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<ri:Resource created="2008-11-16T16:15:41Z" 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>Ni XXV energy levels and radiative rates</title><shortName>J/A+A/488/1155</shortName><identifier>ivo://CDS.VizieR/J/A+A/488/1155</identifier><altIdentifier>doi:10.26093/cds/vizier.34881155</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Duan B.</name></creator><creator><name>Bari M.A.</name></creator><creator><name>Zhong J.Y.</name></creator><creator><name>Yan J.</name></creator><creator><name>Li M.Y.</name></creator><creator><name>Zhang J.</name></creator><date role="Updated">2017-06-22T14:29:16Z</date><date role="Created">2008-11-16T16:15:41Z</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>We report calculations of energy levels and radiative rates for 1300 fine-structure levels generated from 189 configurations of Be-like Nickel. The General Purpose Relativistic Atomic Structure Program (GRASP2), developed by the I.P. Grant group in 1989 and partly improved by our group, is adopted in the calculations of energy levels and radiative rates. Our calculations are compared with those of other numerical methods and experiments so that their accuracy can be assessed. Additionally, the wavelengths, oscillator strengths, and radiative rates (for a given radiative rate and level structure, it is then easy to derive the line strength) a re reported for all electric dipole (E1), electric quadrupole (E2), magnetic dipole (M1) and magnetic quadrupole (M2) transitions among these levels. Finally, the lifetimes of all excited levels are reported.</description><source format="bibcode">2008A&amp;A...488.1155D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/488/1155</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/460/959">J/A+A/460/959 : NiXIX radiative and excitation rates (Aggarwal+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/475/393">J/A+A/475/393 : NiXI radiative and excitation rates (Aggarwal+, 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/488/1155</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/488/1155</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/488/1155</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/488/1155</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/488/1155</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/488/1155</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/488/1155/table1</name><description>The level energies of NiXXV ion</description><column><name>Index</name><description>Index</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><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>Conf</name><description>Configuration</description><ucd>phys.atmol.configuration;instr.setup</ucd></column><column><name>Term</name><description>^2S+1^L_J_ term (1)</description><ucd>phys.atmol.qn</ucd></column><column><name>Expt</name><description>? Expected energy</description><unit>Ry</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>CIV3</name><description>? Energy from CIV3 code</description><unit>Ry</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FAC</name><description>Energy from FAC code (2)</description><unit>Ry</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>GRASP2</name><description>Energy from GRASP code</description><unit>Ry</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>tau</name><description>? Lifetime</description><unit>s</unit><ucd>time.lifetime;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>J/A+A/488/1155/trans</name><description>Transition wavelength, oscillator strengths and radiative rates for transitions in NiXXV</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>Tr</name><description>Simbad column added by the CDS</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>i</name><description>Lower level index</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>j</name><description>Upper level index</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambdaji</name><description>Line wavelength</description><unit>0.1nm</unit><ucd>em.wl;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>gifij</name><description>Oscillator strength value (g_i_f_ij_)</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Aji</name><description>Radiative rate</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>