J/AJ/155/111ivo://CDS.VizieR/J/AJ/155/111doi:10.26093/cds/vizier.51550111CDSLuck R.E.2019-01-07T09:42:26Z2018-11-09T09:01:59ZCDS support team

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

cds-question@unistra.frdwarf-starsf-starseffective-temperaturestellar-massesstellar-ageschemical-abundancesradial-velocitystellar-distanceStellar parameters and abundances have been derived from a sample of 907 F, G, and K dwarfs. The high-resolution, high signal-to-noise spectra utilized were acquired with the HARPS spectrograph of the European Southern Observatory. The stars in the sample with -0.2<[Fe/H]<+0.2 have abundances that strongly resemble that of the Sun, except for the lithium content and the lanthanides. Near the solar temperature, stars show two orders of magnitude range in lithium content. The average content of stars in the local region appears to be enhanced at about the +0.1 level relative to the Sun for the lanthanides. There are over 100 planet hosts in this sample, and there is no discernible difference between them and the non-hosts regarding their lithium content.2018AJ....155..111Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/155/111CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/239 : The Hipparcos and Tycho Catalogues (ESA 1997)I/274 : CCDM (Catalog of Components of Double Multiple stars) (Dommanget+ 2002)J/AJ/77/486 : Dwarf K and M stars in Southern hemisphere (Upgren+, 1972)J/A+AS/106/275 : Theoretical isochrones (Bertelli+ 1994)J/MNRAS/349/757 : Masses, ages and metallicities of F-G dwarfs (Lambert+, 2004)J/MNRAS/372/163 : Activity indices for southern stars (Jenkins+, 2006)J/A+A/533/A141 : Stellar parameters for 582 HARPS FGK stars (Sousa+, 2011)J/A+A/545/A32 : Chemical abundances of 1111 FGK stars (Adibekyan+, 2012)J/ApJ/764/78 : Oxygen abundances in nearby FGK stars (Ramirez+, 2013)J/A+A/562/A71 : Chemical abundances of solar neighbourhood dwarfsJ/A+A/576/A89 : O abundances from HARPS in F-G stars (Bertran de Lis+, 2015)J/AJ/150/88 : Abundances in the local region. I. G and K giantsJ/ApJ/833/225 : -2.6<=[Fe/H]<=0.2 F and G dwarfs. II. AbundancesJ/A+A/599/A96 : [C/H] Chemical abundances of 1110 starsJ/AJ/153/21 : Abundances in the local region. II. F, G, and K dwarfshttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/155/111https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/155/111http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/155/111https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/155/111https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/155/111http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/155/111GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/155/111/table1 (Program stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/155/111/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/155/111/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/155/111/table1?GETtext/xml+votable180.050000true83.5381775-15.28421810.0055555555555555565/5886 6/49 60 75 108 137 185 222 251 278 322 323 325 326 333 334 336 337 340 341 342 348 349 354 357 359 373 375 401 411 456 483 524 548 770 1024 1032 1043 1058 1060 1063 2051 4128 4206 4313 4376 4388 4438 4665 5009 8244 8286 8296 8614 8792 9125 12312 12340 12352 12435 12498 12512 12592 12644 12890 12983 13440 16393 16408 16502 16518 16543 16603 16639 16652 16890 16930 16931 16986 16995 17047 17171 17177 17206 17218 17219 17249 17266 17274 17288 17301 17314 17341 17358 17374 17419 17425 17435 17453 17507 17540 17541 17552 17572 17587 17588 17607 17619 17641 17714 17744 17752 17768 