J/A+A/549/A147ivo://CDS.VizieR/J/A+A/549/A147doi:10.26093/cds/vizier.35490147CDSBensby T.Yee J.C.Feltzing S.Johnson J.A.Gould A.Cohen J.G.,Asplund M.Melendez J.Lucatello S.Han C.Thompson I.Gal-Yam A.,Udalski A.Benett D.P.Bond I.A.Kohei W.Sumi T.Suzuki D.Suzuki K.,Takino S.Tristram P.Yamai N.Yonehara A.2017-06-21T08:21:45Z2013-01-17T07:42:30ZCDS support team

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

cds-question@unistra.frgravitational-lensingchemical-abundancesline-intensitiesWe perform a detailed elemental abundance analysis of dwarf stars in the Galactic bulge, based on high-resolution spectra that were obtained while the stars were optically magnified during gravitational microlensing events. The analysis method is the same as for a large sample of F and G dwarf stars in the Solar neighbourhood, enabling a fully differential comparison between the Bulge and the local stellar populations in the Galactic disc.2013A&A...549A.147Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/549/A147CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/549/A147https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/549/A147http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/549/A147https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/549/A147https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/549/A147http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/549/A147GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/549/A147/stars (Results for bulge stars: atmospheric parameters, velocities, ages, absolute magnitudes, abundance ratios)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/549/A147/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/549/A147/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/549/A147/stars?GETtext/xml+votable180.050000true270.1497917-28.18755560.0055555555555555565/7205 7216 6/28711 28717-28718 28729 28733-28734 28770 28777 28779-28780 28782-28783 28839 28857 28868 28870-28871 28873 28880 28882-28883 28888 29184 39770https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/549/A147?format=asciidefaultJ/A+A/549/A147/table2Equivalent widths and absolute abundances for individual linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintObjectObject name (in MOA, OGLE, or MACHO)meta.id;meta.maincharElElementphys.atmol.elementcharIonIonisation (1=neutral)phys.atmol.ionStageintlambdaLine wavelength0.1nmem.wl;spect.linedoubleLEPLower Excitation PotentialeVphys.atmol.excitation;stat.minfloatlog(gf)oscillator strengthphys.atmol.oscStrengthfloatWsun? Equivalent width of this line in the Sun0.1pmspect.line.eqWidthfloatnullableAsun? Sun absolute abundance (log scale, A(H)=12)phys.abundfloatnullableEW? Equivalent width of this line in the star0.1pmspect.line.eqWidthfloatnullableA? Absolute abundance (log scale, A(H)=12)phys.abundfloatnullableJ/A+A/549/A147/starsResults for bulge stars: atmospheric parameters, velocities, ages, absolute magnitudes, abundance ratiosnFeNumber of Fe lines usedmeta.numberintnCa? Number of Ca lines usedmeta.numberintnullableB_VMAG1-sigma upper estimate of VMAGmagphys.magAbs;em.opt.V;stat.maxfloatnNa? Number of Na lines usedmeta.numberintnullablenZn? Number of Zn lines usedphys.abundintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintObjectObject name (in MOA, OGLE, or MACHO)meta.id;meta.maincharprimaryTeffEffective temperatureKphys.temperature.effectiveinte_TeffError in TeffKstat.error;phys.temperature.effectiveintloggSurface gravitylog(cm.s**-2)phys.gravityfloate_loggError in logglog(cm.s**-2)stat.errorfloatxi(t)Microturbulence