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<ri:Resource created="2015-01-20T08:07:41Z" 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>Tc IV, Tc V and Tc VI oscillator strengths</title><shortName>J/A+A/574/A29</shortName><identifier>ivo://CDS.VizieR/J/A+A/574/A29</identifier><altIdentifier>doi:10.26093/cds/vizier.35740029</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Werner K.</name></creator><creator><name>Rauch T.</name></creator><creator><name>Kucas S.</name></creator><creator><name>Kruk J.W.</name></creator><date role="Updated">2015-06-21T09:31:38Z</date><date role="Created">2015-01-20T08:07:41Z</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>atomic-physics</subject><description>The discovery of technetium (Tc) in the atmospheres of red giants by Merrill (1952ApJ...116...21M) constituted convincing proof that s-process nucleosynthesis is indeed occurring in evolved stars. In principle, Tc should still be present in the atmospheres of hot post-AGB stars and (pre-) white dwarfs although, due to radioactive decay, it should be present in decreasing quantities along post-AGB evolution. The recent discovery of a large number of trans-iron group elements in hot white dwarfs with atomic numbers in the range A=30-56 (Zn to Ba) raises the prospect that Tc (A=43) may also be detected. However, this is currently not feasible because no atomic data exist for ionization stages beyond TcII. As an initial step, we calculated atomic energy levels and oscillator strengths of Tc IV-VI and used these data to compute non-local thermodynamic equilibrium (NLTE) model atmospheres to estimate at which minimum abundance level Tc could be detected. We show that Tc lines can be found in ultraviolet spectra of hot white dwarfs provided Tc is as abundant as other detected trans-Fe elements. We find that radiative levitation can keep Tc in large, easily detectable quantities in the atmosphere. A direct identification of Tc lines is still not feasible because wavelength positions cannot be computed with necessary precision. Laboratory measurements are necessary to overcome this problem. Our results suggest that such efforts are beneficial to the astrophysical community.</description><source format="bibcode">2015A&amp;A...574A..29W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/574/A29</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+A/546/A55">J/A+A/546/A55 : Ge V and Ge VI oscillator strengths (Rauch+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A41">J/A+A/564/A41 : ZnIV and ZnV oscillator strengths (Rauch+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/566/A10">J/A+A/566/A10 : Ba V, Ba VI, and Ba VII oscillator strengths (Rauch+, 2014)</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/574/A29</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/574/A29</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/574/A29</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/574/A29</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/574/A29</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/574/A29</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"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/574/A29/table1</name><description>Tc IV energy levels</description><column><name>Index</name><description>[1/4698] Level index</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>E</name><description>Level energy</description><unit>cm**-1</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>p</name><description>[o/e] Level parity (o for odd, e for even)</description><ucd>phys.atmol.parity;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>J</name><description>[0/12] Angular momentum quantum number J</description><ucd>phys.angMomentum</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>P1</name><description>[6/100] First percentage (1)</description><unit>%</unit><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Conf1</name><description>Configuration of the first percentage</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>term1</name><description>Term of the first percentage</description><ucd>phys.atmol.term</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>P2</name><description>[1/50]? 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