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<ri:Resource created="2014-01-09T07:48:06Z" 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>On the metallicity of open clusters. II.</title><shortName>J/A+A/561/A93</shortName><identifier>ivo://CDS.VizieR/J/A+A/561/A93</identifier><altIdentifier>doi:10.26093/cds/vizier.35610093</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Heiter U.</name></creator><creator><name>Soubiran C.</name></creator><creator><name>Netopil M.</name></creator><creator><name>Paunzen E.</name></creator><date role="Updated">2017-09-19T14:24:02Z</date><date role="Created">2014-01-09T07:48:06Z</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>open-star-clusters</subject><subject>metallicity</subject><subject>effective-temperature</subject><subject>spectroscopy</subject><subject>astronomical-object-identification</subject><description>The literature was searched for [Fe/H] estimates of individual member stars of open clusters (OCs) based on the analysis of high-resolution spectra. The lower limit for spectral resolving power (R={lambda}/{Delta}{lambda}) was set to 25000, and the lower limit for signal-to-noise ratio was set to 50. We searched the PASTEL database (2010A&amp;A...515A.111S, Cat. B/pastel) and the recent literature for such metallicity determinations in references posterior to 1990 and until June 2013. Only stars with an effective temperature lower than 7000K were included to avoid rapid rotators and chemical peculiarities. We eliminated confirmed non-members, spectroscopic binaries, and chemically peculiar stars and kept only stars with a high probability of membership. This resulted in a list of 571 stars in 86 OCs, with 830 metallicity determinations from 94 papers, which we call the starting sample.</description><source format="bibcode">2014A&amp;A...561A..93H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/561/A93</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/B/pastel">B/pastel : The PASTEL catalogue (Soubiran+, 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/561/A93</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/561/A93</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/561/A93</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/561/A93</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/561/A93</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/561/A93</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/A+A/561/A93/table1 (List of the full starting sample of cluster members described in Sect. 2.1.)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/561/A93/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/561/A93/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/561/A93/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>80.0994792</ra><dec>30.6227528</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/75 120 309 320 322 333-334 336-337 341-342 348-349 373 456 460-461 463 472 474-475 483 496 770 1024 1032 1042 1058 1075 1481 1486 1577 1769 1923 2395 2433 2436 3076 3091 3095 3103 3136-3138 3230 4078 4298 4696 4698-4699 4720-4721 6149 14175 14303 14573 14575 14752 15594-15595 15759 16447 16488-16490 20562 20761 20797 21531 21538-21539 21586 21647 21719 22111 22130 22216 22237 22239 22499 22804 22854 22871 22887 23017 23246 23335 23344 23454 23463 23479 23489 23497 23501 23503 23511 23513 23515 23518 23525-23527 23529 23533-23535 23537-23539 23542 23544-23545 23547-23548 23612 23633 23637 23639 23745 23761 23861 24057 24099 24104 24110 24121 24192 24194-24195 24206-24207 24209 24330 24344 24491 24522 28092-28093 28433 28437 28439 28480 28482-28483 28485-28486 28489-28490 28499 28711 29045 29047 29066 29269 29728 29730 30215 30438-30439 30444-30445 31788 31790 31812 33099 37230-37231 37240 37316 37318 37349-37351 37592 37787-37788 37790 37809 37867 37920 37933 37944 37971 38242 38248 39129 39131 39356 39775 39895 39901 40104 40106 40490 40696 41613 41834 42177 42210 42216 42274 42402 42464 43022 43034</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/561/A93?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/561/A93/table1</name><description>List of the full starting sample of cluster members described in Sect. 2.1.</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>Sample</name><description>[1/2] Sample identification (1)</description><ucd>meta.id;src.sample</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster identification</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>RAJ2000</name><description>? Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>DEJ2000</name><description>? Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column><column><name>Vmag</name><description>Magnitude (apparent) in V filter</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BibCode</name><description>Reference for metallicity (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>StarID</name><description>Star identification (3)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="29*">char</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></table><table><name>J/A+A/561/A93/table4</name><description>Weighted mean metallicity of OCs, computed for each reference giving atmospheric parameters based on high-resolution, high-S/N spectra</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>Seq</name><description>[1/86] Sequential number for open clusters</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster identification</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType><flag>primary</flag></column><column><name>B_Teff</name><description>Minimum value of the effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>b_Teff</name><description>Maximum value of the effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>B_logg</name><description>Minimum value of the surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b_logg</name><description>Maximum value of the surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>Mean iron abundance relative to the Sun</description><unit>log(Sun)</unit><ucd>phys.abund.Fe;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s_[Fe/H]</name><description>? 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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>Seq</name><description>[1/84] Sequential number for open clusters</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType><flag>primary</flag></column><column><name>[Fe/H]</name><description>Mean metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Z;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s_[Fe/H]</name><description>? 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