J/A+A/416/655ivo://CDS.VizieR/J/A+A/416/655doi:10.26093/cds/vizier.34160655CDSLyubchik Y.Jones H.R.A.Pavlenko Y.VViti S.Pickering J.C.,Blackwell-Whitehead R.2004-05-31T22:29:29Z2004-05-31T22:27:26ZCDS support team

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

cds-question@unistra.frdwarf-starsinfrared-astronomyspectroscopyatomic-physicsWe provide a set of atomic lines which are suitable for the description of ultracool dwarf spectra from 10000 to 25000{AA}. This atomic linelist was made using both synthetic spectra calculations and existing atlases of infrared spectra of Arcturus and Sunspot umbra. We present plots which show the comparison of synthetic spectra and observed Arcturus and Sunspot umbral spectra for all atomic lines likely to be observable in high resolution infrared spectra.2004A&A...416..655Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/416/655CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJS/103/235 : Arcturus IR spectral atlas (Wallace+ 1996)J/PASP/107/1042 : Infrared Arcturus Atlas (Hinkle+ 1995)J/AJ/126/1526 : IR photometry of ultracool dwarfs (Bouy+, 2003)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/416/655https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/416/655http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/416/655https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/416/655https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/416/655http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/416/655GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/A+A/416/655/table1Atomic lines found in ultracool dwarf synthetic spectrum from 1-2.5umrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPr? Priority of the line for measurement of atomic data (1)meta.idintnullablen_Ion[*] Note on measurements (2)meta.notecharlambdaWavelength of the line in air (3)0.1nmem.wl;phys.atmol.transitiondoubleIonElement name with ionization stagephys.atmol.elementcharUCDssResidual flux (F(line)/F(cont.)) in "ultracool dwarf" synthetic spectrumphot.flux;arith.ratiofloatArssResidual flux (F(line)/F(cont.)) in "Arcturus-like" synthetic spectrumphot.flux;arith.ratiofloatl_ArAt[~] Limit flag on ArAt (4)meta.code.errorcharArAt? Residual line intensity from hard copy of Arcturus atlas (accuracy 0.01-0.02) (6)spect.line.intensityfloatnullablen_ArAt[bl T] Note on ArAt (5)meta.notecharl_SsAt[~] Limit flag on SsAt (4)meta.code.errorcharSsAt? Residual line intensity from hard copy of Sunspot umbra atlas (accuracy 0.02-0.03) (5)spect.line.intensityfloatnullablen_SsAt[bl T] Note on SsAt (5)meta.notecharJ/A+A/416/655/table2Sensitivity of first priority lines to temperature, gravity and metallicity.AtomElement namephys.atmol.elementcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelength0.1nmem.wl;phys.atmol.transitiondoubleLDCentral line intensity in the ultra cool (2000/5.0/0.0) synthetic spectrumphot.flux.density;arith.difffloatSTeffTemperature sensitivity (1)%stat.fit.residualfloatSlogg? logg sensitivity (1)%stat.fit.residualfloatnullableS[M/H]Metallicity sensitivity (1)%stat.fit.residualfloat