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<ri:Resource created="2019-01-25T13:09:03Z" 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>Spectroscopic accuracy for B-like ions with Z=24-30</title><shortName>J/ApJS/239/3</shortName><identifier>ivo://CDS.VizieR/J/ApJS/239/3</identifier><altIdentifier>doi:10.26093/cds/vizier.22390003</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Si R.</name></creator><creator><name>Zhang C.Y.</name></creator><creator><name>Cheng Z.Y.</name></creator><creator><name>Wang K.</name></creator><creator><name>Jonsson P.</name></creator><creator><name>Yao K.</name></creator><creator><name>Gu M.F.,Chen C.Y.</name></creator><date role="Updated">2022-05-05T11:38:55Z</date><date role="Created">2019-01-25T13:09:03Z</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 spectroscopic accuracy for 513 states in the B-like ions with Z=24-30. The energy levels and transition rates are calculated using the second-order many-body perturbation theory, while multiconfiguration Dirac-Hartree-Fock calculations are performed to support the former results. The present two sets of results agree excellently with each other, and can be used as benchmarks in the future. The electron-impact excitation (EIE) collision strengths are calculated based on independent processes and isolated resonances approximation using the distorted wave method. Based on the present atomic data, the spectral lines of these ions are simulated using a collisional radiative model. The amount of energy, transition data, and EIE collision strengths of high accuracy are significantly increased for several B-like ions of astrophysical interest, where experimental data are still very scarce. The results can be used in line identification, plasma modeling, and diagnostics of astrophysical plasmas.</description><source format="bibcode">2018ApJS..239....3S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/239/3</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/ApJS/156/105">J/ApJS/156/105 : Transitions in L-shell ions of Fe and Ni (Gu+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/455/1157">J/A+A/455/1157 : Boron-like Fe XXII transition probabilities (Jonauskas+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/547/A87">J/A+A/547/A87 : B-like iso-electronic sequence (Liang+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/559/A100">J/A+A/559/A100 : Boron isoelectronic sequence data (Jonsson+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/215/26">J/ApJS/215/26 : Energy levels &amp; transition rates of C-like ions (Wang+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/583/A82">J/A+A/583/A82 : Electron-impact excitation for Hydrogen-like ions (Li+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/16">J/ApJS/218/16 : Energy levels &amp; transition rates of Be-like ions (Wang+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/592/A141">J/A+A/592/A141 : Helium-like ions with Z=10-36 transition rates (Si+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/227/16">J/ApJS/227/16 : Energy levels &amp; transition rates for F-like ions (Si+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/226/14">J/ApJS/226/14 : MBPT calc. for Ne-like ions (CrXV-KrXXVII) (Wang+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/223/3">J/ApJS/223/3 : Energies &amp; radiative transition ArXII-ZnXXIV (Wang+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/600/A85">J/A+A/600/A85 : He-like ions (Z=20-42) collision strengths (Si+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/229/37">J/ApJS/229/37 : Energy levels &amp; transition rates of O-like ions (Wang+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/234/40">J/ApJS/234/40 : Be-like ions from BII to NeVII transition data (Wang+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/27">J/ApJS/235/27 : Energy levels &amp; transition rates for P-like ions (Wang+, 2018)</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/239/3</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/239/3</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/239/3</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/239/3</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/239/3</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/239/3</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/239/3/table1</name><description>*Energy levels relative to the ground state and lifetimes from the present MBPT &amp; MCDHF calculations</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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