J/A+A/366/1003ivo://CDS.VizieR/J/A+A/366/1003doi:10.26093/cds/vizier.33661003CDSCastelli F.Munari U.2001-02-11T20:31:42Z2001-02-11T21:31:38ZCDS support team

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

cds-question@unistra.frastronomical-modelsstellar-atmospheresspectroscopyIn this paper we complete the library of synthetic spectra for the range 7650-8750{AA}, which includes the 8500-8750{AA} interval currently base-lined for the spectroscopic observations by GAIA, candidate ESA Cornerstone 5 mission. As for Paper II (Munari & Castelli, Cat. <J/A+AS/141/141>), the spectra are based on Kurucz's codes and line data. The explored metallicity, gravity and temperature ranges are -2.5<=[Z/Z_{sun}_]<=+0.5, 4.5<=logg<=2.0 and 7750<=T_eff_<=50000K, respectively. The 698 new spectra are computed at the same {lambda}/{Delta}{lambda}=20000 resolving power of the observed spectra given in Paper I (Munari & Castelli, Cat. <J/A+AS/137/521>) (131 standard stars mapping the MKK spectral classification system) and the 254 synthetic spectra of Paper II (characterized by T_eff_<=7500K).2001A&A...366.1003Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/366/1003CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/137/521 : 8500-8750{AA} high resolution spectroscopy (Munari+, 1999)J/A+AS/141/141 : 8500-8750{AA} high resolution spectroscopy (Munari+, 2000)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/366/1003https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/366/1003http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/366/1003https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/366/1003https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/366/1003http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/366/1003GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/366/1003/tablesMain absorption lines in the interval 8490-8750{AA} for different spectra of solar metallicity (tables 2, 3 and 4 of the paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength0.1nmem.wldoublen_lambda[1/5]? Number of components of unresolved blendsmeta.noteintnullableIonIdentificationphys.atmol.elementcharMult? Multiplet numberphys.atmol.levelintnullableEPExcitation potential of the lower level in eVeVphys.energy;phys.atmol.excitationfloatEP2Excitation potential of the lower level in cm^-1^cm**-1phys.energy;phys.atmol.excitationdoubleloggfOscillator strengthphys.atmol.wOscStrengthfloatr_loggfSource of loggf (1)meta.refcharTeffEffective temperatureKphys.temperature.effectiveintloggSurface gravitylog(cm.s**-2)phys.gravityfloatRCIResidual central intensity for Teff and loggspect.line.intensityfloat