17804 17881 17887 17904 17929 17944 17970 17993 18005 18139 18157 18195 18203 18366 18373 18548 18614 18615 18637 18641 18711 18792 18835 19003 19072 19108 19217 19345 19466 19491 19585 19768 19808 19974 20145 20492 20495 20557 20582 20593 20621 20633 20640 20739 20746 20766 20873 21060 21066 21080 21114 21117 21118 21121 21177 21270 21326 21386 21400 21477 21484 21516 21550 21604 21691 21774 21779 21809 21906 21953 21989 22118 22120 22146 22159 22252 22579 22590 22608 22613 22619 22708 22746 22760 22813 22818 22823 22931 23017 23033 23061 23066 23096 23123 23140 23177 23187 23201 23335 23342 23344 23369 23387 23388 23410 23429 23454 23463 23479 23481 23489 23490 23495 23497 23501 23503 23511 23515 23518 23525 23534 23535 23537 23538 23539 23543 23548 23550 23561 23575 23583 23661 23774 23780 23873 23960 24068 24104 24110 24192 24195 24198 24209 24212 24252 24315 24597 24729 24769 24816 24831 24876 24924 25015 25078 25102 25136 25168 25225 25276 25401 25424 25473 25484 25538 25567 25584 25622 25636 25793 25820 25854 25880 25889 25906 25966 26082 26133 26142 26160 26183 26289 26305 26465 26496 26610 26617 26652 26676 26679 26768 26812 26828 26888 26906 26924 26975 26997 27006 27083 27254 27255 27374 27395 27661 27741 28400 28719 28763 28874 28894 28919 28961 28987 29043 29146 29196 29225 29239 29255 29289 29349 29422 29483 29521 29541 29675 29688 29721 29774 29833 29838 29842 29900 29928 30015 30343 30484 30512 30526 30536 30576 30789 30825 30848 30878 30894 30929 30939 30943 30951 30965 31011 31029 31101 31104 31130 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38064 38099 38151 38216 38219 38229 38238 38279 38283 38311 38324 38339 38414 38433 38434 38443 38461 38545 38562 38566 38605 38728 38738 38742 38765 38788 38807 38857 38870 38932 38950 38955 38975 38998 39030 39034 39044 39074 39213 39219 39257 39282 39283 39321 39364 39377 39422 39425 39461 39463 39500 39557 39570 39576 39584 39623 39676 39693 39709 39735 39767 39801 39888 39915 39954 39984 40007 40066 40078 40101 40105 40140 40143 40183 40242 40317 40442 40453 40514 40567 40661 40679 40686 40687 40692 40717 40722 40741 40749 40784 40853 40892 40931 40932 40970 41058 41094 41127 41143 41167 41204 41255 41260 41272 41441 41443 41450 41460 41463 41521 41553 41590 41591 41607 41611 41612 41687 41723 41724 41752 41763 41798 41861 41912 41935 41941 41954 41969 42022 42044 42091 42146 42147 42157 42171 42197 42212 42221 42228 42248 42253 42285 42326 42331 42360 42386 42448 42457 42460 42555 42595 42656 42700 42759 42787 42794 42814 42845 42860 42887 42892 42918 42934 43001 43012 43067 43068 43105 43228 43258 43280 43290 43310 43315 43327 43332 43345 43374 43387 43544 43555 43556 43567 43575 43610 43612 43649 43668 43688 43771 43813 43818 43845 43851 43928 43929 43977 43989 44005 44115 44131 44136 44150 44151 44223 44243 44262 44284 44557 44638 44652 44740 44792 44816 44833 44879 44887 44910 45034 45121 45168 45182 45228 45265 45334 45378 45386 45412 45422 45446 45485 45502 45511 45538 45564 45589 45621 45627 45641 45646 45656 45668 45669 45717 45721 45752 45823 45853 45892 45902 45982 46009 46053 46056 46076 46080 46084 46100 46113 46118 46135 46172 46193 46200 46234 46247 46306 46333 46383 46394 46487 46544 46548 46559 46603 46640 46664 46681 46685 46734 46768 46800 46820 46829 46874 46923 46925 46933 46944 46967 46982 46997 47020 47022 47030 47045 47101 47137 47194 47205 47253 47287 47364 47390 47407 47589 47598 47629 47647 47740 47780 47858 47894 47898 47903 47910 47930 47985 48032 48061 48105 48172 48249 48260 48309 48310 48334 48335 48355 