J/A+A/511/A56ivo://CDS.VizieR/J/A+A/511/A56doi:10.26093/cds/vizier.35110056CDSPancino E.Carrera R.RossettiE.Gallart C.2018-02-01T11:50:43Z2010-04-19T15:01:06ZCDS support team

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

cds-question@unistra.fropen-star-clustersgiant-starsline-intensitiesspectroscopyThe present number of Galactic open clusters that have high resolution abundance determinations, not only of [Fe/H], but also of other key elements, is largely insufficient to enable a clear modeling of the Galactic disk chemical evolution. To increase the number of Galactic open clusters with high quality measurements, we obtained high resolution (R~30000), high quality (S/N~50-100 per pixel), echelle spectra with the fiber spectrograph FOCES, at Calar Alto, Spain, for three red clump stars in each of five Open Clusters. We used the classical equivalent width analysis method to obtain accurate abundances of sixteen elements: Al, Ba, Ca, Co, Cr, Fe, La, Mg, Na, Nd, Ni, Sc, Si, Ti, V, and Y. We also derived the oxygen abundance using spectral synthesis of the 6300{AA} forbidden line.2010A&A...511A..56Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/511/A56CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/455/271 : Abundances of red giants in NGC 6441 (Gratton+, 2006)J/A+A/464/953 : Abundances of red giants in NGC 6441 (Gratton+, 2007)J/A+A/505/117 : Abund. of red giants in 15 globular clusters (Carretta+, 2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/511/A56https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/511/A56http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/511/A56https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/511/A56https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/511/A56http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/511/A56GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/511/A56/table1 (Observing logs and programme stars information)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/511/A56/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/511/A56/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/511/A56/table1?GETtext/xml+votable180.050000true99.718752.0328890.0055555555555555566/4298 6149 14175 22216 24522https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/511/A56?format=asciiOpticaldefaultJ/A+A/511/A56/table1Observing logs and programme stars informationrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterCluster namemeta.id.parentcharStarStar number within the clustermeta.id;meta.mainintprimaryRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainBmagB magnitudemagphot.mag;em.opt.BfloatVmagV magnitudemagphot.mag;em.opt.VfloatIcmag? Cousins I magnitudemagphot.mag;em.opt.IfloatnullableRmag? R magnitudemagphot.mag;em.opt.RfloatnullableKsmagKs magnitudemagphot.mag;em.IR.KfloatNExpNumber of exposuresmeta.numberintTExpTotal exposure timestime.duration;obs.exposureintS/NSignal-to-nois ratiostat.snrintSNameSimbad namemeta.idcharJ/A+A/511/A56/table5Atomic data and equivalent widthsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterCluster namemeta.id.parentcharStarStar number within the clustermeta.id;meta.mainintWaveWavelength 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