J/MNRAS/423/122ivo://CDS.VizieR/J/MNRAS/423/122doi:10.26093/cds/vizier.74230122CDSBruntt H.Basu S.Smalley B.Chaplin W.J.Verner G.A.Bedding T.R.,Catala C.Gazzano J.-C.Molenda-Zakowicz J.Thygesen A.O.,Uytterhoeven K.Hekker S.Huber D.Karoff C.Mathur S.Mosser B.,Appourchaux T.Campante T.L.Elsworth Y.Garcia R.A.Handberg R.,Metcalfe T.S.Quirion P.-O.Regulo C.Roxburgh I.W.Stello D.,Christensen-Dalsgaard J.Kawaler S.D.Kjeldsen H.Morris R.L.,Quintana E.V.Sanderfer D.T.2024-07-17T20:15:58Z2013-05-02T15:47:56ZCDS support team

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

cds-question@unistra.frdwarf-starsg-starschemical-abundancesWe present a detailed spectroscopic study of 93 solar-type stars that are targets of the NASA/Kepler mission and provide detailed chemical composition of each target. We find that the overall metallicity is well represented by Fe lines. Relative abundances of light elements (CNO) and {alpha} elements are generally higher for low-metallicity stars. Our spectroscopic analysis benefits from the accurately measured surface gravity from the asteroseismic analysis of the Kepler light curves. The accuracy on the log g parameter is better than 0.03dex and is held fixed in the analysis.2012MNRAS.423..122Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/423/122CatalogResearchIsServedByTAP 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/MNRAS/423/122https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/423/122http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/423/122https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/423/122https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/423/122http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/423/122GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/423/122/table3 (Observed targets and their properties)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/423/122/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/423/122/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/423/122/table3?GETtext/xml+votable180.050000true290.888432537.08937060.0055555555555555565/3694 3776 6/14573 14578 14581 14591 14734 14751 14754 14757 14763 14765 14767 14770 14774 14794 14818-14819 14824 14827 14918 14921-14922 14926 14930-14933 14935 14938-14939 14941 14947-14948 14952 14958-14962 14966-14969 15041 15044 15057 15061-15062 15108 15110 15112 15118 15121 15124 15126 15131-15132 15141 15143-15146 15156 15168 15170 151783.4014663096393355e-19 4.067783865629509e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/423/122?format=asciiOpticaldefaultJ/MNRAS/423/122/table1Atomic data used in the spectral analysisrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElElement with ionization statephys.atmol.element;phys.atmol.ionizationcharlambdawavelength {lambda} ({AA})0.1nmem.wldoubleEpexcitation potentialeVphys.atmol.excitationfloatloggfVOscillator strength from VALDphys.atmol.oscStrengthfloatloggfAdjusted oscillator strength valuephys.atmol.oscStrengthfloatJ/MNRAS/423/122/table3Observed targets and their propertiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKIC number (Cat. V/133)meta.id;meta.mainintprimaryHIP? HIP number (Cat. I/311)meta.idintnullableHD? HD number (Cat. III/135)meta.idintnullableVTmagTycho V magnitudemagphot.mag;em.opt.VfloatVT-KVT-Ks colour indexmagphot.color;em.opt.V;em.IR.KfloatE(B-V)? B-V colour excessmagphot.color.excessfloatnullablee_E(B-V)? rms uncertainty on E(B-V)magstat.errorfloatnullableTeff1? Effective temperature from KICKphys.temperature.effectiveintnullablelogg1? Gravity surface from KIClog(cm.s**-2)phys.gravityfloatnullable[Fe/H]1? Metallicity from KIClog(Sun)phys.abund.ZfloatnullableTeff2Effective temperature from spectroscopy (+/-70K)Kphys.temperature.effectiveintlogg2Gravity surface from spectroscopy (+/-0.08dex)log(cm.s**-2)phys.gravityfloatTeffFinal (asteroseismic) effective temperature (+/-60K)Kphys.temperature.effectiveintloggFinal (asteroseismic) gravity surface (+/-0.03dex)log(cm.s**-2)phys.gravityfloat[Fe/H]Final (asteroseismic) metallicity (+/-0.06dex)phys.abund.ZfloatxiFinal (asteroseismic) microturbulent velocity {xi} (+/-0.06km/s) (1)km/sphys.veloc;phys.atmol.finalfloatvsiniFinal (asteroseismic) rotational velocity (1)km/sphys.veloc.rotatfloatKepDisplay the KIC (Cat. V/133) datameta.ref.urlcharSimbadSimbad column added by the CDSmeta.refchar_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/MNRAS/423/122/table4Abundances relative to the Sun and the number of lines used for 13 elementsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKICKIC number (1)meta.id;meta.mainintIon[1/2] Ionisation state: 1 for neutral, 2 for singly-ionizedphys.atmol.ionStageintLi? Lithum abundance (2)log(Sun)phys.abundfloatnullablee_Li? rms uncertainty on Lilog(Sun)stat.errorfloatnullableo_Li? Number of lines used for Limeta.numberintnullableC? Carbon abundance (2)log(Sun)phys.abundfloatnullablee_C? rms uncertainty on Clog(Sun)stat.errorfloatnullableo_C? Number of lines used for Cmeta.numberintnullableN? Nitrogen abundance (2)log(Sun)phys.abundfloatnullablee_N? rms uncertainty on Nlog(Sun)stat.errorfloatnullableo_N? Number of lines used for Nmeta.numberintnullableO? Oxygen abundance (2)log(Sun)phys.abundfloatnullablee_O? rms uncertainty on Olog(Sun)stat.errorfloatnullableo_O? Number of lines used for Ometa.numberintnullableNa? Sodium abundance (2)log(Sun)phys.abundfloatnullablee_Na? rms uncertainty on Nalog(Sun)stat.errorfloatnullableMg? Magnesium abundance (2)log(Sun)phys.abundfloatnullablee_Mg? rms uncertainty on Mglog(Sun)stat.errorfloatnullableo_Mg? Number of lines used for Mgmeta.numberintnullableSi? Silicium abundance (2)log(Sun)phys.abundfloatnullablee_Si? rms uncertainty on Silog(Sun)stat.errorfloatnullableo_Si? Number of lines used for Simeta.numberintnullableCa? Calcium abundance (2)log(Sun)phys.abundfloatnullablee_Ca? rms uncertainty on Calog(Sun)stat.errorfloatnullableo_Ca? Number of lines used for Cameta.numberintnullableTi? Titanium abundance (2)log(Sun)phys.abundfloatnullablee_Ti? rms uncertainty on Tilog(Sun)stat.errorfloatnullableo_Ti? Number of lines used for Timeta.numberintnullableV? Vanadium abundance (2)log(Sun)phys.abundfloatnullablee_V? rms uncertainty on Vlog(Sun)stat.error;pos.cartesian.yfloatnullableo_V? Number of lines used for Vmeta.numberintnullableCr? Chromium abundance (2)log(Sun)phys.abundfloatnullablee_Cr? rms uncertainty on Crlog(Sun)stat.errorfloatnullableo_Cr? Number of lines used for Crmeta.numberintnullableFe? Iron abundance (2)log(Sun)phys.abundfloatnullablee_Fe? rms uncertainty on Felog(Sun)stat.error;phys.abund.Fefloatnullableo_Fe? Number of lines used for Femeta.numberintnullableNi? Nickel abundance (2)log(Sun)phys.abundfloatnullablee_Ni? rms uncertainty on Nilog(Sun)stat.errorfloatnullableo_Ni? Number of lines used for Nimeta.numberintnullableo_Na? Number of lines used for Nameta.numberintnullable