J/A+A/512/A41ivo://CDS.VizieR/J/A+A/512/A41doi:10.26093/cds/vizier.35120041CDSBensby T.Feltzing S.Johnson J.A.Gould A.Aden D.Asplund M.,Melendez J.Gal-Yam A.Lucatello S.Sana H.Sumi T.Miyake N.,Suzuki N.Han C.Bond I.Udalski A.2018-01-05T08:56:12Z2010-05-04T07:58:02ZCDS 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.2010A&A...512A..41Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/512/A41CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/499/737 : Abundances of microlensed dwarf & subgiants (Bensby+ 2009)J/A+A/533/A134 : Abundances of microlensed stars in the Bulge (Bensby+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/512/A41https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/512/A41http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/512/A41https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/512/A41https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/512/A41http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/512/A41GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/512/A41/table1 (Summary of the so far 15 dwarf star microlensing events in the Bulge that have been observed with high-resolution spectrographs)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/512/A41/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/512/A41/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/512/A41/table1?GETtext/xml+votable180.050000true269.632917-29.2049440.0055555555555555566/28711 28717 28734 28770 28779 28864-28866 28868 28870-28871 28873https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/512/A41?format=asciiOpticaldefaultJ/A+A/512/A41/table1Summary of the so far 15 dwarf star microlensing events in the Bulge that have been observed with high-resolution spectrographsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharprimaryn_Name[*] indicates the star MACHO 109.20893.3423meta.notecharEW[a] a for stars with data in table4meta.codecharAb[+] + for stars with data in table5meta.codecharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainGLON[-90/90] Galactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latfloatTEDuration of the eventdtime.intervalfloatTmaxTime when maximum magnification occured (HJD-2450000)dtime.epochfloatAmaxMaximum magnificationphot.mag;arith.ratiointTobsTime when event was observed with high-resolution spectrograph (MJD)dtime.epochdoubleTexpExposure timestime.duration;obs.exposureintS/NMeasured signal-to-noise ratio per pixel at ~6400{AA}stat.snr;instr.pixelintSpecSpectrograph usedmeta.id;instrcharRSpectral resolutionspect.resolutionintRefReference where the star first appeared (2)meta.ref;pos.framecharSimbadNameSimbad column added by the CDSmeta.idcharJ/A+A/512/A41/table4Equivalent widths and absolute abundances for individual lines (for 8 stars)ElElementphys.atmol.elementcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIonisation (1=neutral)phys.atmol.ionStage;phys.atmol.ionizationintlambdaWavelength0.1nmem.wldoubleLEPLower Excitation PotentialeVphys.atmol.excitation;stat.minfloatEWsunSolar equivalent width of the element0.1pmspect.line.eqWidthfloatA(Sun)Solar absolute abundance (log scale, A(H)=12)phys.abundfloatf_A(Sun)[0,1] 0 if line measured and used, 1 if average abundance from other lines usedmeta.codeintEW(076S)? Equivalent width OGLE-2009-BLG-076S0.1pmspect.line.eqWidthfloatnullableA(076S)? Absolute abundance OGLE-2009-BLG-076Sphys.abundfloatnullableEW(493S)? Equivalent width MOA-2009-BLG-493S0.1pmspect.line.eqWidthfloatnullableA(493S)? Absolute abundance MOA-2009-BLG-493Sphys.abundfloatnullableEW(133S)? Equivalent width MOA-2009-BLG-133S0.1pmspect.line.eqWidthfloatnullableA(133S)? Absolute abundance MOA-2009-BLG-133Sphys.abundfloatnullableEW(475S)? Equivalent width MOA-2009-BLG-475S0.1pmspect.line.eqWidthfloatnullableA(475S)? Absolute abundance MOA-2009-BLG-475Sphys.abundfloatnullableEW(022S)? Equivalent width MACHO-1999-BLG-022S0.1pmspect.line.eqWidthfloatnullableA(022S)? Absolute abundance MACHO-1999-BLG-022Sphys.abundfloatnullableEW(489S)? Equivalent width MOA-2009-BLG-489S0.1pmspect.line.eqWidthfloatnullableA(489S)? Absolute abundance MOA-2009-BLG-489Sphys.abundfloatnullableEW(456S)? Equivalent width MOA-2009-BLG-456S0.1pmspect.line.eqWidthfloatnullableA(456S)? Absolute abundance MOA-2009-BLG-456Sphys.abundfloatnullableEW(259S)? Equivalent width MOA-2009-BLG-259S0.1pmspect.line.eqWidthfloatnullableA(259S)? Absolute abundance MOA-2009-BLG-259Sphys.abundfloatnullableJ/A+A/512/A41/table5Abundances and uncertainties for each stare_[O/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.mainchar[Fe/H]Normalised abundancelog(Sun)phys.abundfloate_[Fe/H]? Error in abundance ratiolog(Sun)stat.error;phys.abund.Fefloatnullable[O/Fe]? Normalised abundance (not NLTE corrected)log(Sun)phys.abundfloatnullable[Na/Fe]? Normalised abundancelog(Sun)phys.abundfloatnullablee_[Na/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Mg/Fe]Normalised abundancelog(Sun)phys.abundfloate_[Mg/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Al/Fe]Normalised abundancelog(Sun)phys.abundfloate_[Al/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Si/Fe]Normalised abundancelog(Sun)phys.abundfloate_[Si/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Ca/Fe]Normalised abundancelog(Sun)phys.abundfloate_[Ca/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Ti/Fe]Normalised abundancelog(Sun)phys.abundfloate_[Ti/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Cr/Fe]? Normalised abundancelog(Sun)phys.abundfloatnullablee_[Cr/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Ni/Fe]Normalised abundancelog(Sun)phys.abundfloate_[Ni/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Zn/Fe]? Normalised abundancelog(Sun)phys.abundfloatnullablee_[Zn/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Y/Fe]? Normalised abundancelog(Sun)phys.abundfloatnullablee_[Y/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullable[Ba/Fe]Normalised abundancelog(Sun)phys.abundfloate_[Ba/Fe]? Error in abundance ratiolog(Sun)phys.abundfloatnullablee_[O/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Na/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Mg/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Al/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Si/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Ca/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Ti/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Cr/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Ni/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Zn/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Y/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablee_[Ba/H]? Error in abundance ratiolog(Sun)stat.error;phys.abundfloatnullablen(Fe)? Number of Fe lines usedmeta.numberintnullablen(O)? Number of O lines usedmeta.numberintnullablen(Na)? Number of Na lines usedmeta.numberintnullablen(Mg)? Number of Mg lines usedmeta.numberintnullablen(Al)? Number of Al lines usedmeta.numberintnullablen(Si)? Number of Si lines usedmeta.numberintnullablen(Ca)? Number of Ca lines usedmeta.numberintnullablen(Ti)? Number of Ti lines usedmeta.numberintnullablen(Cr)? Number of Cr lines usedmeta.numberintnullablen(Ni)? Number of Ni lines usedmeta.numberintnullablen(Zn)? Number of Zn lines usedmeta.numberintnullablen(Y)? Number of Y lines usedmeta.numberintnullablen(Ba)? Number of Ba lines usedmeta.numberintnullable