Fourier-transform spectroscopy of 13C17O and deperturbation analysis of the A1Π (υ=0–3) levels

R. Hakalla*, M. L. Niu, R.W. Field, A. N. Heays, E. J. Salumbides, G. Stark, J.R. Lyons, M. Eidelsberg, J.L. Lemaire, S. R. Federman, N. de Oliveira, W. Ubachs

*Corresponding author for this work

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Abstract

The high-resolution B1Σ+→A1Π (0, 0) and (0, 3) emission bands of the less-abundant 13C17O isotopologue have been investigated by Fourier-transform spectroscopy in the visible region using a Bruker IFS 125HR spectrometer at an accuracy 0.003 cm-1. These spectra are combined with high-resolution photoabsorption measurements of the 13C17O B1Σ+←X1Σ+ (0, 0), B1Σ+←X1Σ+ (1, 0) and C1Σ+←X1Σ+ (0, 0) bands recorded with an accuracy of 0.01 cm-1 using the vacuum ultraviolet Fourier-transform spectrometer, installed on the DESIRS beamline at the SOLEIL synchrotron. In the studied 17,950–22,500 cm-1 and 86,800–92,100 cm-1 regions, 480 transitions have been measured. These new experimental data were combined with data from the C→A and B→A systems, previously analyzed in 13C17O. The frequencies of 1003 transitions derived from 12 bands were used to analyze the perturbations between the A1Π (υ=0–3) levels and rovibrational levels of the d3Δi, e3Σ-, a'3Σ+, I1Σ- and D1Δ states as well as to a preliminary investigation of weak irregularities that appear in the B1Σ+ (υ=0) level. Deperturbed molecular constants and term values of the A1Π state were obtained. The spin-orbit and L-uncoupling interaction parameters as well as isotopologue-independent spin-orbit and rotation-electronic perturbation parameters were derived.

Original languageEnglish
Pages (from-to)312-328
Number of pages17
JournalJournal of Quantitative Spectroscopy and Radiative Transfer
Volume189
Early online date10 Dec 2016
DOIs
Publication statusPublished - Mar 2017

Funding

R. Hakalla thanks LASERLAB-EUROPE for support of this research via funding Grants EUH2020-RIP-654148 and EC's-SFP-284464. We are grateful to the general and technical staff of SOLEIL Synchrotron as well as to the scientific committee for providing beam time under Project numbers 20110121, 20120653, and 20140051. R.W. Field thanks the US National Science Foundation [Grant number CHE-1361865] for support of his research, which includes substantive collaborations. J.R. Lyons and G. Stark thank the NASA Origins of Solar Systems program for support [Grant number NNX14AD49G]. S. Federman was supported by NASA Grants NNG 06-GG70G and NNX10AD80G to the University of Toledo. J.-L. Lemaire thanks the ISMO-CNRS (Institut des Sciences Moléculaires d'Orsay at Université Paris-Sud) for his welcome as honorary professor. R. Hakalla would like to express his gratitude for the support of the European Regional Development Fund and the Polish state budget within the framework of the Carpathian Regional Operational Programme [Grant RPPK.01.03.00-18-001/10] for the period of 2007–2013 through the funding of the Centre for Innovation and Transfer of Natural Science and Engineering Knowledge of the University of Rzeszów.

FundersFunder number
ISMO-CNRS
Institut des Sciences Moléculaires d'Orsay
National Science FoundationCHE-1361865
National Aeronautics and Space AdministrationNNX14AD49G, NNG 06-GG70G, NNX10AD80G
Horizon 2020 Framework Programme670168, 654148
University of Toledo
Université Paris-Sud
European Regional Development FundRPPK.01.03.00-18-001/10

    Keywords

    • CO isotopologue
    • Carbon monoxide
    • FT-spectroscopy
    • High resolution VUV–VIS spectra
    • Perturbation analysis

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