J/ApJ/711/L48ivo://CDS.VizieR/J/ApJ/711/L48doi:10.26093/cds/vizier.17119048CDSCohen J.G.Gould A.Thompson I.B.Feltzing S.Bensby T.Johnson J.A.,Huang W.Melendez J.Lucatello S.Asplund M.2013-03-10T16:19:52Z2013-03-01T12:55:02ZCDS support team

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

cds-question@unistra.frgravitational-lensingWe study a sample of 16 microlensed Galactic bulge main-sequence turnoff region stars for which high-dispersion spectra have been obtained with detailed abundance analyses. We demonstrate that there is a very strong and highly statistically significant correlation between the maximum magnification of the microlensed bulge star and the value of the [Fe/H] deduced from the high resolution spectrum of each object.2010ApJ...711L..48Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/711/L48CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/AcA/50/1 : OGLE microlensing events in Galactic Bulge (Udalski+, 2000)J/AcA/51/175 : OGLE-II DIA microlensing events (Wozniak+, 2001)J/MNRAS/343/1131 : 1998-2000 OGLE events microlensing limits (Tsapras+, 2003)J/ApJ/631/906 : MACHO Galactic Bulge microlensing events (Thomas+, 2005)J/A+A/466/157 : Bulge Microlensing Events (Soto+, 2007)http://www.astrouw.edu.pl/~ogle/ogle3 : OGLE3 Home Pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/711/L48https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/711/L48http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/711/L48https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/711/L48https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/711/L48http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/711/L48GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/ApJ/711/L48/table2Check of 2008 OGLE Bulge microlensing alertsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintOGLEThe OGLE identification numberintu0Separation for lens (1)floattEEinstein radius crossing time (2)dfloatImagUnlensed source I band magnitudemagfloatCode[1/2] 1=original values unchanged, 2=alteredint