J/A+A/535/A30ivo://CDS.VizieR/J/A+A/535/A30doi:10.26093/cds/vizier.35350030CDSCarrera R.Pancino E.2018-01-04T08:23:13Z2011-10-27T07:17:56ZCDS support team

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

cds-question@unistra.fropen-star-clustersline-intensitiesOpen clusters are ideal test particles for studying the chemical evolution of the Galactic disc. However, the number and accuracy of existing high-resolution abundance determinations, not only of [Fe/H], but also of other key elements, remains largely insufficient. We attempt to increase the number of Galactic open clusters that have high quality abundance determinations, and to gather all the literature determinations published so far.2011A&A...535A..30Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/535/A30CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/511/A56 : Abundances of five open clusters (Pancino+, 2010)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/535/A30https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/535/A30http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/535/A30https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/535/A30https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/535/A30http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/535/A30GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/535/A30/table1 (Observing logs and programme star properties)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/535/A30/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/535/A30/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/535/A30/table1?GETtext/xml+votable180.050000true104.5341676.4054440.0055555555555555566/341 2433 2436 4698 22239 23533 235477.952274030004205e-20 4.920466254354166e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/535/A30?format=asciiOpticaldefaultJ/A+A/535/A30/table1Observing logs and programme star propertiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterCluster namemeta.id.parentcharStarStar number within the clustermeta.idintRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainBmagB magnitudemagphot.mag;em.opt.BfloatVmagV magnitudemagphot.mag;em.opt.VfloatRmag? R magnitudemagphot.mag;em.opt.RfloatnullableIcmag? Cousins I magnitudemagphot.mag;em.opt.IfloatnullableKsmagKs magnitudemagphot.mag;em.IR.KfloatNexpNumber of exposuresmeta.numberintTexpTotal exposure timestime.duration;obs.exposureintS/NSignal-to-noise ratiostat.snrintSNameSimbad namemeta.idcharSimbadSimbad column added by the CDScharJ/A+A/535/A30/table5Equivalent widths and atomic data of the programme starsClusterCluster namemeta.id.parentcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar number within the clustermeta.idintlambdaWavelength in Angstroms0.1nmem.wlfloatElElement namemeta.id;phys.atmol.elementcharionIonization stage (1 for neutral element)phys.atmol.ionStageintchiExExcitation potentialeVphys.atmol.excitationfloatloggfLogarithm of the oscillator strengthphys.atmol.oscStrengthfloatEW? Equivalent width (in mA)0.1pmspect.line.eqWidthfloatnullablee_EW? rms uncertainty on EW0.1pmstat.error;spect.line.eqWidthfloatnullableQ? DAOSPEC quality parameter Q (large values are bad)meta.code.qualfloatnullable