J/A+A/410/527ivo://CDS.VizieR/J/A+A/410/527doi:10.26093/cds/vizier.34100527CDSBensby T.Feltzing S.Lundstrom I.2017-12-07T07:27:14Z2003-12-27T21:02:56ZCDS support team

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

cds-question@unistra.frchemically-peculiar-starsIn table 3 we list all spectral lines that have been used in the determination of abundances. Column 1 gives the wavelength (in Angstrom), column 2 the lower excitation potential (in eV), column 3 the correction factor to the classical Unsoeld damping constant, and column 5 the radiation damping constant. An "S" in column 4 indicates that the broadening by collisions have been taken from Anstee & O'Mara (1995MNRAS.276..859A), Barklem & O'Mara (1997MNRAS.290..102B, 1998MNRAS.300..863B), and Barklem et al. (1998MNRAS.296.1057B, 2000, Cat. <J/A+AS/142/467>), instead of the classical Unsoeld broadening (indicated by a "U"). The solar abundance that is given for each element is the photospheric value from Grevesse & Sauval (1998SSRv...85..161G ). Column 6 gives our adopted log gf - values and column 7 the references. In table 6 we give the derived abundances for all individual elements (atoms and ions). The results for each star consist of three rows. The top row gives the mean abundance, the middle row gives the (1 sigma) standard deviation around the mean, and the third row gives the number of spectral lines that was used in computing the mean. All abundances are given relatively our solar values, which in turn is normalized to the standard photospheric values in Grevesse & Sauval (1998SSRv...85..161G ).2003A&A...410..527Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/410/527CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/410/527https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/410/527http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/410/527https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/410/527https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/410/527http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/410/527GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/410/527/table6 (Elemental abundances)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/410/527/table6?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/410/527/table6?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/410/527/table6?GETtext/xml+votable180.050000true6/12621 14419 16386 16679 17301 17606 18035 18123 18614 18821 19345 20145 20593 21177 21179 22823 23096 23201 28763 28987 29210 29721 30848 31029 31130 31132 31172 31619 31768 32473 32552 33456 33717 33774 33910 34204 35080 35533 35576 35968 36035 36365 36693 37408 38918 41272 41764 41941 42042 42115 42248 42326 42486 42760 45364 45485 45669 46076 46593 46681 47073 48065 48105 48283 48687 49114https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/410/527?format=asciiOpticaldefaultJ/A+A/410/527/table6Elemental abundancese_NaISpread in [NaI/H] (2)stat.errorfloatFeIIMean abundance [FeII/H]phys.abundfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHIPHipparcos catalogue numbermeta.id;meta.mainintMem[1,3] Stellar population membership (1)meta.code.memberintFeIMean abundance [FeI/H]phys.abundfloate_FeISpread in [FeI/H] (2)stat.errorfloato_FeINumber of lines usedmeta.numberinte_FeIISpread in [FeII/H] (2)stat.errorfloato_FeIINumber of lines usedmeta.numberintNaIMean abundance [NaI/H]phys.abundfloato_NaINumber of lines usedmeta.numberintMgIMean abundance [MgI/H]phys.abundfloate_MgISpread in [MgI/H] (2)stat.errorfloato_MgINumber of lines usedmeta.numberintAlIMean abundance [AlI/H]phys.abundfloate_AlISpread in [AlI/H] (2)stat.errorfloato_AlINumber of lines usedmeta.numberintSiIMean abundance [SiI/H]phys.abundfloate_SiISpread in [SiI/H] (2)stat.errorfloato_SiINumber of lines usedmeta.numberintCaIMean abundance [CaI/H]phys.abundfloate_CaISpread in [CaI/H] (2)stat.errorfloato_CaINumber of lines usedmeta.numberintTiIMean abundance [TiI/H]phys.abundfloate_TiISpread in [TiI/H] (2)stat.errorfloato_TiINumber of lines usedmeta.numberintTiIIMean abundance [TiII/H]phys.abundfloate_TiIISpread in [TiII/H] (2)stat.errorfloato_TiIINumber of lines usedmeta.numberintCrIMean abundance [CrI/H]phys.abundfloate_CrISpread in [CrI/H] (2)stat.errorfloato_CrINumber of lines usedmeta.numberintCrIIMean abundance [CrII/H]phys.abundfloate_CrIISpread in [CrII/H] (2)stat.errorfloato_CrIINumber of lines usedmeta.numberintNiIMean abundance [NiI/H]phys.abundfloate_NiISpread in [NiI/H] (2)stat.errorfloato_NiINumber of lines usedmeta.numberintZnIMean abundance [ZnI/H]phys.abundfloate_ZnISpread in [ZnI/H] (2)stat.errorfloato_ZnINumber of lines usedmeta.numberintSimbadSimbad column added by the CDSmeta.refchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.mainnullable_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainnullableJ/A+A/410/527/refsReferences for log gf-values in table3.datrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefAbbreviation for the referencemeta.refcharBibCodeBibcodemeta.bib.bibcodecharAutAuthor's namemeta.bib.authorcharJ/A+A/410/527/table3Atomic line datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElemElementphys.atmol.elementcharIonIonisation (1=neutral, 2=ionised)phys.atmol.ionizationintLambdaWavelength0.1nmem.wldoubleLELower excitation potentialeVphys.energy;phys.atmol.excitationfloatdG6Correction factor to Unsoeld dampingphys.damping;phys.atmolfloatDMP[SU] U: Unsoeld damping, S: Barklem dampingmeta.notechargammaRadRadiation dampings**-1stat.paramdoubleloggfOscillator strengthphys.atmol.wOscStrengthfloatr_loggfReference for loggf (see refs.dat)meta.refchar