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<ri:Resource created="2009-09-27T15:16:02Z" 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>Stark broadening of He447.1nm line</title><shortName>J/A+A/503/293</shortName><identifier>ivo://CDS.VizieR/J/A+A/503/293</identifier><altIdentifier>doi:10.26093/cds/vizier.35030293</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gigosos M.A.</name></creator><creator><name>Gonzalez M.A.</name></creator><date role="Updated">2009-09-27T15:24:53Z</date><date role="Created">2009-09-27T15:16:02Z</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>Stark broadening of the 447.1nm line of neutral helium in a weakly coupled plasma has been studied. This spectral line has a very close forbidden component. This means it is very sensitive to the plasma electron density, which is similar to hydrogen lines, for which the Stark effect is linear. The aim of this work is to supply information to be used in the spectroscopic diagnostics of plasmas.</description><source format="bibcode">2009A&amp;A...503..293G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/503/293</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/VI/98">VI/98 : Stark broadening of H lines (Stehle+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/376/1113">J/A+A/376/1113 : Line ratios for helium-like ions (Porquet+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/170/251">J/ApJS/170/251 : Multiplet table for neutral helium (Drake+, 2007)</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/503/293</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/503/293</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/503/293</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/503/293</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/503/293</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/503/293</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/503/293/tables</name><description>Helium I 447.1 nm Stark profiles (tables 2-11 of the paper)</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>logNe</name><description>Electron density (1)</description><unit>log(m**-3)</unit><ucd>phys.density;phys.electron</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dlambda</name><description>Wavelength detuning from the unperturbed wavelength</description><unit>nm</unit><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>IDL0.8/5</name><description>? Stark profile for mu=0.8 and Te=5000K (2)</description><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>IDL0.8/10</name><description>? Stark profile for mu=0.8 and Te=10000K (2)</description><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>IDL0.8/20</name><description>Stark profile for mu=0.8 and Te=20000K (2)</description><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>IDL0.8/40</name><description>Stark profile for mu=0.8 and Te=40000K (2)</description><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>IDL2/5</name><description>? Stark profile for mu=2 and Te=5000K (2)</description><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>IDL2/10</name><description>? 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