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<ri:Resource created="2016-10-10T08:23:45Z" 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>APOGEE/Kepler sample stars abundances</title><shortName>J/A+A/594/A43</shortName><identifier>ivo://CDS.VizieR/J/A+A/594/A43</identifier><altIdentifier>doi:10.26093/cds/vizier.35940043</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hawkins K.</name></creator><creator><name>Masseron T.</name></creator><creator><name>Jofre P.</name></creator><creator><name>Gilmore G.</name></creator><creator><name>Elsworth Y.</name></creator><creator><name>Hekker S.</name></creator><date role="Updated">2018-05-02T08:34:10Z</date><date role="Created">2016-10-10T08:23:45Z</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>surveys</subject><subject>chemical-abundances</subject><subject>spectroscopy</subject><description>The APOGEE survey has obtained high-resolution infrared spectra of more than 100,000 stars. Deriving chemical abundances patterns of these stars is paramount to piecing together the structure of the MilkyWay. While the derived chemical abundances have been shown to be precise for most stars, some calibration problems have been reported, in particular for more metal-poor stars. In this paper, we aim to (1) re-determine the chemical abundances of the APOGEE+Kepler stellar sample (APOKASC) with an independent procedure, line list and line selection, and high-quality surface gravity information from asteroseismology, and (2) extend the abundance catalogue by including abundances that are not currently reported in the most recent APOGEE release (DR12). We fixed the Teff and logg to those determined using spectrophotometric and asteroseismic techniques, respectively. We made use of the Brussels Automatic Stellar Parameter (BACCHUS) code to derive the metallicity and broadening parameters for the APOKASC sample. In addition, we derived differential abundances with respect to Arcturus.</description><source format="bibcode">2016A&amp;A...594A..43H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/594/A43</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/133">V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/133">J/AJ/146/133 : SDSS-III APOGEE DR10 stellar parameters (Meszaros+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/156">J/AJ/146/156 : APOGEE M-dwarf survey. I. Velocities (Deshpande+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/153">J/AJ/149/153 : Abundances of red giants in 10 GC (Meszaros+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/125">J/ApJ/794/125 : IN-SYNC. I. APOGEE stellar parameters (Cottaar+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/445/2758">J/MNRAS/445/2758 : KIC giants Bayesian distances &amp; extinction (Rodrigues+ 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/148/24">J/AJ/148/24 : Extinction maps in the bulge from APOGEE (Schultheis+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/221/24">J/ApJS/221/24 : SDSS-III APOGEE H-band spectral line lists (Shetrone+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/7">J/AJ/149/7 : SDSS-III/APOGEE. I. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>All</name><description>Display all data for this source</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Name</name><description>2MASS name (2MHHMMSSss+DDMMSSs)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>Cluster</name><description>Cluster name</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Hmag</name><description>H-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>? Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>logg</name><description>? Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]</name><description>? Metallicity [Fe/H]</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Fe/H]</name><description>? rms uncertainty on [Fe/H]</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Conv</name><description>? Convolution parameter</description><unit>km/s</unit><ucd>spect.resolution</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Conv</name><description>? rms uncertainty on Conv</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>vmic</name><description>? Microtrubulent velocity</description><unit>km/s</unit><ucd>phys.veloc.microTurb</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_vmic</name><description>? rms uncertainty on vmic</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[C/H]</name><description>? [C/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[C/H]</name><description>? Dispersion on [C/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[N/H]</name><description>? [N/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[N/H]</name><description>? Dispersion on [N/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[O/H]</name><description>? [O/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[O/H]</name><description>? Dispersion on [O/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Na/H]</name><description>? [Na/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Na/H]</name><description>? Dispersion on [Na/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Mg/H]</name><description>? [Mg/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Mg/H]</name><description>? Dispersion on Mg/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Al/H]</name><description>? [Al/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Al/H]</name><description>? Dispersion on [Al/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Si/H]</name><description>? [Si/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Si/H]</name><description>? Dispersion on [Si/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[P/H]</name><description>? [P/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[P/H]</name><description>? Dispersion on [P/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[S/H]</name><description>? [S/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[S/H]</name><description>? Dispersion on [S/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[K/H]</name><description>? [K/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[K/H]</name><description>? Dispersion on [K/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ca/H]</name><description>? [Ca/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Ca/H]</name><description>? Dispersion on [Ca/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ti/H]</name><description>? [Ti/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Ti/H]</name><description>? Dispersion on [Ti/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[V/H]</name><description>? [V/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[V/H]</name><description>? Dispersion on [V/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Cr/H]</name><description>? [Cr/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Cr/H]</name><description>? Dispersion on [Cr/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Mn/H]</name><description>? [Mn/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Mn/H]</name><description>? Dispersion on [Mn/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Co/H]</name><description>? [Co/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Co/H]</name><description>? Dispersion on [Co/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ni/H]</name><description>? [Ni/H] abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Ni/H]</name><description>? Dispersion on [Ni/H]</description><ucd>instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></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>Position from name (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from name (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>