Abstract
The A1Π(v = 1) level of the 12C18O isotopologue was precisely reinvestigated with two complementary spectroscopic techniques. High resolution B1Σ+ → A1Π(0, 1), (1, 1) and C1Σ+ → A1Π(0, 1) emission bands were recorded in the visible region, 20,700 – 26,100 cm−1, with a 1.71 m Fourier-transform spectrometer (Bruker IFS 125-HR) installed at the University of Rzeszów. The resulting line centre accuracy of isolated and medium to strong lines is 0.005 cm−1. In addition, high-resolution spectra of the A1Π ⟵ X1Σ+(1, 0), B1Σ+⟵ X1Σ+(0, 0) and (1, 0) as well as C1Σ+⟵ X1Σ+(0, 0) bands were recorded between 66,200 and 95,250 cm−1 using the vacuum-ultraviolet Fourier-transform spectrometer installed at the DESIRS beamline of the SOLEIL synchrotron. The wavenumber accuracy for isolated and strong spectral lines is 0.01 cm−1. A data set of 626 spectral lines belonging to seven bands was incorporated into a global deperturbation analysis. Significantly improved deperturbed molecular constants for the A1Π(v = 1), a´3Σ+(v = 10), D1Δ(v = 1), and I1Σ−(v = 2) levels, term values of the B1Σ+(v = 0, 1) and C1Σ+(v = 0) Rydberg states as well as the accompanying spin-orbit and rotation-electronic (L-uncoupling) interaction parameters were obtained. The experimental ro-vibrational term values of the A1Π(v = 1) level and its perturbers were also determined. The mixed composition of interacting states is expressed in terms of their 1Π percentage character.
| Original language | English |
|---|---|
| Article number | 107243 |
| Pages (from-to) | 1-16 |
| Number of pages | 16 |
| Journal | Journal of Quantitative Spectroscopy and Radiative Transfer |
| Volume | 255 |
| Early online date | 4 Aug 2020 |
| DOIs | |
| Publication status | Published - Nov 2020 |
Funding
RH thanks LASERLAB-EUROPE for support of this research [grant numbers EUH2020-RIP-654148 , EC's-SPF-284464 ] and European Regional Development Fund and the Polish state budget within the framework of the Carpathian Regional Operational Programme [grant number RPPK.01.03.00-18-001/10] through the funding of the Center for Innovation and Transfer of Natural Sciences and Engineering Knowledge of the University of Rzeszów. WU and AH thank the Dutch Astrochemistry Network (NWO) for support [grant number 648.000.021]. AH was funded by the NASA Postdoctoral Program through the NASA Astrobiology Institute. RWF is grateful to the US National Science Foundation [grant number CHE-1800410 ]. The authors are grateful to the general and technical staff of SOLEIL synchrotron for providing beam time under project numbers 20120653 and 20160118. RH thanks LASERLAB-EUROPE for support of this research [grant numbers EUH2020-RIP-654148, EC's-SPF-284464] and European Regional Development Fund and the Polish state budget within the framework of the Carpathian Regional Operational Programme [grant number RPPK.01.03.00-18-001/10] through the funding of the Center for Innovation and Transfer of Natural Sciences and Engineering Knowledge of the University of Rzesz?w. WU and AH thank the Dutch Astrochemistry Network (NWO) for support [grant number 648.000.021]. AH was funded by the NASA Postdoctoral Program through the NASA Astrobiology Institute. RWF is grateful to the US National Science Foundation [grant number CHE-1800410]. The authors are grateful to the general and technical staff of SOLEIL synchrotron for providing beam time under project numbers 20120653 and 20160118.
| Funders | Funder number |
|---|---|
| Dutch Astrochemistry Network | |
| National Aeronautics and Space Administration | |
| NASA Astrobiology Institute | |
| National Science Foundation | 1800410, 20120653, 20160118, CHE-1800410 |
| Nederlandse Organisatie voor Wetenschappelijk Onderzoek | 648.000.021 |
| Horizon 2020 Framework Programme | 654148 |
| European Commission | 284464 |
| European Regional Development Fund | RPPK.01.03.00-18-001/10 |
Keywords
- CO
- Deperturbation analysis
- Fourier-transform spectroscopy
- High-resolution VUV and VIS spectra
- Isotopologues
- Spin-orbit, spin-electronic and rotation-electronic couplings
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