Abstract
A new ro-vibrational line list for the ground electronic state of the main isotopologue of acetylene, (C2H2)-C-12, is computed as part of the ExoMol project. The aCeTY line list covers the transition wavenumbers up to 10 000 cm(-1) (lambda > 1 mu m), with lower and upper energy levels up to 12 000 and 22 000 cm(-1) considered, respectively. The calculations are performed up to a maximum value for the vibrational angular momentum, K-max = L-max = 16, and maximum rotational angular momentum, J = 99. Higher values of J were not within the specified wavenumber window. The aCeTY line list is considered to be complete up to 2200 K, making it suitable for use in characterizing high-temperature exoplanet or cool stellar atmospheres. Einstein-A coefficients, which can directly be used to calculate intensities at a particular temperature, are computed for 4.3 billion (4 347 381 911) transitions between 5 million (5 160803) energy levels. We make comparisons against other available data for (C2H2)-C-12, and demonstrate this to be the most complete line list available. The line list is available in electronic form from the online CDS and ExoMol data bases.
| Original language | English |
|---|---|
| Pages (from-to) | 1531-1545 |
| Number of pages | 15 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 493 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - Apr 2020 |
Keywords
- molecular data
- planets and Satellites: atmospheres
- stars: atmosphere
- stars: carbon
- ROTATION-VIBRATION SPECTRUM
- DYNAMIC-MODEL ATMOSPHERES
- NEAR-INFRARED SPECTRA
- CARBON STARS
- ABSORPTION-SPECTRUM
- SPECTROSCOPIC DATA
- AGB STARS
- CHEMISTRY
- METHANE
- CM(-1)
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