to-line scatter in [Cu/H]log(Sun)stat.errorfloatdel[Cu/H]t[0.02/0.06] Error from differential stellar parameters in [Cu/H]log(Sun)stat.errorfloate_del[Cu/H][0.03/0.06] Uncertainty in del[Cu/H] (2)log(Sun)stat.error;phys.abundfloat[Cu/H]A[-0.51/0.28] Component A nLBL method [Cu/H]Alog(Sun)phys.abundfloat[Cu/H]Al[0.01/0.07] Statistical line-to-line scatter in [Cu/H]Alog(Sun)stat.errorfloat[Cu/H]At[0.01/0.1] Error from differential stellar parameters in [Cu/H]Alog(Sun)stat.errorfloate_[Cu/H]A[0.03/0.11] Uncertainty in [Cu/H]Alog(Sun)stat.error;phys.abundfloat[Cu/H]B[-0.44/0.3] Component B nLBL method [Cu/H]Blog(Sun)phys.abundfloat[Cu/H]Bl[0.01/0.05] Statistical line-to-line scatter in [Cu/H]Blog(Sun)stat.errorfloat[Cu/H]Bt[0.01/0.07] Error from differential stellar parameters in [Cu/H]Blog(Sun)stat.errorfloate_[Cu/H]B[0.03/0.08] Uncertainty in [Cu/H]Blog(Sun)stat.error;phys.abundfloatdel[Zn/H][-0.21/0.14] Differential method [Zn/H] (1)log(Sun)phys.abundfloatdel[Zn/H]l[0/0.04] Statistical line-to-line scatter in [Zn/H]log(Sun)stat.errorfloatdel[Zn/H]t[0.02/0.17] Error from differential stellar parameters in [Zn/H]log(Sun)stat.errorfloate_del[Zn/H][0.02/0.17] Uncertainty in del[Zn/H] (2)log(Sun)stat.error;phys.abundfloat[Zn/H]A[-0.5/0.21] Component A nLBL method [Zn/H]Alog(Sun)phys.abundfloat[Zn/H]Al[0/0.06] Statistical line-to-line scatter in [Zn/H]Alog(Sun)stat.error;stat.valuefloat[Zn/H]At[0.01/0.19] Error from differential stellar parameters in [Zn/H]Alog(Sun)stat.errorfloate_[Zn/H]A[0.02/0.19] Uncertainty in [Zn/H]Alog(Sun)stat.error;phys.abundfloat[Zn/H]B[-0.44/0.26] Component B nLBL method [Zn/H]Blog(Sun)phys.abundfloat[Zn/H]Bl[0/0.1] Statistical line-to-line scatter in [Zn/H]Blog(Sun)stat.error;stat.valuefloat[Zn/H]Bt[0.01/0.05] Error from differential stellar parameters in [Zn/H]Blog(Sun)stat.errorfloate_[Zn/H]B[0.02/0.1] Uncertainty in [Zn/H]Blog(Sun)stat.error;phys.abundfloatdel[Sr/H][-0.34/0.13]? Differential method [Sr/H] (1)log(Sun)phys.abundfloatnullabledel[Sr/H]l[0.1/0.1]? Statistical line-to-line scatter in [Sr/H]log(Sun)stat.errorfloatnullabledel[Sr/H]t[0.02/0.43] Error from differential stellar parameters in [Sr/H]log(Sun)stat.errorfloate_del[Sr/H][0.1/0.44]? Uncertainty in del[Sr/H] (2)log(Sun)stat.error;phys.abundfloatnullable[Sr/H]A[-0.57/0.53] Component A nLBL method [Sr/H]Alog(Sun)phys.abundfloat[Sr/H]Al[0.02/0.17] Statistical line-to-line scatter in [Sr/H]Alog(Sun)stat.error;stat.valuefloat[Sr/H]At[0.01/0.34] Error from differential stellar parameters in [Sr/H]Alog(Sun)stat.errorfloate_[Sr/H]A[0.06/0.38] Uncertainty in [Sr/H]Alog(Sun)stat.error;phys.abundfloat[Sr/H]B[-0.61/0.21]? Component B nLBL method [Sr/H]Blog(Sun)phys.abundfloatnullable[Sr/H]Bl[0/0.17]? Statistical line-to-line scatter in [Sr/H]Blog(Sun)stat.error;stat.valuefloatnullable[Sr/H]Bt[0.02/0.24] Error from differential stellar parameters in [Sr/H]Blog(Sun)stat.errorfloate_[Sr/H]B[0.04/0.29]? Uncertainty in [Sr/H]Blog(Sun)stat.error;phys.abundfloatnullabledel[Y/H][-0.25/0.16] Differential method [Y/H] (1)log(Sun)phys.abundfloatdel[Y/H]l[0/0.06] Statistical line-to-line scatter in [Y/H]log(Sun)stat.errorfloatdel[Y/H]t[0.05/0.08] Error from differential stellar parameters in [Y/H]log(Sun)stat.errorfloate_del[Y/H][0.05/0.1] Uncertainty in del[Y/H] (2)log(Sun)stat.error;phys.abundfloat[Y/H]A[-0.63/0.23] Component A nLBL method [Y/H]Alog(Sun)stat.fitfloat[Y/H]Al[0/0.07] Statistical line-to-line scatter in [Y/H]Alog(Sun)stat.error;stat.valuefloat[Y/H]At[0.02/0.2] Error from differential stellar parameters in [Y/H]Alog(Sun)stat.errorfloate_[Y/H]A[0.04/0.21] Uncertainty in [Y/H]Alog(Sun)stat.error;phys.abundfloat[Y/H]B[-0.6/0.12] Component B nLBL method [Y/H]Blog(Sun)stat.fitfloat[Y/H]Bl[0.01/0.07] Statistical line-to-line scatter in [Y/H]Blog(Sun)stat.error;stat.valuefloat[Y/H]Bt[0.02/0.12] Error from differential stellar parameters in [Y/H]Blog(Sun)stat.errorfloate_[Y/H]B[0.04/0.13] Uncertainty in [Y/H]Blog(Sun)stat.error;phys.abundfloatdel[Zr/H][-0.25/0.22] Differential method [Zr/H] (1)log(Sun)phys.abundfloatdel[Zr/H]l[0/0.06] Statistical line-to-line scatter in [Zr/H]log(Sun)stat.errorfloatdel[Zr/H]t[0.02/0.08] Error from differential stellar parameters in [Zr/H]log(Sun)stat.errorfloate_del[Zr/H][0.03/0.09] Uncertainty in del[Zr/H] (2)log(Sun)stat.error;phys.abundfloat[Zr/H]A[-0.48/0.42] Component A nLBL method [Zr/H]Alog(Sun)phys.abundfloat[Zr/H]Al[0/0.07] Statistical line-to-line scatter in [Zr/H]Alog(Sun)stat.error;stat.valuefloat[Zr/H]At[0.04/0.18] Error from differential stellar parameters in [Zr/H]Alog(Sun)stat.errorfloate_[Zr/H]A[0.04/0.18] Uncertainty in [Zr/H]Alog(Sun)stat.error;phys.abundfloat[Zr/H]Bl[0.01/0.09] Statistical line-to-line scatter in [Zr/H]Blog(Sun)stat.error;stat.valuefloat[Zr/H]Bt[0.03/0.15] Error from differential stellar parameters in [Zr/H]Blog(Sun)stat.errorfloate_[Zr/H]B[0.04/0.16] Uncertainty in [Zr/H]Blog(Sun)stat.error;phys.abundfloatdel[Ba/H][-0.23/0.08] Differential method [Ba/H] (1)log(Sun)phys.abundfloatdel[Ba/H]l[0/0.1] Statistical line-to-line scatter in [Ba/H]log(Sun)stat.errorfloatdel[Ba/H]t[0.02/0.36] Error from differential stellar parameters in [Ba/H]log(Sun)stat.errorfloate_del[Ba/H][0.02/0.37] Uncertainty in del[Ba/H] (2)log(Sun)stat.error;phys.abundfloat[Ba/H]A[-0.21/0.61] Component A nLBL method [Ba/H]Alog(Sun)phys.abundfloat[Ba/H]Al[0.02/0.11] Statistical line-to-line scatter in [Ba/H]Alog(Sun)stat.errorfloat[Ba/H]At[0.01/0.37] Error from differential stellar parameters in [Ba/H]Alog(Sun)stat.errorfloate_[Ba/H]A[0.03/0.38] Uncertainty