48362 48402 48490 48519 48530 48531 48541 48545 48581 48607 48651 48652 48664 48705 48736 48757 48773 48821 48846 48883 48943 49064 49114 491283.322582951404819e-19 3.852589004194616e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/155/111?format=asciidefaultJ/AJ/155/111/table1Program starsSimbadNameSimbad column added by the CDSmeta.idcharIDPrimary identifier (G1)meta.id;meta.maincharprimaryHR[6/8969]? HR number (G1)meta.idintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintmoreindicates data in Tables 2-6 for this starmeta.ref.urlcharHDHD identifier (G1)meta.idcharHIP[57/118321]? Hipparcos number (Cat. I/239) (G1)meta.idintnullableCCDMIdentifier in the Catalog of Components of Double & Multiple stars (cat. I/274) (G1)meta.idcharm_CCDMCCDM componentmeta.code.multipcharClusterCluster identifier (G1)meta.idcharSpTypeMK spectral type (G1)src.spTypecharplx[5.41/796.92] Hipparcos parallax (G1)maspos.parallaxfloate_plx[0.14/25.9]? Error in plx (G1)masstat.error;pos.parallaxfloatnullableVmag[0.01/10.38] Apparent Johnson V band magnitude (G1)magphot.mag;em.opt.VfloatRV[-171.42/310.77]? Radial velocity (G1)km/sphys.veloc;pos.heliocentricdoublenullablee_RV[0/7.4]? Error in RV (G1)km/sstat.errorfloatnullablel_vsin(i)[<] Limit flag on vsin(i)meta.code.errorcharvsin(i)[0/100]? Literature projected rotational velocitykm/sphys.veloc.rotatfloatnullableDist[1.3/184.8] Distancepcpos.distance;pos.heliocentricfloatE(B-V)[0/0.042] The (B-V) color excess (1)magphot.color.excessfloatVMag[3.01/8.4] Absolute V band magnitudemagphys.magAbs;em.opt.VfloatHost[H] Indicates system hosts planet(s) (2)meta.codechar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/AJ/155/111/table2Effective temperature, mass, and age datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDPrimary identifier (G1)meta.id;meta.maincharTeff[4174/6815] Effective temperatureKphys.temperature.effectiveinte_Teff[8/99]? Standard deviation in TeffKstat.error;phys.temperature.effectiveintnullableo_Teff[1/13] Number of color(s) used to derive Teffmeta.numberintlogL[-1.12/0.79] Log luminosity (logL/L_{Sun}_)log(solLum)phys.luminosityfloatB1Mass[0.62/1.45]? Mass determined from the Bertelli et al. (1994, J/A+AS/106/275) isochronessolMassphys.massfloatnullableB1Age[0.63/12.02]? Age determined from the Bertelli et al. (1994, J/A+AS/106/275) isochronesGyrtime.agefloatnullableDMass[0.57/1.49]? Mass determined from the Dotter et al. (2008ApJS..178...89D) isochronessolMassphys.massfloatnullableDAge[0.6/12.5]? Age determined from the Dotter et al. (2008ApJS..178...89D) isochronesGyrtime.agefloatnullableYMass[0.58/1.51]? Mass determined from the Demarque et al. (2004ApJS..155..667D) isochronessolMassphys.massfloatnullableYAge[0.6/12.0]? Age determined from the Demarque et al. (2004ApJS..155..667D) isochronesGyrtime.agefloatnullableB2Mass[0.56/1.48]? Mass determined from the BaSTI Team (2016) isochrones (1)solMassphys.massfloatnullableB2Age[0.6/12.5]? Age determined from the BaSTI Team (2016) isochrones (1)Gyrtime.agefloatnullableMassavg[0.57/1.47]? Average masssolMassphys.massfloatnullableMRange[0/0.49]? Range in mass determinationsolMassstat.errorfloatnullableAgeavg[0.6/12.13]? Average ageGyrtime.age;stat.meanfloatnullableARange[0/10.79]? Range in age determinationGyrstat.errorfloatnullableMass[0.57/1.47] Adopted mass (2)solMassphys.massfloatlogg[3.79/5.13] Log surface gravity (G2)log(cm.s**-2)phys.gravityfloatJ/AJ/155/111/table3Parameter and iron datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDPrimary identifier (G1)meta.id;meta.maincharTeff[4174/6815] Effective