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<ri:Resource created="2005-08-20T16:53:17Z" 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>Abundances of 15 solar analogues</title><shortName>J/AZh/81/541</shortName><identifier>ivo://CDS.VizieR/J/AZh/81/541</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Galeev A.I.</name></creator><creator><name>Bikmaev I.F.</name></creator><creator><name>Musaev F.A.</name></creator><creator><name>Galazutdinov G.A.</name></creator><date role="Updated">2017-12-18T07:57:45Z</date><date role="Created">2005-08-20T16:53:17Z</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>g-stars</subject><subject>chemical-abundances</subject><description>The results of a spectroscopic analysis of 15 stars that are photometric analogues of the Sun are reported. The effective temperatures and surface gravities in the stellar atmospheres are derived from published photometric indices and the HIPPARCOS parallaxes. The abundances of 33 elements ranging from lithium to europium are analyzed based on high-dispersion spectra taken with the new Coude echelle spectrometer of the Terskol Observatory in the northern Caucasus. The main parameters of most of the stars agree with the data of an [Fe/H] catalog published in 2001. Our study of the chemical compositions of the sample stars indicates that photometric analogues of the Sun can be divided into three groups according to their elemental abundances: six stars have solar chemical composition, four have abundance excesses, and five have some abundance deficiencies. The sample contains two metal-deficient subgiants (HD 133002 and HD 225239).</description><source format="bibcode">2004AZh....81..541G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/81/541</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/393/225">J/A+A/393/225 : Starspot cycles of six young solar analogues (Messina+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/409/1017">J/A+A/409/1017 : Magnetic activity of 6 young solar stars. II (Messina+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/327/587">J/A+A/327/587 : Abundances of 9 solar-type stars (Tomkin+ 1997)</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/AZh/81/541</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/81/541</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/81/541</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AZh/81/541</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AZh/81/541</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AZh/81/541</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AZh/81/541/table2 (Photometric solar analogues)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AZh/81/541/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AZh/81/541/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AZh/81/541/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>243.905293</ra><dec>-8.369442</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1341 2476 5522 9492 9648 10225 12238 12890 13778 14411 14650 15174 16883 17944 18637 19796 20440 23515 25966 30579 30878 31478 32021 32585</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AZh/81/541?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AZh/81/541/table2</name><description>Photometric solar analogues</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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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>HD</name><description>HD number</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff</name><description>Effective Temperature</description><unit>K</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>Suface gravity</description><unit>cm.s**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>Metallicity [Fe/H] (logarithmic scale)</description><unit>Sun</unit><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AZh/81/541/abund</name><description>Elemental abundances (tables 6, 7 and 8)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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