in [Ba/H]Alog(Sun)stat.error;phys.abundfloat[Ba/H]B[-0.22/0.56] Component B nLBL method [Ba/H]Blog(Sun)phys.abundfloat[Ba/H]Bl[0.02/0.11] Statistical line-to-line scatter in [Ba/H]Blog(Sun)stat.errorfloat[Ba/H]Bt[0.02/0.07] Error from differential stellar parameters in [Ba/H]Blog(Sun)stat.errorfloate_[Ba/H]B[0.03/0.11] Uncertainty in [Ba/H]Blog(Sun)stat.error;phys.abundfloatdel[La/H][-0.42/0.19]? Differential method [La/H] (1)log(Sun)phys.abundfloatnullabledel[La/H]l[0/0.19]? Statistical line-to-line scatter in [La/H]log(Sun)stat.errorfloatnullabledel[La/H]t[0.04/0.12] Error from differential stellar parameters in [La/H]log(Sun)stat.errorfloate_del[La/H][0.04/0.2]? Uncertainty in del[La/H] (2)log(Sun)stat.error;phys.abundfloatnullable[La/H]A[-0.19/0.48] Component A nLBL method [La/H]Alog(Sun)phys.abundfloat[La/H]Al[0/0.14] Statistical line-to-line scatter in [La/H]Alog(Sun)stat.errorfloat[La/H]At[0.01/0.22] Error from differential stellar parameters in [La/H]Alog(Sun)stat.errorfloate_[La/H]A[0.03/0.26] Uncertainty in [La/H]Alog(Sun)stat.error;phys.abundfloat[La/H]B[-0.08/0.4]? Component B nLBL method [La/H]Blog(Sun)phys.abundfloatnullable[La/H]Bl[0/0.11]? Statistical line-to-line scatter in [La/H]Blog(Sun)stat.errorfloatnullable[La/H]Bt[0.02/0.28] Error from differential stellar parameters in [La/H]Blog(Sun)stat.errorfloate_[La/H]B[0.04/0.3]? Uncertainty in [La/H]Blog(Sun)stat.error;phys.abundfloatnullabledel[Nd/H][-0.21/0.22] Differential method [Nd/H] (1)log(Sun)phys.abundfloatdel[Nd/H]l[0/0.18] Statistical line-to-line scatter in [Nd/H]log(Sun)stat.errorfloatdel[Nd/H]t[0.04/0.09] Error from differential stellar parameters in [Nd/H]log(Sun)stat.errorfloate_del[Nd/H][0.05/0.18] Uncertainty in del[Nd/H] (2)log(Sun)stat.error;phys.abundfloat[Nd/H]A[-0.37/0.3] Component A nLBL method [Nd/H]Alog(Sun)phys.abundfloat[Nd/H]Al[0/0.13] Statistical line-to-line scatter in [Nd/H]Alog(Sun)stat.errorfloat[Nd/H]At[0.05/0.23] Error from differential stellar parameters in [Nd/H]Alog(Sun)stat.errorfloate_[Nd/H]A[0.06/0.24] Uncertainty in [Nd/H]Alog(Sun)stat.error;phys.abundfloat[Nd/H]B[-0.22/0.31] Component B nLBL method [Nd/H]Blog(Sun)phys.abundfloat[Nd/H]Bl[0.01/0.13] Statistical line-to-line scatter in [Nd/H]Blog(Sun)stat.errorfloat[Nd/H]Bt[0.03/0.19] Error from differential stellar parameters in [Nd/H]Blog(Sun)stat.errorfloate_[Nd/H]B[0.04/0.21] Uncertainty in [Nd/H]Blog(Sun)stat.error;phys.abundfloatdel[Eu/H][-0.26/0.25]? Differential method [Eu/H] (1)log(Sun)phys.abundfloatnullabledel[Eu/H]l[0/0.12]? Statistical line-to-line scatter in [Eu/H]log(Sun)stat.errorfloatnullabledel[Eu/H]t[0.04/0.15] Error from differential stellar parameters in [Eu/H]log(Sun)stat.errorfloate_del[Eu/H][0.06/0.18]? Uncertainty in