Spectroscopy and perturbation analysis of the CO AX (2,0), (3,0) and (4,0) bands
arXiv:1510.02509 · doi:10.1080/00268976.2015.1108472
Abstract
The (2,0) (3,0) and (4,0) bands of the AX system of CO have been re-investigated by high-resolution vacuum ultraviolet absorption spectroscopy. A VUV Fourier-transform spectrometer, illuminated by synchrotron radiation, was applied to record a jet-cooled spectrum, a room temperature static gas spectrum and a high temperature (900 K) quasi-static gas spectrum, resulting in absolute accuracies of 0.010.02 cm for the rotational line frequencies. Precise laser-based data were included in the analysis allowing for a highly accurate determination of band origins. Rotational levels up to were observed. The data were used to perform an improved analysis of the perturbations in the A, , , and levels by vibrational levels of the D, I, e, d, and a states.
12 pages, 4 figures, 5 tables, Molecular Physics (2015) accepted
References in corpus (4)
- The CO A-X System for Constraining Cosmological Drift of the Proton-Electron Mass Ratio
- Constraint on a varying proton-to-electron mass ratio from molecular hydrogen absorption toward quasar SDSS J123714.60+064759.5
- High-precision laser spectroscopy of the CO A - X (2,0), (3,0) and (4,0) bands
- VUV-synchrotron absorption studies of N and CO at 900 K
Cited by in corpus (4)
- Constraint on a cosmological variation in the proton-to-electron mass ratio from electronic CO absorption
- Spectroscopy and perturbation analysis of the A(v=0) state of CO
- Fourier-transform spectroscopy of CO and deperturbation analysis of the A ( = 0 - 3) levels
- Precision spectroscopy and comprehensive analysis of perturbations in the ) state of CO