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<ri:Resource created="2013-01-16T09:19:14Z" 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>Carbon and oxygen abundances in FGK stars</title><shortName>J/ApJ/735/41</shortName><identifier>ivo://CDS.VizieR/J/ApJ/735/41</identifier><altIdentifier>doi:10.26093/cds/vizier.17350041</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Petigura E.A.</name></creator><creator><name>Marcy G.W.</name></creator><date role="Updated">2017-11-29T11:49:08Z</date><date role="Created">2013-01-16T09:19:14Z</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>late-type-stars</subject><subject>spectroscopy</subject><description>We present carbon and oxygen abundances for 941 FGK stars -the largest such catalog to date. We find that planet-bearing systems are enriched in these elements. We self-consistently measure N_C_/N_O_, which is thought to play a key role in planet formation. We identify 46 stars with N_C_/N_O_&gt;=1.00 as potential hosts of carbon-dominated exoplanets. We measure a downward trend in [O/Fe] versus [Fe/H] and find distinct trends in the thin and thick disks, supporting the work of Bensby et al. Finally, we measure sub-solar N_C_/N_O_=0.40^+0.11^_-0.07_, for WASP-12, a surprising result as this star is host to a transiting hot Jupiter whose dayside atmosphere was recently reported to have N_C_/N_O_&gt;=1 by Madhusudhan et al. Our measurements are based on 15,000 high signal-to-noise spectra taken with the Keck 1 telescope as part of the California Planet Search. We derive abundances from the [OI] and CI absorption lines at {lambda}=6300 and 6587{AA} using the SME spectral synthesizer.</description><source format="bibcode">2011ApJ...735...41P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/735/41</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/A+A/547/A106">J/A+A/547/A106 : Li abundances in the FGK dwarfs (Mishenina+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A141">J/A+A/533/A141 : Stellar parameters for 582 HARPS FGK stars (Sousa+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A71">J/A+A/526/A71 : C abundances in G and K nearby stars (Da Silva+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/465/271">J/A+A/465/271 : Oxygen abundances in nearby stars (Ramirez+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/168/297">J/ApJS/168/297 : Stellar parameters of nearby cool stars (Takeda+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/1063">J/AJ/129/1063 : Abundances of stars within 15pc of the Sun (Luck+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/57/65">J/PASJ/57/65 : CNO abundances of solar-type stars (Takeda+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/159/141">J/ApJS/159/141 : Spectroscopic properties of cool stars. 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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>Name</name><description>Source name or HD number (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Vmag</name><description>[-26.7/11.7] HIP catalog Johnson V band magnitude (2)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[0/127]? HIP distance (2)</description><unit>pc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Teff</name><description>[4707/6441] Effective temperature (3)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>log(g)</name><description>[2.7/5.0] Log of the surface gravity (3)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pop</name><description>Membership from Peek 2009PhDT.......205P: dn=thin disk; dk=thick disk; h=halo</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Host</name><description>[yes/no ] Does star host a planet?</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>[M/H]</name><description>(All elements heavier than He)/H abundance (3)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ni/H]</name><description>[-2/0.69] The Ni/H abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NO</name><description>[0/421] Number of oxygen lines fit for each star</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[O/H]</name><description>[-0.91/0.43]? The O/H abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[O/H]</name><description>? Lower limit uncertainty in [O/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_[O/H]</name><description>? Upper limit uncertainty in [O/H]</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NC</name><description>[0/294] Number of carbon lines fit for each star</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[C/H]</name><description>[-0.52/0.52]? The C/H abundance (5)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[C/H]</name><description>? Lower limit uncertainty in [C/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_[C/H]</name><description>? Upper limit uncertainty in [C/H]</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>C/O</name><description>[0.24/1.55]? The C/O abundance (5)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_C/O</name><description>? Lower limit uncertainty in C/O</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_C/O</name><description>? 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