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<ri:Resource created="2003-01-04T09:00:09Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>{gamma} Ser &amp; 101 Her elemental abundances</title><shortName>J/A+A/394/187</shortName><identifier>ivo://CDS.VizieR/J/A+A/394/187</identifier><altIdentifier>doi:10.26093/cds/vizier.33940187</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Caliskan H.</name></creator><creator><name>Adelman S.J.</name></creator><creator><name>Cay M.T.</name></creator><creator><name>Gulliver A.F.</name></creator><creator><name>Tektunali H.G.</name></creator><creator><name>Teker A.</name></creator><date role="Updated">2003-01-04T08:01:59Z</date><date role="Created">2003-01-04T09:00:09Z</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>chemically-peculiar-stars</subject><description>Elemental abundances analysis of the superficially normal stars {gamma} Ser (F6 V) and 101 Herculis (A7 V) consistent with previous studies of this series using photographic region spectrograms obtained with Reticon and CCD detectors produced derived values that are generally solar except for Al which is very underabundant and the rare earths which do not have the solar pattern. Similar discrepancies from solar values are seen in other superficially normal stars of this series with similar temperatures. Our results for {gamma} Ser are in acceptable agreement with other recent studies based on different techniques and spectral regions.</description><source format="bibcode">2002A&amp;A...394..187C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/394/187</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/107/353">J/A+AS/107/353 : CP stars (Lopez-Garcia+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/125/219">J/A+AS/125/219 : mu Lep, 7 Sex, HR 4817 &amp; 28 Her abundances (Adelman+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/129/563">J/A+AS/129/563 : Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/137/227">J/A+AS/137/227 : HD 133029 &amp; HD 192913 abundances (Lopez-Garcia+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/367/597">J/A+A/367/597 : ups Her, phi Her &amp; HR 7018 abundances (Adelman+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/367/859">J/A+A/367/859 : {alpha} Scl and HD 170973 abundances (Lopez-Garcia+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/371/1078">J/A+A/371/1078 : alpha Dra, tau Her, gamma Lyr, HR 7926 (Adelman+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/316/514">J/MNRAS/316/514 : 28 And &amp; 99 Her elemental abundances (Adelman+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/406/975">J/A+A/406/975 : theta And, eps Del, eps Aqr, iota And (Kocer+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/406/987">J/A+A/406/987 : xi Oct, alpha Sex, 68 Tau elemental abund. (Pintado+, 2003)</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/394/187</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/394/187</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/394/187</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/394/187</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/394/187</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/394/187</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/394/187/table3a</name><description>Elemental abundances</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>Ion</name><description>Ion</description><ucd>phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>No</name><description>Multiplet number from Moore (1945) if first line of multiplet, if not from Moore an initial indicating the paper (1)</description><ucd>phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Lambda</name><description>Laboratory wavelength (air)</description><unit>0.1nm</unit><ucd>em.wl;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(gf)</name><description>Oscillator strength</description><ucd>phys.atmol.wOscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_log(gf)</name><description>Reference to oscillator strength (2)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>EW1</name><description>? Equivalent width for {gamma} Ser</description><unit>pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(N/Ntot)1</name><description>? Elemental abundance for {gamma} Ser (3)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EW2</name><description>? Equivalent width for 101 Her</description><unit>pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(N/Ntot)2</name><description>? Elemental abundance for 101 Her (3)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/394/187/table3b</name><description>Relative abundances</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>Ion</name><description>Ion</description><ucd>phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType><flag>primary</flag></column><column><name>El</name><description>Element</description><ucd>phys.atmol.element</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>log(El/Ntot)1</name><description>? Elemental abundance for {gamma} Ser (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log(El/Ntot)1</name><description>? rms uncertainty on log(El/Ntot)1</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(El/Ntot)2</name><description>? Elemental abundance for 101 Her (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log(El/Ntot)2</name><description>? rms uncertainty on log(El/Ntot)2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/394/187/table4</name><description>Comparison of derived and solar abundances</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>Ion</name><description>Ion</description><ucd>phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType><flag>primary</flag></column><column><name>logN/H1</name><description>? Elemental abundance for 99 Her (1)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logN/H2</name><description>? Elemental abundance for {gamma} Ser (1)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logN/H2</name><description>? rms uncertainty on logN/H2</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_logN/H1</name><description>Number of lines used to derive logN/H1 and logN/H2</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logN/H3</name><description>? Elemental abundance for 28 And (1)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logN/H4</name><description>? Elemental abundance for 101 Her (1)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logN/H4</name><description>? rms uncertainty on logN/H4</description><unit>log(Sun)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_logN/H3</name><description>? 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