J/ApJS/238/34ivo://CDS.VizieR/J/ApJS/238/34doi:10.26093/cds/vizier.22380034CDSSantana J.A.Lopez-Dauphin N.A.Morales Butler E.J.Beiersdorfer P.2019-02-27T06:08:55Z2019-01-24T15:00:18ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fratomic-physicsCalculated level energies for valence and K-vacancy states are provided for the ion series SVII-SXIV and ArIX-ArXVI. The calculations were performed with the relativistic Multi-Reference Moller-Plesset Perturbation Theory method (MR-MP). The data set includes all the level energies with configurations 1s^2^2(s,p)^q^, 1s^2^2(s,p)^q-1^nl, 1s^1^2(s,p)^q+1^, 1s^1^2(s,p)^q^nl, 2(s,p)^q+2^, and 2(s,p)^q+1^nl, where 1<=q<=8, n<=5, and l<=3. We have compared our results with data from the National Institute of Standards and Technology (NIST) online database and with previous calculations. The average deviation of valence level energies ranges from 0.16eV in Ne-like ions to 0.01eV in Li-like ions, showing that the present MR-MP valence level energies are highly accurate. In the case of K-vacancy states, the deviation is generally below 0.3eV for Li-like SXIV and ArXVI. The deviation for K-vacancy energies in other L-shell ions (Be-, B-, C-, N-, and O-like Ar ions) is higher but likely because the NIST-recommended values have a higher uncertainty. The data set includes many n=4 and n=5 valence and K-vacancy levels in L-shell ions of S and Ar that have not been previously reported. The data can be used for line identification and modeling of L-shell ions of S and Ar in astrophysical and laboratory-generated plasmas, and as energy references in the absence of more accurate laboratory measurements.2018ApJS..238...34Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/238/34CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/125/149 : CHIANTI: An Atomic Database For Emission Lines I. (Dere+ 1997)J/A+A/436/1141 : Radiative rates in Ar XIII, Ar XIV & Ar XV (Aggarwal+, 2005)J/ApJS/156/105 : Transitions in L-shell ions of Fe and Ni (Gu+, 2005)J/A+A/518/A64 : Na-like iso-electronic sequence. II. (Liang+, 2010)J/A+A/533/A87 : Sulphur ions iso-electronic sequence (Liang+, 2011)J/A+A/547/A87 : B-like iso-electronic sequence (Liang+, 2012)J/ApJS/207/11 : Fe XVI radiative rates (Diaz+, 2013)J/A+A/564/A24 : Carbon isoelectronic sequence data (Ekman+, 2014)J/ApJS/215/26 : Energy levels & transition rates of C-like ions (Wang+, 2014)J/ApJS/218/16 : Energy levels & transition rates of Be-like ions (Wang+, 2015)J/ApJS/223/3 : Energies & radiative transition -- ArXII-ZnXXIV (Wang+, 2016)J/ApJS/234/13 : Relativistic MR-MP energy levels for Si (Santana+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/238/34https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/238/34http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/238/34https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/238/34https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/238/34http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/238/34GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJS/238/34/table1Level energies in L-shell ions of S evaluated with the MR-MP methodJJ levelphys.atmol.qncharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintN[3/10] Number of electronsmeta.numberintInd[1/3900] Level indexmeta.idintConfigThe jj-Configuration (1)meta.notecharParParity ("odd" or "even")phys.atmol.paritycharEnergy[0/7232] Present MR-MP energieseVphys.energy;phys.atmol.leveldoubleJ/ApJS/238/34/table2Level energies in L-shell ions of Ar evaluated with the MR-MP methodrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintN[3/10] Number of electronsmeta.numberintInd[1/3900] Level indexmeta.idintConfigThe jj-Configuration (1)meta.notecharJJ levelphys.atmol.qncharParParity ("odd" or "even")phys.atmol.paritycharEnergy[0/7232] Present MR-MP energieseVphys.energy;phys.atmol.leveldouble