What It Takes to Compute Highly Accurate Rovibrational Line Lists for Use in Astrochemistry

Author:

Huang Xinchuan12,Schwenke David W.3,Lee Timothy J.4ORCID

Affiliation:

1. SETI Institute, 189 Bernardo Avenue, Suite 200, Mountain View, California 94043, United States

2. MS 245-6, Astrophysics Branch, Space Science and Astrobiology Division, NASA Ames Research Center, Moffett Field, California 94035, United States

3. MS 258-2, NAS Facility, NASA Ames Research Center, Moffett Field, California 94035, United States

4. MS245-3, Planetary Systems Branch, Space Science and Astrobiology Division, NASA Ames Research Center, Moffett Field, California 94035, United States

Funder

National Aeronautics and Space Administration

Publisher

American Chemical Society (ACS)

Subject

General Medicine,General Chemistry

Reference67 articles.

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4. Exploring the limits of the Data-Model-Theory synergy: “Hot” MW transitions for rovibrational IR studies

5. Fortney, J. J.; Robinson, T. D.; Domagal-Goldman, S.; Amundsen, D. S.; Brogi, M.; Claire, M.; Crisp, D.; Hebrard, E.; Imanaka, H.; de Kok, R.; Marley, M. S.; Teal, D.; Barman, T.; Bernath, P.; Burrows, A.; Charbonneau, D.; Freedman, R. S.; gelino, D.; Helling, C.; Heng, K.; Jensen, A. G.; Kane, S.; Kempton, E. M.R.; Kopparapu, R. K.; Lewis, N. K.; Lopez-Morales, M.; Lyons, J.; Lyra, W.; Meadows, V.; Moses, J.; Pierrehumbert, R.; Venot, O.; Wang, S. X.; Wright, J. T. The Need for Laboratory Work to Aid in The Understanding of Exoplanetary Atmospheres. 2016; pp 1–18, http://arxiv.org/abs/1602.06305.

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