J/ApJS/239/30ivo://CDS.VizieR/J/ApJS/239/30doi:10.26093/cds/vizier.22390030CDSWang K.Song C.X.Jonsson P.Del Zanna G.Schiffmann S.Godefroid M.,Gaigalas G.Zhao X.H.Si R.Chen C.Y.Yan J.2019-03-21T10:47:36Z2019-03-11T11:53:18ZCDS support team

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

cds-question@unistra.fratomic-physicsWe present a consistent set of calculated energies and E1, M1, E2, M2 radiative transition data for the main n=3 levels from the 3s^2^3p^4^, 3p^6^, 3s3p^4^3d, 3s^2^3p^2^3d^2^, 3s3p^5^, 3s^2^3p^3^3d, and 3s3p^3^3d^2^ configurations for S-like ions from CrIX to CuXIV. The fully relativistic multiconfiguration Dirac-Hartree-Fock method implemented in the GRASP2K code (Jonsson+ 2007CoPhC.177..597J ; 2013CoPhC.184.2197J) is used to perform the present calculations. The excitation energies of the lowest 47 levels from the 3s^2^3p^4^, 3s3p^5^, and 3s^2^3p^3^3d configurations, producing the strongest lines, are found to be in good agreement, reaching spectroscopic accuracy, with the latest experimental values for FeXI evaluated by Del Zanna. Our energies can reliably be used to identify in astrophysical and laboratory spectra the 3s^2^3p^3^3d levels in other S-like ions, which are mostly unknown. On the contrary, significant discrepancies with the 3s3p^4^3d levels were found, emphasizing the need for more detailed experimental studies. A few new tentative identifications are suggested. The benchmarks we present indicate that our consistent set of radiative data is accurate and can be used for spectral line modeling.2018ApJS..239...30Whttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/239/30CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/125/149 : CHIANTI- An Atomic Database For Emission Lines I. (Dere+ 1997)J/ApJ/543/1016 : SERTS-97 EUV spectrum of solar active region (Brosius+ 2000)J/A+A/514/A40 : IRON project. LXVIII (Del Zanna+, 2010)J/A+A/549/A42 : FeXI soft X-ray lines (Del Zanna+, 2013)J/A+A/559/A100 : Boron isoelectronic sequence data (Jonsson+, 2013)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/227/16 : Energy levels & transition rates for F-like ions (Si+, 2016)J/ApJS/226/14 : MBPT calculations for Ne-like ions (Wang+, 2016)J/ApJS/223/3 : Energies & radiative transition ArXII to ZnXXIV (Wang+, 2016)J/ApJS/229/37 : Energy levels & transition rates of O-like ions (Wang+, 2017)J/ApJS/234/40 : Be-like ions from BII to NeVII transition data (Wang+, 2018)J/ApJS/235/27 : Energy levels & transition rates for P-like ions (Wang+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/239/30https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/239/30http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/239/30https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/239/30https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/239/30http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/239/30GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJS/239/30/table3Energy levels relative to the ground state along with radiative lifetime for the lowest 159 (227, 236, 304, 376, 436) states of Cr IX (Mn X, Fe XI, Co XII, Ni XIII, Cu XIV).recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZ[24/29] Atomic numbermeta.id;meta.mainintKey[1/435] Key numbermeta.idintLevelConfiguration and LSJ levelphys.atmol.configurationEMCDHF1[0/1631257] Energy levels, the present ab initio calculationscm**-1phys.energy;phys.atmol.levelintEMCDHF2[0/1631005] Energy levels, shifted energies of excited states (1)cm**-1phys.energyintENIST[0/763830]? Observed NIST energies (2)cm**-1phys.energy;phys.atmol.levelintnullableEMRMP[0/763720]? MR-MP calculations (3)cm**-1phys.energy;phys.atmol.levelintnullableLifetime-l[0/21.1] Lifetimes, present calculations in length gaugestime.lifetime;phys.atmol.leveldoubleLifetime-v[0/21.5] Lifetimes, present calculations in velocity gaugestime.lifetime;phys.atmol.leveldoubleLS-compLS eigenvector (4)meta.notecharJ/ApJS/239/30/table4Transition wavelengths, transition rates A, weighted oscillator strengths gf and line strengths between the states of Cr IX, Mn X, Fe XI, Co XII, Ni XIII, and Cu XIV listed in Table 3.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZ[24/29] Atomic numbermeta.id;meta.mainintj[1/245] Upper levelmeta.idinti[2/434] Lower levelmeta.idintWave[61.3/200240] Wavelength; Angstroms0.1nmem.wl;phys.atmol.transitiondoubleTypeTransition typemeta.notecharA-l[0.0001/3e+11] Transition rates, length forms**-1physdoublegf-l[5.9e-13/7.5] Weighted oscillator strengths, length formphys.atmol.oscStrengthdoubleStr-l[5.7e-10/84] Line strength; Atomic units, length formspect.line.intensitydoubleA-v[6.7e-05/3e+11]? Transition rates, velocity forms**-1phys.veloc;phys.atmol.transProb;phys.atmol.transitiondoublenullablegf-v[1.8e-12/7.5]? Weighted oscillator strengths, velocity formphys.atmol.oscStrengthdoublenullableStr-v[6.8e-10/4.6]? Line strength; Atomic units, velocity formspect.line.intensitydoublenullableBF[1e-05/1]? Branching fraction from the upper levelphys.atmol.branchingRatiodoublenullabledT[0/1]? Relative difference of the transition rates (1)phys.atmol.transProb;arith.diffdoublenullable