J/A+A/580/A10ivo://CDS.VizieR/J/A+A/580/A10doi:10.26093/cds/vizier.35800010CDSCastelli F.Kurucz R.L.Cowley C.R.2015-11-01T17:09:56Z2015-07-20T07:43:46ZCDS support team

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

cds-question@unistra.frpeculiar-variable-starsspectroscopyastronomical-modelsstellar-atmospheresThe NIST database lists several MnI lines that were observed in the laboratory but not classified. They cannot be used in spectrum synthesis because their atomic line data are unknown. These lines are concentrated in the 2380-2700{AA} interval. We aimed to assign energy levels and loggf values to these lines. Semi-empirical line data for MnII computed by Kurucz were used to synthesize the ultraviolet spectrum of the slow-rotating, HgMn star HD 175640. The spectrum was compared with the high-resolution spectrum observed with the HST-STIS equipment. A UVES spectrum covering the 3050-10000{AA} region was also examined.2015A&A...580A..10Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/580/A10CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJS/205/14 : Energy levels and spectral lines of MnII (Kramida+, 2013)J/A+A/425/263 : Spectroscopic atlas of HD175640 (Castelli+, 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/580/A10https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/580/A10http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/580/A10https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/580/A10https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/580/A10http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/580/A10GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/580/A10/tablea1The new energy levels of MnII and the predicted observed in the spectrumrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintE1[82303/119938] Energy of the upper levelcm**-1phys.energy;phys.atmol.leveldoubleConf1Configuration of the upper energy levelphys.energyTerm1Term of the upper energy level configurationphysJ1[1/7] J quantum number of the upper energy levelmeta.id;meta.mainfloatE0[14325/85637] Energy of the lower energy levelcm**-1phys.energy;phys.atmol.leveldoubleConf0Configuration of the lower energy levelphys.energyTerm0Term of the lower energy level configurationphysJ0[0/8] J quantum number of the lower energy levelmeta.idfloatlam.R[1444./3036] Wavelength from energy levels ({lambda}(Ritz))0.1nmem.wl;phys.atmol.transitiondoubleloggflog(gf) value computed by Kurucz (K14)phys.absorption.coefffloatlam.N[2382/2958]? Wavelength from the NIST database ({lambda}(NIST))0.1nmem.wldoublenullableNotesNotes (1)meta.notecharJ/A+A/580/A10/tablea2Lines from the NIST database in the 2400-3040{AA} interval that are observed in the spectrum, but are either not predicted or predicted as too weakrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambda[2409/2933] Wavelength from the NIST database0.1nmem.wldoubleloggflog(gf) value computed by Kurucz (K14)phys.absorption.coefffloatE0[27589/79801] Energy of the lower levelcm**-1phys.energy;phys.atmol.leveldoubleJ0[0/6] J quantum number of the lower energy levelmeta.id;meta.mainintConf0Configuration of the lower energy levelphys.energyTerm0Term of the lower energy level configurationphysE1[66645/119279] Energy of the upper levelcm**-1phys.energy;phys.atmol.leveldoubleJ1[1/6] J quantum number of the upper energy levelmeta.idintConf1Configuration of the upper energy levelphys.energyTerm1Term of the upper energy level configurationphysNotesNotes (1)meta.notechar