temperatureKphys.temperature.effectiveintlogg[3.79/5.13] Log surface gravity (G2)log(cm.s**-2)phys.gravityfloatVt[0.17/5] Microturbulent velocitykm/sphys.velocfloatVbroad[1.2/80] Broadening velocity (G3)km/sspect.line.broadfloat[FeI/H][5.43/8.39] Total iron abundance computed from neutral iron lines (1)phys.abund.Fe;meta.modelledfloate_[FeI/H][0.02/1.18] Standard deviation in [FeI/H]stat.error;phys.abundfloato_[FeI/H][2/548] Number of neutral iron lines used to calculate [FeI/H]meta.numberint[FeII/H][5.42/9.37]? Total iron abundance computed from first-ionization stage iron lines (1)phys.abund.Fe;meta.modelledfloatnullablee_[FeII/H][0.03/1.29]? Standard deviation in [FeII/H]stat.error;phys.abundfloatnullableo_[FeII/H][1/81]? Number of first-ionization stage iron lines used to calculate [FeII/H]meta.numberintnullable[Fe/H][-2.04/1.02] Differential value in logarithms relative to the solar abundance for iron (2)log(Sun)stat.value;arith.difffloatJ/AJ/155/111/table4[x/H] for Z > 10recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDPrimary identifier (G1)meta.id;meta.maincharTeff[4174/6815] Effective temperatureKphys.temperature.effectiveintlogg[3.79/5.13] Log surface gravity (G2)log(cm.s**-2)phys.gravityfloatVt[0.17/5] Microturbulent velocitykm/sphys.velocfloatVbroad[1.2/80] Broadening velocity (G3)km/sspect.line.broadfloat[Na/H][-2.14/1.33]? Differential value in logarithm relative to the solar abundance for sodium (1)log(Sun)phys.abundfloatnullable[Mg/H][-1.81/1.09]? Differential value in logarithm relative to the solar abundance for magnesium (1)log(Sun)phys.abundfloatnullable[Al/H][-1.36/0.57]? Differential value in logarithm relative to the solar abundance for aluminum (1)log(Sun)phys.abundfloatnullable[Si/H][-1.48/0.97]? Differential value in logarithm relative to the solar abundance for silicon (1)log(Sun)phys.abundfloatnullable[S/H][-0.68/1.91]? Differential value in logarithm relative to the solar abundance for sulfur (1)log(Sun)phys.abundfloatnullable[Ca/H][-1.76/2.04]? Differential value in logarithm relative to the solar abundance for calcium (1)log(Sun)phys.abundfloatnullable[Sc/H][-1.97/2.7]? Differential value in logarithm relative to the solar abundance for scandium (1)log(Sun)phys.abundfloatnullable[Ti/H][-1.72/1.93] Differential value in logarithm relative to the solar abundance for titanium (1)log(Sun)phys.abundfloat[V/H][-2.38/2.07]? Differential value in logarithm relative to the solar abundance for vanadium (1)log(Sun)phys.abundfloatnullable[Cr/H][-2.11/1.62] Differential value in logarithm relative to the solar abundance for chromium (1)log(Sun)phys.abundfloat[Mn/H][-2.62/2.76]? Differential value in logarithm relative to the solar abundance for manganese (1)log(Sun)phys.abundfloatnullable[Fe/H][-2.04/1.03] Differential value in logarithm relative to the solar abundance for iron (1)log(Sun)phys.abundfloat[Co/H][-2.05/3.3]? Differential value in logarithm relative to the solar abundance for cobalt (1)log(Sun)phys.abundfloatnullable[Ni/H][-2.1/1.28] Differential value in logarithm relative to the solar abundance for nickel (1)log(Sun)phys.abundfloat[Cu/H][-1.61/0.94]? Differential value in logarithm relative to the solar abundance for copper (1)log(Sun)phys.abundfloatnullable[Zn/H][-2.04/0.71]? Differential value in logarithm relative to the solar abundance for zinc (1)log(Sun)phys.abundfloatnullable[Sr/H][-1.88/2.45]? Differential value in logarithm relative to the solar abundance for strontium (1)log(Sun)phys.abundfloatnullable[Y/H][-1.86/2.12]? Differential value in logarithm