J/A+A/566/A10ivo://CDS.VizieR/J/A+A/566/A10doi:10.26093/cds/vizier.35660010CDSRauch T.Werner K.Quinet P.Kruk J.W.2017-07-11T13:09:10Z2014-05-30T08:01:58ZCDS support team

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

cds-question@unistra.fratomic-physicsFor the spectral analysis of high-resolution and high-signal-to-noise (S/N) spectra of hot stars, state-of-the-art non-local thermodynamic equilibrium (NLTE) model atmospheres are mandatory. These are strongly dependent on the reliability of the atomic data that is used for their calculation. Reliable Ba V-VII oscillator strengths are used to identify Ba lines in the spectra of the DA-type white dwarf G191-B2B and the DO-type white dwarf RE 0503-289 and to determine their photospheric Ba abundances. We newly calculated Ba V-VII oscillator strengths to consider their radiative and collisional bound-bound transitions in detail in our NLTE stellar-atmosphere models for the analysis of Ba lines exhibited in high-resolution and high-S/N UV observations of G191-B2B and RE 0503-289.2014A&A...566A..10Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/566/A10CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/546/A55 : Ge V and Ge VI oscillator strengths (Rauch+, 2012)J/A+A/564/A41 : Zn IV and Zn V oscillator strengths (Rauch+, 2014)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/566/A10https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/566/A10http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/566/A10https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/566/A10https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/566/A10http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/566/A10GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/566/A10/BaCombined table from original tablesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonSimbad column added by the CDSphys.atmol.ionStageintnullablelambda[312/115309] Wavelength {lambda}0.1nmem.wl;phys.atmol.transitiondoubleE0Lower level, energycm**-1phys.energy;phys.atmol.levelintP0[o/e] Lower level, parity (odd/even)phys.atmol.paritycharJ0[0/5] Lower level, angular momentum quantum number jphys.atmol.qnfloatE1Upper level, energycm**-1phys.energy;phys.atmol.levelintP1[o/e] Upper level, parity (odd/even)phys.atmol.paritycharJ1[0/5] Upper level, angular momentum quantum number Jphys.angMomentumfloatloggfCalculated HRF log gf value (1)phys.absorption.coeff;meta.modelledfloatloggAgA value (2)s**-1phys.atmol.transProbdoubleCFcancellation factor as defined by Cowan (3)phys.atmolfloat