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<ri:Resource created="2023-02-24T08:49:54Z" 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>Chemical abundances in open cluster Stock 2</title><shortName>J/AJ/164/255</shortName><identifier>ivo://CDS.VizieR/J/AJ/164/255</identifier><altIdentifier>doi:10.26093/cds/vizier.51640255</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Casamiquela L.</name></creator><creator><name>Gebran M.</name></creator><creator><name>Agueros M.A.</name></creator><creator><name>Bouy H.</name></creator><creator><name>Soubiran C.</name></creator><date role="Updated">2023-05-26T08:53:23Z</date><date role="Created">2023-02-24T08:49:54Z</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>a-stars</subject><subject>chemical-abundances</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><subject>effective-temperature</subject><description>The recently rediscovered open cluster Stock2, located roughly 375pc away and about 400Myr old, has the potential to be an exciting new testbed for our understanding of stellar evolution. We present results from a spectroscopic campaign to characterize stars near the cluster's main-sequence turnoff; our goal is to identify candidate chemically peculiar stars among the cluster's A-stars. We obtained echelle spectra for 64 cluster members with ESPaDOnS on the 3.6m Canada-France-Hawaii Telescope, Maunakea Observatory, USA, and for six stars with SOPHIE on the 1.93m telescope at the Observatoire de Haute-Provence, France. We complemented these new observations with those of 13 high-mass cluster members from the HARPS-N archive; our overall sample is of 71 stars. We derived the fundamental parameters (Teff, logg, [M/H]) as well as v_e_sini for our sample using the sliced inverse regression technique, and then used iSpec to derive individual abundances of 12 chemical species. With these abundance determinations, we identified nine A-stars with anomalous levels of Sc, Ca, and other metallic lines. Follow-up observations of these Am candidates with a known age can transform them into benchmarks for evolutionary models that include atomic diffusion and help build a better understanding of the complex interactions between macroscopic and microscopic processes in stellar interiors.</description><source format="bibcode">2022AJ....164..255C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/164/255</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/475/1053">J/A+A/475/1053 : Magnetic fields in Ap/Bp stars (Auriere+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/523/A91">J/A+A/523/A91 : CoRoT/Exoplanet fields with MATISSE (Gazzano+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/523/A71">J/A+A/523/A71 : A and F stars abundances in the Hyades (Gebran+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/573/A67">J/A+A/573/A67 : Fundamental stellar parameters from PolarBase (Paletou+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/589/A83">J/A+A/589/A83 : PCA-based inversion of stellar parameters (Gebran+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/616/A10">J/A+A/616/A10 : 46 open clusters GaiaDR2 HRdiagrams (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/879/100">J/ApJ/879/100 : K2 rotation periods Hyades &amp; Praesepe members (Douglas+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/485/3623">J/MNRAS/485/3623 : Red giants abundance analysis open clusters (Reddy+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/640/A1">J/A+A/640/A1 : Portrait Galactic disc (Cantat-Gaudin+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/635/A8">J/A+A/635/A8 : Differential abundances of open clusters (Casamiquela+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/645/A106">J/A+A/645/A106 : Atomic data for the Gaia-ESO Survey (Heiter+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A147">J/A+A/661/A147 : Galac. interstellar dust Gaia-2MASS 3D maps (Lallement+, 2022)</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/AJ/164/255</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/164/255</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/164/255</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/164/255</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/164/255</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/164/255</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/AJ/164/255/table2 (Atmospheric parameters and abundances of the analyzed spectra)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/164/255/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/164/255/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/164/255/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>37.3398719</ra><dec>57.0898853</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/815 901 6/3254 3256 3259 3306 3589 3600-3601 3603</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/164/255?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/164/255/table2</name><description>Atmospheric parameters and abundances of the analyzed spectra</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Uncertainty in [Cr/H]</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Si/H]</name><description>[0/1.04]? iSpec Si abundance relative to the Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Si/H]</name><description>[0.01/0.4]? Uncertainty in [Si/H]</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[O/H]</name><description>[-0.68/1.79]? iSpec O abundance relative to the Sun</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[O/H]</name><description>[0.1/0.7]? 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