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<ri:Resource created="2010-05-31T20:26:58Z" 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>N K-shell photoabsorption</title><shortName>J/ApJS/185/477</shortName><identifier>ivo://CDS.VizieR/J/ApJS/185/477</identifier><altIdentifier>doi:10.26093/cds/vizier.21850477</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Garcia J.</name></creator><creator><name>Kallman T.R.</name></creator><creator><name>Witthoeft M.</name></creator><creator><name>Behar E.</name></creator><creator><name>Mendoza C.</name></creator><creator><name>Palmeri P.,Quinet P.</name></creator><creator><name>Bautista M.A.</name></creator><creator><name>Klapisch M.</name></creator><date role="Updated">2010-06-04T16:02:17Z</date><date role="Created">2010-05-31T20:26:58Z</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>Reliable atomic data have been computed for the spectral modeling of the nitrogen K lines, which may lead to useful astrophysical diagnostics. Data sets comprise valence and K-vacancy level energies, wavelengths, Einstein A-coefficients, radiative and Auger widths, and K-edge photoionization cross sections. An important issue is the lack of measurements that are usually employed to fine-tune calculations so as to attain spectroscopic accuracy. In order to estimate data quality, several atomic structure codes are used and extensive comparisons with previous theoretical data have been carried out. In the calculation of K photoabsorption with the Breit-Pauli R-matrix method, both radiation and Auger dampings, which cause the smearing of the K edge, are taken into account. This work is part of a wider project to compute atomic data in the X-ray regime to be included in the database of the popular xstar modeling code.</description><source format="bibcode">2009ApJS..185..477G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/185/477</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/410/359">J/A+A/410/359 : Radiative and Auger decay for Fe II-Fe IX (Palmeri+, 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/ApJS/185/477</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/185/477</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/185/477</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/185/477</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/185/477</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/185/477</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/ApJS/185/477/table10</name><description>Valence and Auger levels for nitrogen ions</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>N</name><description>[1/7] Ion electron occupancy</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>i</name><description>[1/50] Level index</description><ucd>meta.code;spect.index;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>2S+1</name><description>[1/6] Spin multiplicity</description><ucd>phys.atmol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>L</name><description>[0/2] Total orbital angular momentum quantum number</description><ucd>phys.atmol.qn</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>2J</name><description>[0/7] The 2*(Total angular momentum quantum number)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Config</name><description>Electron configuration assignment</description><ucd>phys.atmol.configuration</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>Energy</name><description>Level energy</description><unit>eV</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ar</name><description>Level radiative width</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Aa</name><description>Level Auger width</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/ApJS/185/477/table11</name><description>Radiative K-transition data nitrogen ions</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>N</name><description>[1/7] Ion electron occupancy</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>j</name><description>[3/50] Upper level index</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>i</name><description>[1/20] Lower level index</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambda</name><description>Transition wavelength</description><unit>0.1nm</unit><ucd>em.wl;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Aji</name><description>Transition probability</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>gf</name><description>Weighted oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>