del[Eu/H] (2)log(Sun)stat.error;phys.abundfloatnullable[Eu/H]A[-0.11/0.48]? Component A nLBL method [Eu/H]Alog(Sun)phys.abundfloatnullable[Eu/H]Al[0/0.14]? Statistical line-to-line scatter in [Eu/H]Alog(Sun)stat.error;stat.valuefloatnullable[Eu/H]At[0.03/0.21] Error from differential stellar parameters in [Eu/H]Alog(Sun)stat.errorfloate_[Eu/H]A[0.06/0.23]? Uncertainty in [Eu/H]Alog(Sun)stat.error;phys.abundfloatnullable[Eu/H]B[-0.03/0.48]? Component B nLBL method [Eu/H]Blog(Sun)phys.abundfloatnullable[Eu/H]Bl[0.03/0.18]? Statistical line-to-line scatter in [Eu/H]Blog(Sun)stat.error;stat.valuefloatnullable[Eu/H]Bt[0.03/0.33] Error from differential stellar parameters in [Eu/H]Blog(Sun)stat.errorfloate_[Eu/H]B[0.1/0.34]? Uncertainty in [Eu/H]Blog(Sun)stat.error;phys.abundfloatnullabledel[Li/H][-1.01/0.74]? Differential method [Li/H] (1)log(Sun)phys.abundfloatnullabledel[Li/H]l[0.1/0.1]? Statistical line-to-line scatter in [Li/H]log(Sun)stat.errorfloatnullabledel[Li/H]t[0.02/0.05] Error from differential stellar parameters in [Li/H]log(Sun)stat.errorfloate_del[Li/H][0.1/0.1]? Uncertainty in del[Li/H] (2)log(Sun)stat.error;phys.abundfloatnullable[Li/H]A[0.63/1.46]? Component A nLBL method [Li/H]Alog(Sun)phys.abundfloatnullable[Li/H]Al[0.1/0.1]? Statistical line-to-line scatter in [Li/H]Alog(Sun)stat.errorfloatnullable[Li/H]At[0/0.05] Error from differential stellar parameters in [Li/H]Alog(Sun)stat.errorfloate_[Li/H]A[0.1/0.11]? Uncertainty in [Li/H]Alog(Sun)stat.error;phys.abundfloatnullable[Li/H]B[0.04/1.92]? Component B nLBL method [Li/H]Blog(Sun)phys.abundfloatnullable[Li/H]Bl[0.1/0.1]? Statistical line-to-line scatter in [Li/H]Blog(Sun)stat.errorfloatnullable[Li/H]Bt[0.01/0.04] Error from differential stellar parameters in [Li/H]Blog(Sun)stat.errorfloate_[Li/H]B[0.1/0.11]? Uncertainty in [Li/H]Blog(Sun)stat.error;phys.abundfloatnullabledel[C/H][-0.18/0.14] Differential method [C/H] (1)log(Sun)phys.abundfloatdel[C/H]l[0/0.03] Statistical line-to-line scatter in [C/H]log(Sun)stat.errorfloatdel[C/H]t[0.01/0.04] Error from differential stellar parameters in [C/H]log(Sun)stat.errorfloate_del[C/H][0.01/0.05] Uncertainty in del[C/H] (2)log(Sun)stat.error;phys.abundfloat[C/H]A[-0.34/0.48] Component A nLBL method [C/H]Alog(Sun)stat.fit;phys.abundfloat[C/H]Al[0.01/0.03] Statistical line-to-line scatter in [C/H]Alog(Sun)stat.errorfloat[C/H]At[0.01/0.11] Error from differential stellar parameters in [C/H]Alog(Sun)stat.errorfloate_[C/H]A[0.02/0.11] Uncertainty in [C/H]Alog(Sun)stat.error;phys.abundfloatJ/ApJ/921/118/refsReferences (from Table 7)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefReference codemeta.notecharBibCodeBibcode of the reference if anymeta.bib.bibcodecharAuthAuthormeta.bib.authorcharCommCommentmeta.notechar