relative to the solar abundance for yttrium (1)log(Sun)phys.abundfloatnullable[Zr/H][-1.72/3.14]? Differential value in logarithm relative to the solar abundance for zirconium (1)log(Sun)phys.abundfloatnullable[Ba/H][-2.24/0.72]? Differential value in logarithm relative to the solar abundance for barium (1)log(Sun)phys.abundfloatnullable[La/H][-1.6/1.31]? Differential value in logarithm relative to the solar abundance for lanthanum (1)log(Sun)phys.abundfloatnullable[Ce/H][-1.06/3.48]? Differential value in logarithm relative to the solar abundance for cerium (1)log(Sun)phys.abundfloatnullable[Nd/H][-1.77/5.58]? Differential value in logarithm relative to the solar abundance for neodymium (1)log(Sun)phys.abundfloatnullable[Sm/H][-0.91/3.62]? Differential value in logarithm relative to the solar abundance for samarium (1)log(Sun)phys.abundfloatnullable[Eu/H][-0.23/0.71]? Differential value in logarithm relative to the solar abundance for europium (1)log(Sun)phys.abundfloatnullableJ/AJ/155/111/table5Lithium, carbon, and oxygen datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDPrimary identifier (G1)meta.id;meta.maincharTeff[4174/6815] Effective temperatureKphys.temperature.effectiveintlogg[3.79/5.13] Log surface gravity (G2)log(cm.s**-2)phys.gravityfloatVt[0.17/5] Microturbulent velocitykm/sphys.velocfloatVbroad[1.2/80] Broadening velocity (G3)km/sspect.line.broadfloat[Fe/H][-2.04/1.02] Iron abundance (1)log(Sun)phys.abund.Fefloatl_[Li/H][<] Upper limit flag on [Li/H]meta.code.error;phys.abundchar[Li/H][-0.5/3.4] Lithium abundance (2)phys.abundfloatNLTE[-0.04/0.19] Correction for non-local thermodynamic equilibriumarith.factorfloatC505.2[6.56/9.2]? Log carbon abundance from C I 505.2 nm linephys.abundfloatnullableC538.2[6.16/8.78]? Log carbon abundance from C I 538.2 nm linephys.abundfloatnullableC2[7.47/9.08]? Log carbon abundance from C2 Swan lines (primary indicator at 513.5 nm)phys.abundfloatnullableO615.5[8.08/9.46]? Log oxygen abundance from O I 615.5 nm tripletphys.abundfloatnullableO630.0[7.74/9.28]? Log oxygen abundance from [O I] 630.0 nm linephys.abundfloatnullableCmean[6.53/9.06]? Mean log carbon abundance (3)phys.abundfloatnullableOmean[7.74/9.28]? Mean log oxygen abundance (3)phys.abundfloatnullable[C/H]mean[-1.9/0.63]? Mean carbon abundance relative to the solar valuelog(Sun)phys.abundfloatnullable[O/H]mean[-0.95/0.59]? Mean oxygen abundance relative to the solar valuelog(Sun)phys.abundfloatnullable[C/Fe]mean[-1.24/0.82]? Mean carbon abundance relative to ironlog(Sun)phys.abundfloatnullable[O/Fe]mean[-0.44/1.2]? Mean oxygen abundance relative to ironlog(Sun)phys.abundfloatnullableJ/AJ/155/111/table6Log {epsilon} details for Z > 10o_logZrI[1/20]? Number of lines used to derive logZrImeta.numberintnullableo_logFeI[2/548] Number of lines used to derive logFeImeta.numberinto_logSiI[1/50]? Number of lines used to derive logSiImeta.numberintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDPrimary identifier (G1)meta.id;meta.maincharTeff[4174/6815] Effective temperatureKphys.temperature.effectiveintlogg[3.79/5.13] Log surface gravity (G2)log(cm.s**-2)phys.gravityfloatVt[0.17/5] Microturbulent velocitykm/sphys.velocfloatVbroad[1.2/80] Broadening velocity (G3)km/sspect.line.broadfloatlogNaI[4.14/7.61]? Mean log Na I number abundance (1)phys.abundfloatnullablee_logNaI[0.01/0.46]? Standard deviation in logNaIstat.errorfloatnullableo_logNaI[1/8]? Number of lines used to derive logNaImeta.numberintnullablelogMgI[5.87/8.77]? Mean log Mg I number abundance (1)phys.abundfloatnullablee_logMgI[0.02/0.59]? Standard