J/A+A/523/A58ivo://CDS.VizieR/J/A+A/523/A58doi:10.26093/cds/vizier.35230058CDSWende S.Reiners A.Seifahrt A.Bernath P.F.2017-06-19T07:57:06Z2010-11-16T09:38:06ZCDS support team

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

cds-question@unistra.frspectroscopyinfrared-astronomylate-type-starsm-starsWe present an atlas for the iron-hydride molecule (FeH) in the z-range (990nm to 1076.6nm). We used high-resolution CRIRES spectra of the M-dwarf GJ1002, which is an ideal target for the investigation of FeH, because it is only very slow rotating (<3km/s) and exhibits only weak magnetic fields. The identified lines stem mainly from the (0-0) and (1-1) vibronic transitions, but also from the (1-0), (2-1), (2-2), (3-2), and (4-3) transitions. For the confirmation of the identifications, we used means of statistic and cross-correlation as well as the line intensities. We corrected the theoretical positions if needed and scaled the line intensities till they match the observations.2010A&A...523A..58Whttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/523/A58CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/523/A58https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/523/A58http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/523/A58https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/523/A58https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/523/A58http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/523/A58GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfrareddefaultJ/A+A/523/A58/table4FeH line datasAScaling factor for Aarith.factordoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaOObserved position (vacuum wavelength)0.1nmem.wl;phys.atmol.transitiondoublelambdaTTheoretical position (vacuum wavelength)0.1nmem.wl;phys.atmol.transitiondoublevlLower vibrational statephys.atmol.configurationintvuUpper vibrational statephys.atmol.configurationintOmegalLower {Omega}phys.atmol.qnfloatOmegauUpper {Omega}phys.atmol.qnfloatJlLower rotational statephys.mol.qnfloatJuUpper rotational statephys.mol.qnfloatB[1/3] Branch: 1=P-branch, 2=Q-branch, 3=R-branchmeta.codeintAEinstein A values**-1phys.atmol.transProbdoubleElLower level energyeVphys.energy;phys.atmol.levelfloatDlambdaPosition correction0.1nmarith.factor;posfloatBlendBlend fractionmeta.codefloatClClassification of the line (1)meta.code.classcharCommentComment, if the line is blended by and atomic feature, or if the classification of the line did not agree with the scaling factor of the Einstein A values (class {ne} s_A_)meta.notechar