

Spectra of selected CO2 isotopologues at T = 296 K, scaled by terrestrial isotopic abundances. In addition to 12C16O2, only 13C16O2 and 16O12C18O produce detectable IR features. — astro-ph.EP
Extensive rovibrational line lists are constructed for 12 isotopologues of carbon dioxide: 12C16O2, 13C16O2, 12C17O2, 13C17O2, 12C18O2, 13C18O2, 16O12C17O, 16O12C18O, 16O13C17O, 16O13C18O, 17O12C18O, and 17O13C18O.
The variational program TROVE was employed together with an exact kinetic energy operator, accurate empirical potential energy surface (Ames-2) and the ab initio dipole moment surface Ames-2021-40K. Empirical energy levels from the most recent MARVEL analyses, as well as from the HITRAN and CDSD databases, are used to replace calculated values where available.
The line lists are further supplemented by assigning AFGL quantum numbers using machine-learning based estimators. The resulting data were employed to generate opacities with four radiative transfer codes, TauREx, ARCiS, NEMESIS, and petitRADTRANS, both for individual isotopologues and for CO2 at terrestrial isotopic natural abundance. All line lists and associated data are available at this http URL.
Sergei N. Yurchenko, Marco G. Barnfield, Charles A. Bowesman, Ryan P. Brady, Elizabeth R. Guest, Kyriaki Kefala, Qing-He Ni, Armando N. Perri, Oleksiy A. Smola, Andrei Solokov, Chenyi Tao, Jonathan Tennyson
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Astrophysics of Galaxies (astro-ph.GA); Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:2512.13889 [astro-ph.EP] (or arXiv:2512.13889v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2512.13889
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Related DOI:
https://doi.org/10.1093/mnras/staf2135
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Submission history
From: Sergei Yurchenko N
[v1] Mon, 15 Dec 2025 20:46:49 UTC (8,952 KB)
https://arxiv.org/abs/2512.13889
Astrobiology, Astrochemistry,