deviation in logMgIstat.errorfloatnullableo_logMgI[1/8]? Number of lines used to derive logMgImeta.numberintnullablelogAlI[5.16/7.08]? Mean log Al I number abundance (1)phys.abundfloatnullablee_logAlI[0/0.4]? Standard deviation in logAlIstat.errorfloatnullableo_logAlI[1/3]? Number of lines used to derive logAlImeta.numberintnullablelogSiI[6.05/8.6]? Mean log Si I number abundance (1)phys.abundfloatnullablee_logSiI[0.02/1.32]? Standard deviation in logSiIstat.errorfloatnullablelogSiII[5.84/10.47]? Mean log Si II number abundance (1)phys.abundfloatnullablee_logSiII[0/0.57]? Standard deviation in logSiIIstat.errorfloatnullableo_logSiII[1/2]? Number of lines used to derive logSiIImeta.numberintnullablelogSI[6.56/9.14]? Mean log S I number abundance (1)phys.abundfloatnullablee_logSI[0/0.97]? Standard deviation in logSIstat.errorfloatnullableo_logSI[1/8]? Number of lines used to derive logSImeta.numberintnullablelogCaI[-1.69/2.11]? Mean log Ca I number abundance (1)phys.abundfloatnullablee_logCaI[0.03/0.59]? Standard deviation in logCaIstat.errorfloatnullableo_logCaI[1/41]? Number of lines used to derive logCaImeta.numberintnullablelogCaII[-0.56/2.76]? Mean log Ca II number abundance (1)phys.abundfloatnullablee_logCaII[0/1.29]? Standard deviation in logCaIIstat.errorfloatnullableo_logCaII[1/4]? Number of lines used to derive logCaIImeta.numberintnullablelogScI[2.05/5.87]? Mean log Sc I number abundance (1)phys.abundfloatnullablee_logScI[0.01/1.04]? Standard deviation in logScIstat.errorfloatnullableo_logScI[1/15]? Number of lines used to derive logScImeta.numberintnullablelogScII[1.2/4.71]? Mean log Sc II number abundance (1)phys.abundfloatnullablee_logScII[0.01/0.69]? Standard deviation in logScIIstat.errorfloatnullableo_logScII[1/17]? Number of lines used to derive logScIImeta.numberintnullablelogTiI[3.31/6.92] Mean log Ti I number abundance (1)phys.abundfloate_logTiI[0.04/1.65] Standard deviation in logTiIstat.errorfloato_logTiI[2/172] Number of lines used to derive logTiImeta.numberintlogTiII[3.16/6.56]? Mean log Ti II number abundance (1)phys.abundfloatnullablee_logTiII[0.03/1.18]? Standard deviation in logTiIIstat.errorfloatnullableo_logTiII[1/50]? Number of lines used to derive logTiIImeta.numberintnullablelogVI[1.53/5.98]? Mean log V I number abundance (1)phys.abundfloatnullablee_logVI[0.03/2.63]? Standard deviation in logVIstat.errorfloatnullableo_logVI[1/76]? Number of lines used to derive logVImeta.numberintnullablelogVII[1.79/7.05]? Mean log V II number abundance (1)phys.abundfloatnullablee_logVII[0.01/1.27]? Standard deviation in logVIIstat.errorfloatnullableo_logVII[1/11]? Number of lines used to derive logVIImeta.numberintnullablelogCrI[3.43/7.35]? Mean log Cr I number abundance (1)phys.abundfloatnullablee_logCrI[0.03/1.3]? Standard deviation in logCrIstat.errorfloatnullableo_logCrI[1/156]? Number of lines used to derive logCrImeta.numberintnullablelogCrII[3.69/8.41]? Mean log Cr II number abundance (1)phys.abundfloatnullablee_logCrII[0/1.11]? Standard deviation in logCrIIstat.errorfloatnullableo_logCrII[1/20]? Number of lines used to derive logCrIImeta.numberintnullablelogMnI[2.85/8.24]? Mean log Mn I number abundance (1)phys.abundfloatnullablee_logMnI[0.04/1.13]? Standard deviation in logMnIstat.errorfloatnullableo_logMnI[1/41]? Number of lines used to derive logMnImeta.numberintnullablelogFeI[5.43/8.39] Mean log Fe I number abundance (1)meta.idfloate_logFeI[0.02/1.18] Standard deviation in logFeIstat.errorfloatlogFeII[5.42/9.37]? Mean log Fe II number abundance (1)meta.idfloatnullablee_logFeII[0.03/1.29]? Standard deviation in logFeIIstat.errorfloatnullableo_logFeII[1/81]? Number of lines used to derive logFeIImeta.numberintnullablelogCoI[2.89/8.24]? Mean log Co I number abundance (1)phys.abundfloatnullablee_logCoI[0/1.59]? Standard deviation in logCoIstat.errorfloatnullableo_logCoI[1/75]? Number of lines used to derive logCoImeta.numberintnullablelogNiI[4.12/7.5] Mean log Ni I number abundance (1)phys.abundfloate_logNiI[0.04/1.22]? Standard deviation in logNiIstat.errorfloatnullableo_logNiI[1/186] Number of lines used to derive logNiImeta.numberintlogCuI[2.61/5.16]? Mean log Cu I number abundance (1)phys.abundfloatnullablee_logCuI[0/1.25]? Standard deviation in logCuIstat.errorfloatnullableo_logCuI[1/6]? Number of lines used to derive logCuImeta.numberintnullablelogZnI[2.53/5.28]? Mean log Zn I number abundance (1)phys.abundfloatnullablee_logZnI[0.01/1.09]? Standard deviation in logZnIstat.errorfloatnullableo_logZnI[1/4]? Number of lines used to derive logZnImeta.numberintnullablelogSrI[1.09/5.42]? Mean log Sr I number abundance (1)phys.abundfloatnullablee_logSrI[0/0.75]? Standard deviation in logSrIstat.errorfloatnullableo_logSrI[1/4]? Number of lines used to derive logSrImeta.numberintnullablelogYI[0.39/5.53]? Mean log Y I number abundance (1)phys.abundfloatnullablee_logYI[0.01/2.28]? Standard deviation in logYIstat.errorfloatnullableo_logYI[1/13]? Number of lines used to derive logYImeta.numberintnullablelogYII[0.43/4.14]? Mean log Y II number abundance (1)phys.abundfloatnullablee_logYII[0.02/0.76]? Standard deviation in logYIIstat.errorfloatnullableo_logYII[1/18]? Number of lines used to derive logYIImeta.numberintnullablelogZrI[1.7/5.82]? Mean log Zr I number abundance (1)phys.abundfloatnullablee_logZrI[0.01/1.13]? Standard deviation in logZrIstat.errorfloatnullablelogZrII[0.97/5.96]? Mean log Zr II number abundance (1)phys.abundfloatnullablee_logZrII[0/1.46]? Standard deviation in logZrIIstat.errorfloatnullableo_logZrII[1/15]? Number of lines used to derive logZrIImeta.numberintnullablelogBaII[0.08/3.04]? Mean log Ba II number abundance (1)phys.abundfloatnullablee_logBaII[0/0.31]? Standard deviation in logBaIIstat.errorfloatnullableo_logBaII[1/4]? Number of lines used to derive logBaIImeta.numberintnullablelogLaII[-0.37/2.54]? Mean log La II number abundance (1)phys.abundfloatnullablee_logLaII[0/1.01]? Standard deviation in logLaIIstat.errorfloatnullableo_logLaII[1/10]? Number of lines used to derive logLaIImeta.numberintnullablelogCeII[0.67/5.2]? Mean log Ce II number abundance (1)phys.abundfloatnullablee_logCeII[0.01/2.47]? Standard deviation in logCeIIstat.errorfloatnullableo_logCeII[1/39]? Number of lines used to derive logCeIImeta.numberintnullablelogPrII[-0.19/4.12]? Mean log Pr II number abundance (1)phys.abundfloatnullablee_logPrII[0.01/0.89]? Standard deviation in logPrIIstat.errorfloatnullableo_logPrII[1/8]? Number of lines used to derive logPrIImeta.numberintnullablelogNdII[-0.2/7.15]? Mean log Nd II number abundance (1)phys.abundfloatnullablee_logNdII[0.05/3.48]? Standard deviation in logNdIIstat.errorfloatnullableo_logNdII[1/42]? Number of lines used to derive logNdIImeta.numberintnullablelogSmII[0.18/4.71]? Mean log Sm II number abundance (1)phys.abundfloatnullablee_logSmII[0.01/2.19]? Standard deviation in logSmIIstat.errorfloatnullableo_logSmII[1/33]? Number of lines used to derive logSmIImeta.numberintnullablelogEuII[0.25/1.19]? Mean log Eu II number abundance (1)phys.abundfloatnullableo_logEuII[1]? Number of lines used to derive logEuIImeta.numberintnullable