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<ri:Resource created="2014-02-07T08:31:19Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Chemical abundances of solar neighbourhood dwarfs</title><shortName>J/A+A/562/A71</shortName><identifier>ivo://CDS.VizieR/J/A+A/562/A71</identifier><altIdentifier>doi:10.26093/cds/vizier.35620071</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bensby T.</name></creator><creator><name>Feltzing S.</name></creator><creator><name>Oey M.S.</name></creator><date role="Updated">2019-04-08T13:44:28Z</date><date role="Created">2014-02-07T08:31:19Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>chemical-abundances</subject><subject>spectroscopy</subject><subject>stellar-ages</subject><subject>dwarf-stars</subject><description>We present a detailed elemental abundance study of 714 F and G dwarf and subgiant stars in the Solar neighbourhood. The analysis is based on high-resolution spectra obtained with MIKE on the Magellan telescope, FEROS on the ESO 1.5m and 2.2m telescopes, HARPS on the ESO 3.6m telescope, UVES on the ESO Very Large Telescope, SOFIN and FIES on the Nordic Optical Telescope. Our data show that there is an old and alpha-enhanced disk population, and a younger and less alpha-enhanced disk population. While they overlap greatly in metallicity between -0.7&lt;[Fe/H]&lt;+0.1, they show a bimodal distribution in [alpha/Fe]. This bimodality becomes even clearer if stars where stellar parameters and abundances show larger uncertainties (Teff&lt;5400K) are discarded, showing that it is important to constrain the data set to a narrow range in the stellar parameters if small differences between stellar populations are to be revealed. In addition, we find that the alpha-enhanced population has orbital parameters placing the stellar birthplaces in the inner Galactic disk while the low-alpha stars mainly come from the outer Galactic disk, fully consistent with the recent claims of a short scale-length for the alpha-enhanced Galactic thick disk. We have also investigated the properties of the Hercules stream and the Arcturus moving group.</description><source format="bibcode">2014A&amp;A...562A..71B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/562/A71</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/118/895">J/AJ/118/895 : Milky way and stellar distributions (Tiede+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/377/911">J/A+A/377/911 : Solar neighborhood age-metallicity relation (Feltzing+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/325/1365">J/MNRAS/325/1365 : Solar neighborhood metallicity distribution (Haywood+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/30/173">J/PAZh/30/173 : Space velocities of solar neighborhood stars (Borkova+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/714/663">J/ApJ/714/663 : Stellar density map of the Milky Way (de Jong+, 2010)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/562/A71</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/562/A71</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Abundance ratio Ti/H normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ti/H</name><description>? Uncertainty on abundance ratio Ti/H</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>O/Ti</name><description>? Abundance ratio O/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_O/Ti</name><description>? Uncertainty on abundance ratio O/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Na/Ti</name><description>? Abundance ratio Na/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Na/Ti</name><description>? Uncertainty on abundance ratio Na/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mg/Ti</name><description>? Abundance ratio Mg/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Mg/Ti</name><description>? Uncertainty on abundance ratio Mg/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Al/Ti</name><description>? Abundance ratio Al/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Al/Ti</name><description>? Uncertainty on abundance ratio Al/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Si/Ti</name><description>? Abundance ratio Si/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Si/Ti</name><description>? Uncertainty on abundance ratio Si/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ca/Ti</name><description>? Abundance ratio Ca/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>TeffH</name><description>Teff when using Hipparcos parallax for logg</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Ca/Ti</name><description>? Uncertainty on abundance ratio Ca/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Cr/Ti</name><description>? Abundance ratio Cr/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Cr/Ti</name><description>? Uncertainty on abundance ratio Cr/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ni/Ti</name><description>? Abundance ratio Ni/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ni/Ti</name><description>? Uncertainty on abundance ratio Ni/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Fe/Ti</name><description>? Abundance ratio Fe/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Fe/Ti</name><description>? Uncertainty on abundance ratio Fe/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Zn/Ti</name><description>? Abundance ratio Zn/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Zn/Ti</name><description>? Uncertainty on abundance ratio Zn/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Y/Ti</name><description>? Abundance ratio Y/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Y/Ti</name><description>? Uncertainty on abundance ratio Y/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ba/Ti</name><description>? Abundance ratio Ba/Ti normalised to Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ba/Ti</name><description>? Uncertainty on abundance ratio Ba/Ti</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>nFe1</name><description>Number of lines per Fe1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nFe2</name><description>Number of lines per Fe2 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nO1</name><description>? Number of lines per O1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nNa1</name><description>? Number of lines per Na1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nMg1</name><description>? Number of lines per Mg1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nAl1</name><description>? Number of lines per Al1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nSi1</name><description>? Number of lines per Si1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nCa1</name><description>? Number of lines per