parameter {xi}km/sphys.veloc.microTurbfloate_xi(t)Error in xi(t)km/sstat.errorfloat[Fe/H]Metallicitylog(Sun)phys.abund.Zfloate_[Fe/H]Error in [Fe/H]log(Sun)stat.error;phys.abund.FefloatnFeINumber of Fe I lines usedmeta.numberintnFeII? Number of Fe II lines usedmeta.numberintnullableHRVHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentricfloatMStellar masssolMassphys.massfloatlogLLuminositylog(solLum)phys.luminosityfloatAgeStellar ageGyrtime.agefloatb_Age1-sigma lower estimate of AgeGyrtime.age;stat.minfloatB_Age1-sigma upper estimate of AgeGyrtime.age;stat.maxfloat(V-I)0Intrinsic (V-I)_0_ colour from spectroscopymagphot.color;em.opt.V;em.opt.IfloatVMAGAbsolute V magnitude from spectroscopymagphys.magAbs;em.opt.Vfloatb_VMAG1-sigma lower estimate of VMAGmagphys.magAbs;em.opt.V;stat.minfloatIMAGAbsolute I magnitude from spectroscopymagphys.magAbs;em.opt.IfloatIMAG.m? Absolute I magnitude from microlensingmagphys.magAbsfloatnullable(V-I)0.m? Intrinsic (V-I)_0_ colour from microlensingmagphot.color;em.opt.V;em.opt.IfloatnullableTeff.m? Effective temperature from microlensingKphys.temperature.effectiveintnullableSimbadSimbad column added by the CDSmeta.ref.urlchar[O/Fe]? Normalised Oxygen abundancelog(Sun)phys.abundfloatnullablee_[O/Fe]? Error in Oxygen abundance ratiolog(Sun)stat.error;phys.abundfloatnullablenO? Number of O lines usedphys.abundintnullable[Na/Fe]? Normalised Natrium abundancelog(Sun)phys.abundfloatnullablee_[Na/Fe]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullable[Mg/Fe]? Normalised Magnesium abundancelog(Sun)phys.abundfloatnullablee_[Mg/Fe]? Error in Mg abundance ratiolog(Sun)stat.error;phys.abundfloatnullablenMg? Number of Mg lines usedmeta.numberintnullable[Al/Fe]? Normalised Aluminium abundancelog(Sun)phys.abundfloatnullablee_[Al/Fe]? Error in Al abundance ratiolog(Sun)stat.error;phys.abundfloatnullablenAl? Number of Al lines usedphys.abundintnullable[Si/Fe]? Normalised Silicium abundancelog(Sun)phys.abundfloatnullablee_[Si/Fe]? Error in Si abundance ratiolog(Sun)stat.error;phys.abundfloatnullablenSi? Number of Si lines usedmeta.numberintnullable[Ca/Fe]? Normalised Calcium abundancelog(Sun)phys.abundfloatnullablee_[Ca/Fe]? Error in Ca abundance ratiolog(Sun)stat.error;phys.abundfloatnullable[Ti/Fe]? Normalised Titanium abundancelog(Sun)phys.abundfloatnullablee_[Ti/Fe]? Error in Ti abundance ratiolog(Sun)stat.error;phys.abundfloatnullablenTi? Number of Ti lines usedmeta.numberintnullable[Cr/Fe]? Normalised Chromium abundancelog(Sun)phys.abundfloatnullablee_[Cr/Fe]? Error in Cr abundance ratiolog(Sun)stat.error;phys.abundfloatnullablenCr? Number of Cr lines usedmeta.numberintnullable[Ni/Fe]? Normalised Nickel abundancelog(Sun)phys.abundfloatnullablee_[Ni/Fe]? Error in Ni abundance ratiolog(Sun)stat.error;phys.abundfloatnullablenNi? Number of Ni lines usedmeta.numberintnullable[Zn/Fe]? Normalised Zinc abundancelog(Sun)phys.abundfloatnullablee_[Zn/Fe]? Error in Zn abundance ratiolog(Sun)stat.error;phys.abundfloatnullable[Y/Fe]? Normalised Yttrium abundancelog(Sun)phys.abundfloatnullablee_[Y/Fe]? Error in Y abundance ratiolog(Sun)stat.error;phys.abundfloatnullablenY? Number of Y lines usedmeta.numberintnullable[Ba/Fe]? Normalised Barium abundancelog(Sun)phys.abundfloatnullablee_[Ba/Fe]? Error in Ba abundance ratiolog(Sun)stat.error;phys.abundfloatnullablenBa? Number of Ba lines usedphys.abundintnullable_RAPosition from Simbad and table 1 of the paper (right ascension part)degpos.eq.ra;meta.main_DEPosition from Simbad and table 1 of the paper (declination part)degpos.eq.dec;meta.main