ExoMol line lists XVIII. The high temperature spectrum of VO
arXiv:1609.06120 · doi:10.1093/mnras/stw1969
Abstract
An accurate line list, VOMYT, of spectroscopic transitions is presented for hot VO. The 13 lowest electronic states are considered. Curves and couplings are based on initial {\it ab initio} electronic structure calculations and then tuned using available experimental data. Dipole moment curves, used to obtain transition intensities, are computed using high levels of theory (e.g. MRCI/aug-cc-pVQZ using state-specific or minimal-state CAS for dipole moments). This line list contains over 277 million transitions between almost 640,000 energy levels. It covers the wavelengths longer than 0.29 m and includes all transitions from energy levels within the lowest nine electronic states which have energies less than 20,000 \cm{} to upper states within the lowest 13 electronic states which have energies below 50,000 \cm{}. The line lists give significantly increased absorption at infrared wavelengths compared to currently available VO line lists. The full line lists is made available in electronic form via the CDS database and at www.exomol.com.
MNRAS in press
References in corpus (14)
- A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
- An Optical Spectroscopic Study of T Tauri Stars. I. Photospheric Properties
- Atomic and Molecular Opacities for Brown Dwarf and Giant Planet Atmospheres
- Can TiO Explain Thermal Inversions in the Upper Atmospheres of Irradiated Giant Planets?
- Transmission spectral properties of clouds for hot Jupiter exoplanets
- Pseudo 2D chemical model of hot Jupiter atmospheres: application to HD 209458b and HD 189733b
- TiO and VO broad band absorption features in the optical spectrum of the atmosphere of the hot-Jupiter HD209458b
- ExoMol molecular line lists: IX The spectrum of AlO
- Transit spectroscopy with JWST: Systematics, starspots and stitching
- A search for TiO in the optical high-resolution transmission spectrum of HD 209458b: Hindrance due to inaccuracies in the line database
- Evidence against a strong thermal inversion in HD 209458 b from high-dispersion spectroscopy
- The calculated rovibronic spectrum of scandium hydride, ScH
- Hybrid variation-perturbation method for calculating rovibrational energy levels of polyatomic molecules
- Ab initio calculations to support accurate modelling of the rovibronic spectroscopy calculations of vanadium monoxide (VO)
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- A method for the variational calculation of hyperfine-resolved rovibronic spectra of diatomic molecules
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