Ca1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nTi1</name><description>? Number of lines per Ti1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nTi2</name><description>? Number of lines per Ti2 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nCr1</name><description>? Number of lines per Cr1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nCr2</name><description>? Number of lines per Cr2 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nNi1</name><description>? Number of lines per Ni1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nZn1</name><description>? Number of lines per Zn1 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nY2</name><description>? Number of lines per Y2 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nBa2</name><description>? Number of lines per Ba2 ion</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>sFe1</name><description>1-{sigma} line-to-line dispersion per Fe1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sFe2</name><description>1-{sigma} line-to-line dispersion per Fe2 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sO1</name><description>? 1-{sigma} line-to-line dispersion per O1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sNa1</name><description>? 1-{sigma} line-to-line dispersion per Na1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sMg1</name><description>? 1-{sigma} line-to-line dispersion per Mg1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sAl1</name><description>? 1-{sigma} line-to-line dispersion per Al1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sSi1</name><description>? 1-{sigma} line-to-line dispersion per Si1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sCa1</name><description>? 1-{sigma} line-to-line dispersion per Ca1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sTi1</name><description>? 1-{sigma} line-to-line dispersion per Ti1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sTi2</name><description>? 1-{sigma} line-to-line dispersion per Ti2 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sCr1</name><description>? 1-{sigma} line-to-line dispersion per Cr1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sCr2</name><description>? 1-{sigma} line-to-line dispersion per Cr2 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sNi1</name><description>? 1-{sigma} line-to-line dispersion per Ni1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sZn1</name><description>? 1-{sigma} line-to-line dispersion per Zn1 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sY2</name><description>? 1-{sigma} line-to-line dispersion per Y2 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sBa2</name><description>? 1-{sigma} line-to-line dispersion per Ba2 ion</description><ucd>stat.variance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>plx</name><description>Hipparcos parallax</description><unit>mas</unit><ucd>pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_plx</name><description>Uncertainty in plx</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>Heliocentric distance</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GLON</name><description>Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ulsr</name><description>U velocity relative to LSR</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Vlsr</name><description>V velocity relative to LSR</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Wlsr</name><description>W velocity relative to LSR</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Rmin</name><description>Perigalactic distance of stellar orbit</description><unit>kpc</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rmax</name><description>Apogalactic distance of stellar orbit</description><unit>kpc</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zmax</name><description>Maximum distance from galactic plane</description><unit>kpc</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e</name><description>[0/1] Eccentricity of stellar orbit</description><ucd>src.orbital.eccentricity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lz</name><description>Orbital angular momentum</description><unit>kpc.km/s</unit><ucd>phys.angMomentum</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Elsr</name><description>Orbital energy normalised to LSR</description><ucd>src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>td/d</name><description>Thick disk-to-thin disk probability ratio</description><ucd>stat.likelihood</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>td/h</name><description>Thick disk-to-halo probability ratio</description><ucd>stat.likelihood</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>her/td</name><description>Hercules-to-thick disk probability ratio</description><ucd>stat.likelihood</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>her/d</name><description>Hercules-to-thin disk probability ratio</description><ucd>stat.likelihood</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>TeffI</name><description>Uncorrected ion.bal. temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>loggI</name><description>Uncorrected ion.bal. gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggH</name><description>logg when using Hipparcos parallax</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fe1H</name><description>Absolute FeI abundance when using Hipparcos parallax</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fe2H</name><description>Absolute FeII abundance when using Hipparcos parallax</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/A+A/562/A71/tablec2</name><description>Atomic line data, solar equivalent widths, and solar abundances</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>El</name><description>Element</description><ucd>phys.atmol.element</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Ion</name><description>Ion (1=neutral, 2=ionised)</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambda</name><description>Line wavelength</description><unit>0.1nm</unit><ucd>em.wl;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>loggf</name><description>Oscillator strength (1)</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LEP</name><description>Lower excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EW</name><description>Line equivalent width</description><unit>pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Abun</name><description>Absolute abundance 12+log(N/H) (2)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/562/A71/tablec1</name><description>Stars rejected from analysis</description><column><name>HIP</name><description>Hipparcos number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>Rej</name><description>[1/2] Reason for rejection (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>