A high-resolution line list for AlO
arXiv:2110.15295 · doi:10.1093/mnras/stab2525
Abstract
Indications of aluminium monoxide in atmospheres of exoplanets are being reported. Studies using high-resolution spectroscopy should allow a strong detection but require high accuracy laboratory data. A \textsc{marvel} (measured active rotational-vibrational energy levels) analysis is performed for the available spectroscopic data on AlO: 22\,473 validated transitions are used to determine 6\,485 distinct energy levels. These empirical energy levels are used to provide an improved, spectroscopically accurate version of the ExoMol ATP line list for AlO; at the same time the accuracy of the line lists for the isotopically-substituted species AlO, AlO and AlO are improved by correcting levels in line with the corrections used for AlO. These line lists are available from the ExoMol database at http://www.exomol.com.
References in corpus (16)
- ExoMol molecular line lists XXXV: a rotation-vibration line list for hot ammonia
- The 2020 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres
- ExoMol molecular line lists -- XXXVII: spectra of acetylene
- ExoMol molecular line lists: IX The spectrum of AlO
- ExoMol line lists VIII: A variationally computed line list for hot formaldehyde
- New Avenues for Thermal Inversions in hot Jupiters
- ExoMol molecular line lists XIX: high accuracy computed hot line lists for HO and HO
- ExoMol line lists XXXI: Spectroscopy of lowest eights electronic states of C
- MARVEL analysis of the measured high-resolution rovibronic spectra of TiO
- MARVEL analysis of the measured high-resolution rovibrational spectra of C2H2
- An update to the MARVEL dataset and ExoMol line list for 12C2
- Aluminium oxide in the atmosphere of hot Jupiter WASP-43b
- An improved rovibrational linelist of formaldehyde, \spec{h212c16o}
- Search for aluminium monoxide in the winds of oxygen-rich AGB stars
- Analysis of the TiO isotopologues in stellar optical spectra
- A potential new method for determining the temperature of cool stars