J/MNRAS/450/1900ivo://CDS.VizieR/J/MNRAS/450/1900doi:10.26093/cds/vizier.74501900CDSAdibekyan V.Zh.Sousa S.G.Santos N.C.Delgado Mena E.,Gonzalez Hernandez J. I.Israelian G.Mayor M.Khachatryan G.,Adibekyan V.Benamati L.Santos N.C.Alves S.Lovis C.Udry S.,Israelian G.Sousa S.G.Tsantaki M.Mortier A.Sozzetti A.,De Medeiros J.R.2024-08-14T20:21:38Z2015-04-30T12:07:28ZCDS support team

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

cds-question@unistra.frsolar-system-planetschemically-peculiar-starsWe performed a uniform and detailed abundance analysis of 12 refractory elements for a sample of 257 G- and K-type evolved stars from the CORALIE planet search program. This sample, being homogeneously analyzed, can be used as a comparison sample for other planet-related studies, as well as for different type of studies related to stellar and Galaxy astrophysics. The abundances of the chemical elements were determined using an LTE abundance analysis relative to the Sun, with the spectral synthesis code MOOG and a grid of Kurucz ATLAS9 atmospheres. To separate the Galactic stellar populations both a purely kinematical approach and a chemical method were applied.2015MNRAS.450.1900Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/450/1900CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/410/527 : Abundances in the Galactic disk (Bensby+, 2003)J/A+A/418/551 : Galactic disk stars abund. & velocities (Mishenina+, 2004)J/MNRAS/367/1329 : Elemental abundances for 176 stars (Reddy+, 2006)J/A+A/497/563 : Chemical abundances of 451 stars (Neves+, 2009)J/A+A/545/A32 : Chemical abundances of 1111 FGK stars (Adibekyan+, 2012)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/450/1900https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/450/1900http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/450/1900https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/450/1900https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/450/1900http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/450/1900GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/450/1900/stars (Combined table from original tables)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/450/1900/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/450/1900/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/450/1900/stars?GETtext/xml+votable180.050000true2.3526731-45.74742530.0055555555555555566/16442 16496 16519 20513 20548 20556 20614 20751 21026 24804 24838 25097 28687 28776 28782 28934 28968 32834 32866 32873 32904 33014 33018 33059 33073 33206 33214 33221-33223 33308 33338 33364 33377 33383 33398 33471 33535 33538 33545-33546 33557 33675 33749 33761 33786 33797 33822 33921 33995 34021 34051 34206 34255 34288 34338 34343 34520 34664 34666 34730 34869 34890 34968 35025 35116 35154 35170 35185 35191 35225 35264 35290 35351 35396 35415 35451 35459 35494 35597 35602 35673 35958 35984 36032 36892 36916 36973 37032 37091 37202 37239 37260 37276 37322 37343 37398 37407 37412 37423 37427 37435 37491 37498 37507 37642 37648 37664 37684 37712 37718 37723 37731 37779 37828 37934 37937 38027 38107 38137 38158 38333 38404 38419 38494 38501 38530 38543 38584 38651 38696 38779 38915 38954 38990 38996 39001 39009 39026 39034 39058 39090 39183 39256 39297 39302 39323 39336 39343 39363 39397 39399 39443 39605 39615 39680 39685 39879 39888 39939 39978 40048 40090 40106 40989 41008 41064 41193 41220 41298 41323 41376 41594 41672 41734 41765 41775 41839 41887 41899 42005 42051 42080 42145 42172 42441 42462 42514 42598 42661 42686 42689 42702 42727 42750 42921 43032 43176 43275 43285 43424 43430 43442 43602 43621 43686 43922 45124 45138 45171 45176 45438 45489 45616 45627 45721 45752 46110 46334 46389 46395 46491 46502 46705 46714 46851 46918 46958 46960 47011 47113 47181 47193 47207 47237 47263 47336 47354 47396 47424 47433 47586 47640 47652 47715 47745 