J/A+A/582/A81ivo://CDS.VizieR/J/A+A/582/A81doi:10.26093/cds/vizier.35820081CDSJofre P.Heiter U.Soubiran C.Blanco-Cuaresma S.Masseron T.,Nordlander T.Chemin L.Worley C.C.Van Eck S.Hourihane A.Gilmore G.,Adibekyan V.Bergemann M.Cantat-Gaudin T.Delgado-Mena E.,Gonzalez Hernandez J.I.Guiglion G.Lardo C.de Laverny P.Lind K.,Magrini L.Mikolaitis S.Montes D.Pancino E.Recio-Blanco A.Sordo R.,Sousa S.Tabernero H.M.Vallenari A.2018-09-08T13:28:56Z2015-10-13T10:20:44ZCDS support team

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

cds-question@unistra.frchemical-abundancesIn the current era of large spectroscopic surveys of the Milky Way, reference stars for calibrating astrophysical parameters and chemical abundances are of paramount importance. We determine elemental abundances of Mg, Si, Ca, Sc, Ti, V, Cr, Mn, Co, and Ni for our predefined set of Gaia FGK benchmark stars. By analysing high-resolution spectra with a high signal-to-noise ratio taken from several archive datasets, we combined results of eight different methods to determine abundances on a line-by-line basis. We performed a detailed homogeneous analysis of the systematic uncertainties, such as differential versus absolute abundance analysis. We also assessed errors that are due to non-local thermal equilibrium and the stellar parameters in our final abundances.2015A&A...582A..81Jhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/582/A81CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIII/281 : Gaia FGK benchmark stars v2.1 (Jofre+, 2018)J/A+A/564/A133 : Gaia FGK benchmark stars: metallicity (Jofre+, 2014)J/A+A/566/A98 : The Gaia Benchmark Stars - Library (Blanco-Cuaresma+, 2014)J/A+A/592/A70 : Gaia FGK stars: low-metallicities candidates (Hawkins+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/582/A81https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/582/A81http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/582/A81https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/582/A81https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/582/A81http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/582/A81GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/582/A81/stars (List of studied stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/582/A81/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/582/A81/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/582/A81/stars?GETtext/xml+votable180.050000true243.9070833-8.36944440.0055555555555555566/15 2923 4376 4574 6219 8767 8845 12953 13301 17425 18907 22120 22300 23096 23540 24715 26302 26457 26552 26975 28664 30878 33281 35118 36035 36693 36697 41763 42081 42248 44542https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/582/A81?format=asciidefaultJ/A+A/582/A81/tablec31Procyon elemental abundance measurements for different methods for each lineElAtomic number of elementphys.atmol.elementintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec14epsilon eri elemental abundance measurements for different methods for each lineElAtomic number of elementphys.atmol.elementintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec33Sun elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec6alpha Cet elemental abundance measurements for different methods for each lineElAtomic number of elementphys.atmol.elementintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec7alpha Tau elemental abundance measurements for different methods for each lineElAtomic number of elementphys.atmol.elementintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec8Arcturus elemental abundance measurements for different methods for each linebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec9beta Ara elemental abundance measurements for different methods for each lineElAtomic number of elementphys.atmol.elementintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec10beta Gem elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec11beta Hyi elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec12beta Vir elemental abundance measurements for different methods for each lineispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec13delta Eri elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec15epsilon For elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec16epsilon Vir elemental abundance measurements for different methods for each lineElAtomic number of elementphys.atmol.elementintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec17eta Boo elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec18gamma Sge elemental abundance measurements for different methods for each lineepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec19Gmb 1830 elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec20HD 22879 elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec21HD49933 elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec22HD84937 elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec23HD107328 elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec25HD140283 elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec26HD220009 elemental abundance measurements for different methods for each lineElAtomic number of elementphys.atmol.elementintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec27ksi Hya elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec28mu Ara elemental abundance measurements for different methods for each lineElAtomic number of elementphys.atmol.elementintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec24HD122563 elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/starsList of studied starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000? Simbad right ascension (J2000)pos.eq.ra;meta.mainnullableDEJ2000? Simbad declination (J2000)pos.eq.dec;meta.mainnullableStarStar namemeta.id;meta.maincharFileNameName of the table with elemental abundancesmeta.id;phys.abund;meta.tablecharSimbadSimbad column added by the CDSmeta.ref.urlcharJ/A+A/582/A81/infolineLine information (table C36)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatIonIonisation stage of the linephys.atmol.ionStageintloggfOscillation strength of the linespect.line.intensityfloatEPExcitation potential of the lineeVphys.atmol.excitation;spect.linefloatGESflagQuality flag of Gaia-ESO line listmeta.code.qual;spect.linecharFG-dwarf[YN-] Golden flag for stars in group of FG-dwarfs (1)meta.codecharK-dwarf[YN-] Golden flag for stars in group of K-dwarfs (1)meta.codecharmetal-poor[YN-] Golden flag for stars in group of metal-poor stars (1)meta.codecharFGK-giant[YN-] Golden flag for stars in group of FGK-giants (1)meta.codecharM-giant[YN-] Golden flag for stars in group of M-giants (1)meta.codecharJ/A+A/582/A81/tablec118 Sco elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec261 Cyg A elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec361 Cyg B elemental abundance measurements for different methods for each linegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec4alpha Cen A elemental abundance measurements for different methods for each lineElAtomic number of elementphys.atmol.elementintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec5alpha Cen B elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec29mu Cas elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec30mu Leo elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec32psi Phe elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullableJ/A+A/582/A81/tablec34tau Cet elemental abundance measurements for different methods for each linerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElAtomic number of elementphys.atmol.elementintlambdaWavelength of line used in the abundance determination0.1nmem.wl;spect.linefloatlog(eps)? Abundance obtained for the line after combining methods (1)phys.abundfloatnullableNLTE? NLTE correction for that line (1)arith.factorfloatnullableEWpor? Equivalent width obtained by the Porto method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWepi? Equivalent width obtained by the EPINARBO method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWbol? Equivalent width obtained by the Bologna method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWucm? Equivalent width obtained by the UCM method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEWulb? Equivalent width obtained by the ULB method (1)0.1pmspect.line.eqWidth;meta.modelledfloatnullableispec? Abundance obtained by the iSpec method (1)phys.abundfloatnullablepor? Abundance obtained by the Porto method (1)phys.abundfloatnullablegau? Abundance obtained by the Gauguin method (1)phys.abundfloatnullableepi? Abundance obtained by the EPINARBO method (1)phys.abundfloatnullablebol? Abundance obtained by the Bologna method (1)phys.abundfloatnullablesyn? Abundance obtained by the synspec method (1)phys.abundfloatnullableucm? Abundance obtained by the UCM method (1)phys.abundfloatnullableulb? Abundance obtained by the ULB method (1)phys.abundfloatnullable