J/ApJS/239/11ivo://CDS.VizieR/J/ApJS/239/11doi:10.26093/cds/vizier.22390011CDSCivis S.Kubelik P.Ferus M.Zanozina E.M.Pastorek A.,Naskidashvili A.V.Chernov V.E.2022-05-05T11:46:23Z2019-01-28T09:58:46ZCDS support team

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

cds-question@unistra.fratomic-physicsinfrared-astronomyspectroscopyPrecision laboratory measurements are presented for 135 OI lines in the infrared (including 51 lines not measured previously in the laboratory) using time-resolved Fourier transform infrared spectroscopy in the 800-13000cm^-1^ region. The fine structure of some lines is observed for the first time. Using our linelist together with all relevant measurements from other works, we perform a re-optimization of OI level energies to obtain an internally consistent system of 2p^3^[^4^S]nl levels. Some OI level energies measured long ago are corrected. We also present a long list of oscillator strengths calculated with the help of quantum defect theory.2018ApJS..239...11Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/239/11CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/416/655 : Atomic lines in IR for ultracool dwarfs (Lyubchik+, 2004)J/ApJS/178/280 : Compendium of ISO far-IR extragalactic data (Brauher+, 2008)J/ApJ/753/13 : OI equivalent widths in Be stars (Mathew+, 2012)J/A+A/554/A24 : Infra-red transitions of Ca and Mg (Civis+, 2013)J/ApJ/778/132 : C and O abundances in 55 Cnc (Teske+, 2013)J/ApJ/791/58 : C & O abundances across the Hertzsprung gap (Adamczak+, 2014)J/ApJS/211/27 : An atlas of FUV spectra of 31 Cyg (Bauer+, 2014)J/A+A/568/A25 : C and O abundances in stellar populations (Nissen+, 2014)J/ApJS/214/26 : Line lists for CN isotopes transitions (Sneden+, 2014)J/A+A/573/A12 : SN1993J spectra 100-500 days post-explosion (Jerkstrand+, 2015)J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016)J/ApJS/225/15 : IR excess stars from Tycho-2 and AllWISE (Cotten+, 2016)J/ApJS/226/19 : FIR spectra of AGNs from Herschel (Fernandez-Ontiveros+, 2016)J/ApJS/222/1 : Faint ALMA 1.2mm sources down to ~0.02mJy (Fujimoto+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/239/11https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/239/11http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/239/11https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/239/11https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/239/11http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/239/11GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/ApJS/239/11/table2OI level energies extracted from the present measurement and other worksrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefRef = "Reference" levels (Zink+ 1991ApJ...371L..85Z ; De Natale+ 1993PhRvA..48757D)meta.codecharLevelLevelmeta.id;phys.atmol.levelEnergy[158/107598]? Energy level from this workcm**-1phys.energy;phys.atmol.leveldoublenullablee_Energy[0/0.05] Energy level uncertaintycm**-1stat.error;phys.energydoubleELOPT[158/107598] LOPT code (Kramida 2011CoPhC.182..419K) energy levelcm**-1meta.code;phys.energy;phys.atmol.leveldoublee_ELOPT[5e-06/0.02] ELOPT uncertaintycm**-1stat.errordoubleEM16? Energy level from Moore 1976stas.book.....Mcm**-1phys.energy;phys.atmol.leveldoublenullablef_EM16[a] Flag on EM16 (1)meta.codecharEB87[105441/107598]? Energy level from Brown+ 1987CPL...133..239Bcm**-1phys.energy;phys.atmol.leveldoublenullableEC88[102968/107598]? Energy level from Chang+ 1988PhyS...38...22Ccm**-1phys.energy;phys.atmol.leveldoublenullableEI08[158/105410]? Energy level from Ivanov+ 2008MNRAS.389L...4Icm**-1phys.energy;phys.atmol.leveldoublenullablee_EI08[5e-06/0.008]? EI08 uncertaintycm**-1stat.errordoublenullableEM17[76794/105166]? Energy level from Marinov+ 2017JPhB...50f5003Mcm**-1phys.energy;phys.atmol.leveldoublenullablee_EM17[0.004/0.009]? EM17 uncertaintycm**-1stat.errorfloatnullableJ/ApJS/239/11/table3*The experimentally measured lines included into our level optimizationRefReferences (1)meta.refcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTransitionTransition, i <- kphys.atmol.transProb;phys.atmol.transitionnu[0.02/105182.1] Used wavenumbercm**-1em.freqdoublee_nu[3.7e-05/0.08] Uncertainty of used wavenumbercm**-1stat.errordoubleO-Ritz[-0.05/0.05] Observed-minus-Ritz valuescm**-1stat.fit.omc;phys.energydoubleJ/ApJS/239/11/table4*QDT-calculated transition dipole line strengths, Sik, oscillator strengths, fik, and transition probabilities, Aki, of the oxygen atom in the 800-13000cm^-1^ rangerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTransitionTransition, i <- kphys.atmol.transProb;phys.atmol.transitionEi[73768.2/106788.6] Lower level energy, Eicm**-1phys.energy;phys.atmol.leveldoubleEk[86625.7/107597.5] Upper level energy, Ekcm**-1phys.energy;phys.atmol.leveldoublenu[807.2/12863.3] Ritz wavenumbercm**-1em.freqdoublelambda[777.1/12388.2] Air wavelengthnmem.wl;phys.atmol.transitiondoubleSik-QDT[0.003/78000] Transition dipole line strength, QDT (in au), this workspect.line.intensitydoublefik-QDT[8.9e-06/2.2] Oscillator strength, QDT, this workphys.atmol.oscStrengthdoubleAik-QDT[61.5/41500000] Transition probability, QDT, this works**-1phys.atmol.transProbdoublefik-NIST[1.7e-05/1.3]? Oscillator strength from NISTphys.atmol.oscStrengthdoublenullableacc-NISTNIST accuracy codes (1)meta.code.qualcharRef-NISTNIST Reference codes (2)meta.bibchar