47807 47809 47823 47991 48147 48175 48188https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/450/1900?format=asciidefaultJ/MNRAS/450/1900/starsCombined table from original tablesStarStar's identifiermeta.id;meta.maincharprimaryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNwNumber of equivalent widths for this starmeta.numberintnullable[Mg/H]Abundance [Mg/H] (Z=12) (G1)log(Sun)phys.abundfloat[Al/H]? Abundance [Al/H] (Z=13) (G1)log(Sun)phys.abundfloatnullable[Si/H]Abundance [Si/H] (Z=14) (G1)log(Sun)phys.abundfloat[Ca/H]Abundance [Ca/H] (Z=20) (G1)log(Sun)phys.abundfloat[ScI/H]Abundance [ScI/H] (Z=21.0) (G1)log(Sun)phys.abundfloat[ScII/H]Abundance [ScII/H] (Z=21.1) (G1)log(Sun)phys.abundfloat[TiI/H]Abundance [TiI/H] (Z=22.0) (G1)log(Sun)phys.abundfloat[TiII/H]Abundance [TiII/H] (Z=22.0) (G1)log(Sun)phys.abundfloat[V/H]Abundance [V/H] (Z=23) (G1)log(Sun)phys.abundfloat[CrI/H]Abundance [CrI/H] (Z=24.0) (G1)log(Sun)phys.abundfloat[Co/H]Abundance [Co/H] (Z=27) (G1)log(Sun)phys.abundfloat[Ni/H]Abundance [Ni/H] (Z=28) (G1)log(Sun)phys.abundfloatSimbadSimbad column added by the CDSphys.abundcharUlsrU velocity of the star relative to the LSR (1)km/sphys.veloc;pos.cartesian.xintnullableVlsrV velocity of the star relative to the LSR (1)km/sphys.veloc;pos.cartesian.yintnullableWlsrW velocity of the star relative to the LSR (1)km/sphys.veloc;pos.cartesian.zintnullablepD1[0/1] Probability of a star belonging to the thick disc according to B03 (2)stat.fit.goodnessfloatnullableptD1[0/1] Probability of a star belonging to the thin disc according to B03 (2)stat.fit.goodnessfloatnullablepH1[0/1] Probability of a star belonging to the halo according to B03 (2)stat.fit.goodnessfloatnullablepop1probable population where the star belongs according to B03 (thin, thick or trans)src.classcharpD2[0/1] Probability of a star belonging to the thick disc according to R03 (3)stat.fit.goodnessfloatnullableptD2[0/1] Probability of a star belonging to the thin disc according to R03 (3)stat.fit.goodnessfloatnullablepH2[0/1] Probability of a star belonging to the halo according to R03 (3)stat.fit.goodnessfloatnullablepop2probable population where the star belongs according to R03 (thin, thick or trans)src.classchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/MNRAS/450/1900/table2Abundances, rms, error, and number of lines for each star and elementrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar's identifiermeta.id;meta.maincharNwNumber of equivalent widths for this starmeta.numberintnullable[Na/H]? Abundance [Na/H] (Z=11) (G1) (1)log(Sun)phys.abundfloatnullablee_[Na/H]rms uncertainty of [Na/H]log(Sun)stat.error;phys.abundfloats_[Na/H]Total error of [Na/H]log(Sun)stat.error;phys.abundfloat[Na/H]cAbundance [Na/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[Na/H]Number of Na lines usedmeta.numberint[Mg/H]Abundance [Mg/H] (Z=12) (G1) (1)log(Sun)phys.abundfloate_[Mg/H]rms uncertainty of [Mg/H]log(Sun)stat.error;phys.abundfloats_[Mg/H]Total error of [Mg/H]log(Sun)stat.error;phys.abundfloat[Mg/H]cAbundance [Mg/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[Mg/H]Number of MgI lines usedmeta.numberint[Al/H]? Abundance [Al/H] (Z=13) (G1) (1)log(Sun)phys.abundfloatnullablee_[Al/H]? rms uncertainty of [Al/H]log(Sun)stat.error;phys.abundfloatnullables_[Al/H]Total error of [Al/H]log(Sun)stat.error;phys.abundfloat[Al/H]cAbundance [Al/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[Al/H]? Number of AlI lines usedmeta.numberintnullable[Si/H]Abundance [Si/H] (Z=14) (G1)log(Sun)phys.abundfloate_[Si/H]rms uncertainty of [Si/H]log(Sun)stat.error;phys.abundfloats_[Si/H]Total error of [Si/H]log(Sun)stat.error;phys.abundfloat[Si/H]cAbundance [Si/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[Si/H]Number of SiI lines usedmeta.numberint[Ca/H]Abundance [Ca/H] (Z=20) (G1)log(Sun)phys.abundfloate_[Ca/H]rms uncertainty of [Ca/H]log(Sun)stat.error;phys.abundfloats_[Ca/H]Total error of [Ca/H]log(Sun)stat.error;phys.abundfloato_[Ca/H]Number of CaI lines usedmeta.numberint[ScI/H]Abundance [ScI/H] (Z=21.0) (G1) (1)log(Sun)phys.abundfloate_[ScI/H]rms uncertainty of [ScI/H]log(Sun)stat.error;phys.abundfloats_[ScI/H]Total error of [ScI/H]log(Sun)stat.error;phys.abundfloat[ScI/H]cAbundance [ScI/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[ScI/H]Number of ScI lines usedmeta.numberint[ScII/H]Abundance [ScII/H] (Z=21.1) (G1)log(Sun)phys.abundfloate_[ScII/H]rms uncertainty of [ScII/H]log(Sun)stat.error;phys.abundfloats_[ScII/H]Total error of [ScII/H]log(Sun)stat.error;phys.abundfloat[ScII/H]cAbundance [ScII/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[ScII/H]Number of ScII lines usedmeta.numberint[TiI/H]Abundance [TiI/H] (Z=22.0) (G1)log(Sun)phys.abundfloate_[TiI/H]rms uncertainty of [TiI/H]log(Sun)stat.error;phys.abundfloats_[TiI/H]Total error of [TiI/H]log(Sun)stat.error;phys.abundfloato_[TiI/H]Number of TiI lines usedmeta.numberint[TiII/H]Abundance [TiII/H] (Z=22.1) (G1)log(Sun)phys.abundfloate_[TiII/H]rms uncertainty of [TiII/H]log(Sun)stat.error;phys.abundfloats_[TiII/H]Total error of [TiII/H]log(Sun)stat.error;phys.abundfloato_[TiII/H]Number of TiII lines usedmeta.numberint[V/H]Abundance [V/H] (Z=23) (G1)log(Sun)phys.abundfloate_[V/H]rms uncertainty of [V/H]log(Sun)stat.error;phys.abundfloats_[V/H]Total error of [V/H]log(Sun)stat.error;phys.abundfloat[V/H]cAbundance [V/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[V/H]Number of VI lines usedmeta.numberint[CrI/H]Abundance [CrI/H] (Z=24.0) (G1)log(Sun)phys.abundfloate_[CrI/H]rms uncertainty of [CrI/H]log(Sun)stat.error;phys.abundfloats_[CrI/H]Total error of [CrI/H]log(Sun)stat.error;phys.abundfloat[CrI/H]cAbundance [CrI/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[CrI/H]Number of CrI lines usedmeta.numberint[CrII/H]? Abundance [CrII/H] (Z=24.1) (G1) (1)log(Sun)phys.abundfloatnullablee_[CrII/H]? rms uncertainty of [CrII/H]log(Sun)stat.error;phys.abundfloatnullables_[CrII/H]? Total error of [CrII/H]log(Sun)stat.error;phys.abundfloatnullable[CrII/H]c? Abundance [CrII/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloatnullableo_[CrII/H]? Number of CrII lines usedmeta.numberintnullable[Mn/H]Abundance [Mn/H] (Z=25) (G1) (1)log(Sun)phys.abundfloate_[Mn/H]rms uncertainty of [Mn/H]log(Sun)stat.error;phys.abundfloats_[Mn/H]Total error of [Mn/H]log(Sun)stat.error;phys.abundfloato_[Mn/H]Number of MnI lines usedmeta.numberint[Co/H]Abundance [Co/H] (Z=27) (G1)log(Sun)phys.abundfloate_[Co/H]rms uncertainty of [Co/H]log(Sun)stat.error;phys.abundfloats_[Co/H]Total error of [Co/H]log(Sun)stat.error;phys.abundfloat[Co/H]cAbundance [Co/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[Co/H]Number of CoI lines usedmeta.numberint[Ni/H]Abundance [Ni/H] (Z=28) (G1)log(Sun)phys.abundfloate_[Ni/H]rms uncertainty of [Ni/H]log(Sun)stat.error;phys.abundfloats_[Ni/H]Total error of [Ni/H]log(Sun)stat.error;phys.abundfloat[Ni/H]cAbundance [Ni/H] after correction for effective temperature trend (2)log(Sun)phys.abundfloato_[Ni/H]Number of NiI lines usedmeta.numberintJ/MNRAS/450/1900/ewEquivalent widths of the spectral lines used to derive abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar's identifiermeta.id;meta.maincharlambdaCentral wavelength0.1nmem.wl.centralfloatEWEquivalent width of the line0.1pmspect.line.eqWidthfloatJ/MNRAS/450/1900/linelistAtomic parameters for lines selected in the paperrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElElement and ionization statephys.atmol.element;phys.atmol.ionizationcharlambda[4792/6773] Central wavelength0.1nmem.wl.centralfloatEPExcitation potentialeVphys.atmol.excitationfloatloggfOscilator strengthphys.atmol.collStrengthfloatDab[-3.9/10.8] Difference in abundances between dwarfs and giants relative to {sigma} (1)phys.abundfloat