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<ri:Resource created="2004-04-10T16:35:57Z" status="active" updated="2025-06-13T15:25:00Z" 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>Oxygen abundances in the Galactic disk</title><shortName>J/A+A/415/155</shortName><identifier>ivo://CDS.VizieR/J/A+A/415/155</identifier><altIdentifier>doi:10.26093/cds/vizier.34150155</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bensby T.</name></creator><creator><name>Feltzing S.</name></creator><creator><name>Lundstrom I.</name></creator><date role="Updated">2018-01-04T08:21:45Z</date><date role="Created">2004-04-10T16:35:57Z</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>line-intensities</subject><description>Oxygen abundances for the 72 program stars. Column one gives the Hipparcos number, columns 2-6 the derived oxygen abundances for the different indicators relative to the photospheric oxygen abundance {epsilon}(O)_{sun}_=8.83). Columns 7-11 give the abundances relative to our solar abundances, i.e. [O/H]_{sun}_=0 for all indicators. Columns 12-14 give the abundances for the triplet that have been corrected for NLTE effects according the the prescription in Gratton et al. (1999, Cat. &lt;J/A+A/350/955&gt;), and normalized to the new NLTE corrected abundance for the Sun. Column 15 gives the NLTE correction terms from Gratton et al. (1999, Cat. &lt;J/A+A/350/955&gt;) (GCEG) that were applied to the abundances in columns 12-14. Column 15 gives the empirical NLTE correction we determined (Eq. 1 in article}. Columns 16-19 give the measured equivalent widths for the forbidden [OI] line at 636.3nm and the permitted oxygen triplet lines at 777nm.</description><source format="bibcode">2004A&amp;A...415..155B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/415/155</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/J/A+A/350/955">J/A+A/350/955 : Atmospheric parameters in metal-poor 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>HIP</name><description>Hipparcos number (0=Sun)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>A6300</name><description>? Abundance [O/H] from 6300 line</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>A6363</name><description>? Abundance [O/H] from 6363 line</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>A7772</name><description>? Abundance [O/H] from 7771.95 line</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>A7774</name><description>? 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NLTE-corrected and normalized abundance [O/H] from 7774.17 line</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>A7775nlte</name><description>? NLTE-corrected and normalized abundance [O/H] from 7775.39 line</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>nlteGCEG</name><description>? NLTE-correction from Gratton et al. (J/A+A/350/955)</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>nlteTW</name><description>Empirical NLTE-correction from Eq. 1 in article</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EW6363</name><description>? 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