J/MNRAS/501/1440ivo://CDS.VizieR/J/MNRAS/501/1440doi:10.26093/cds/vizier.75011440CDSCarvajal Gallego H.Palmeri P.Quinet P.2024-08-21T20:17:01Z2021-01-13T07:01:59ZCDS support team

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

cds-question@unistra.fratomic-physicsLarge-scale calculations of atomic structures and radiative properties have been carried out for singly, doubly- and trebly ionized cerium. For this purpose, the purely relativistic multiconfiguration Dirac-Hartree-Fock (MCDHF) method was used, taking into account the effects of valence-valence and core-valence electronic correlations in detail. The results obtained were then used to calculate the expansion opacities characterizing the kilonovae observed as a result of neutron star mergers. Comparisons with previously published experimental and theoretical studies have shown that the results presented in this work are the most complete currently available, in terms of quantity and quality, concerning the atomic data and monochromatic opacities for CeII, CeIII and CeIV ions.2021MNRAS.501.1440Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/501/1440CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/501/1440https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/501/1440http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/501/1440https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/501/1440https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/501/1440http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/501/1440GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/MNRAS/501/1440/table6MCDHF radiative parameters in CeIIEloLower level energycm**-1phys.energy;phys.atmol.levelintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength in vacuum0.1nmem.wldoublePloLower level parity ((o)= odd; (e)= even)phys.atmol.paritycharJloLower level total angular quantum numberphys.mol.qnfloatEupUpper level energycm**-1phys.energy;phys.atmol.levelintPupUpper level parity ((o)= odd; (e)= even)phys.atmol.paritycharJupUpper level total angular quantum numberphys.mol.qnfloatloggfWeighted oscillator strength in log scalephys.atmol.oscStrengthfloatGAWeighted transition probabilityphys.atmol.transProbdoubleB/CBabushkin over Coulomb gauges ratiophys.atmoldoubleJ/MNRAS/501/1440/table7MCDHF radiative parameters in CeIIIrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength in vacuum0.1nmem.wldoubleEloLower level energycm**-1phys.energy;phys.atmol.levelintPloLower level parity ((o)= odd; (e)= even)phys.atmol.paritycharJloLower level total angular quantum numberphys.mol.qnfloatEupUpper level energycm**-1phys.energy;phys.atmol.levelintPupUpper level parity ((o)= odd; (e)= even)phys.atmol.paritycharJupUpper level total angular quantum numberphys.mol.qnfloatloggfWeighted oscillator strength in log scalephys.atmol.oscStrengthfloatGAWeighted transition probabilityphys.atmol.transProbdoubleB/CBabushkin over Coulomb gauges ratiophys.atmoldoubleJ/MNRAS/501/1440/table8MCDHF radiative parameters in CeIVrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength in vacuum0.1nmem.wldoubleEloLower level energycm**-1phys.energy;phys.atmol.levelintPloLower level parity ((o)= odd; (e)= even)phys.atmol.paritycharJloLower level total angular quantum numberphys.mol.qnfloatEupUpper level energycm**-1phys.energy;phys.atmol.levelintPupUpper level parity ((o)= odd; (e)= even)phys.atmol.paritycharJupUpper level total angular quantum numberphys.mol.qnfloatloggfWeighted oscillator strength in log scalephys.atmol.oscStrengthfloatGAWeighted transition probabilityphys.atmol.transProbdoubleB/CBabushkin over Coulomb gauges ratiophys.atmoldouble