J/A+A/608/A112ivo://CDS.VizieR/J/A+A/608/A112doi:10.26093/cds/vizier.36080112CDSNissen P.E.Silva Aguirre V.Christensen-Dalsgaard J.Collet R.,Grundahl F.Slumstrup D.2017-12-14T14:14:52Z2017-12-13T07:19:11ZCDS support team

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

cds-question@unistra.frchemical-abundancesHARPS-N spectra with S/N>250 and MARCS model atmospheres were used to derive abundances of C, O, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni, Zn, and Y in ten stars from the Kepler LEGACY sample including the binary pair 16 Cyg A and B. Stellar gravities and ages were obtained from seismic data and effective temperatures were determined by comparing non-LTE iron abundances derived from FeI and FeII lines. Available non-LTE corrections were also applied when deriving abundances of the other elements.2017A&A...608A.112Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/608/A112CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/133 : Kepler Input Catalog (Kepler Mission Team, 2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/608/A112https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/608/A112http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/608/A112https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/608/A112https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/608/A112http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/608/A112GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/608/A112/table1 (Stellar parameters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/608/A112/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/608/A112/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/608/A112/table1?GETtext/xml+votable180.050000true286.438585838.52293420.0055555555555555566/14757 14819 14921 14948 14959 14969 15062 15174 15178https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/608/A112?format=asciidefaultJ/A+A/608/A112/table1Stellar parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKepler Input Catalog number (Cat. V/133)meta.id;meta.mainintIDObject namemeta.idcharS/NSignal-to-noise ratio of HARPS-N spectrumstat.snrintTeff(ion)Effective temperature from ionization balanceKphys.temperature.effectiveinte_Teff(ion)rms uncertainty of Teff(ion)Kstat.errorintTeff(exc)Effective temperature from excitation balanceKphys.temperature.effectiveinte_Teff(exc)rms uncertainty of Teff(exc)Kstat.errorint[Fe/H]Logarithmic Fe/H ratiolog(Sun)phys.abund.Fe;arith.ratiofloate_[Fe/H]rms uncertainty of [Fe/H]log(Sun)stat.error;phys.abund.FefloatVturbMicroturbulence parameterkm/sstat.paramfloate_Vturbrms uncertainty of microturbulence parameterkm/sstat.errorfloatloggLogarithmic surface gravitylog(cm.s**-2)phys.gravityfloatAgeStellar asteroseismic ageGyrtime.agefloate_Agerms uncertainty of stellar ageGyrstat.error;time.agefloatvsiniProjected equatorial rotation velocitykm/sphys.veloc.rotatfloatSimbadSimbad column added by the CDSmeta.ref.urlchar_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/A+A/608/A112/table2Abundance ratiosrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKepler Input Catalog number (Cat. V/133)meta.id;meta.mainint[Fe/H]Logarithmic Fe/H ratiolog(Sun)phys.abund.Fe;arith.ratiofloate_[Fe/H]rms uncertainty of [Fe/H]log(Sun)stat.error;phys.abund.Fefloat[C/Fe]Logarithmic C/Fe ratiolog(Sun)phys.abundfloate_[C/Fe]rms uncertainty of [C/Fe]log(Sun)stat.error;phys.abundfloat[O/Fe]Logarithmic O/Fe ratiolog(Sun)phys.abundfloate_[O/Fe]rms uncertainty of [O/Fe]log(Sun)stat.error;phys.abundfloat[Na/Fe]Logarithmic Na/Fe ratiolog(Sun)phys.abundfloate_[Na/Fe]rms uncertainty of [Na/Fe]log(Sun)stat.error;phys.abundfloat[Mg/Fe]Logarithmic Mg/Fe ratiolog(Sun)phys.abundfloate_[Mg/Fe]rms uncertainty of [Mg/Fe]log(Sun)stat.error;phys.abundfloat[Al/Fe]Logarithmic Al/Fe ratiolog(Sun)phys.abundfloate_[Al/Fe]rms uncertainty of [Al/Fe]log(Sun)stat.error;phys.abundfloat[Si/Fe]Logarithmic Si/Fe ratiolog(Sun)phys.abundfloate_[Si/Fe]rms uncertainty of [Si/Fe]log(Sun)stat.error;phys.abundfloat[S/Fe]Logarithmic S/Fe ratiolog(Sun)phys.abundfloate_[S/Fe]rms uncertainty of [S/Fe]log(Sun)stat.error;phys.abundfloat[Ca/Fe]Logarithmic Ca/Fe ratiolog(Sun)phys.abundfloate_[Ca/Fe]rms uncertainty of [Ca/Fe]log(Sun)stat.error;phys.abundfloat[Ti/Fe]Logarithmic Ti/Fe ratiolog(Sun)phys.abundfloate_[Ti/Fe]rms uncertainty of [Ti/Fe]log(Sun)stat.error;phys.abundfloat[Cr/Fe]Logarithmic Cr/Fe ratiolog(Sun)phys.abundfloate_[Cr/Fe]rms uncertainty of [Cr/Fe]log(Sun)stat.error;phys.abundfloat[Ni/Fe]Logarithmic Ni/Fe ratiolog(Sun)phys.abundfloate_[Ni/Fe]rms uncertainty of [Ni/Fe]log(Sun)stat.error;phys.abundfloat[Zn/Fe]Logarithmic Zn/Fe ratiolog(Sun)phys.abundfloate_[Zn/Fe]rms uncertainty of [Zn/Fe]log(Sun)stat.error;phys.abundfloat[Y/Fe]Logarithmic Y/Fe ratiolog(Sun)phys.abundfloate_[Y/Fe]rms uncertainty of [Y/Fe]log(Sun)stat.error;phys.abundfloat