The DOI matches its Crossref record; 23 of the 23 references it cites were found in a registry or an index.
A high-accuracy computed water line list
Open accessAbstract
A computed list of H216O infrared transition frequencies and intensities is presented. The list, BT2, was produced using a discrete variable representation two-step approach for solving the rotation–vibration nuclear motions. It is the most complete water line list in existence, comprising over 500 million transitions (65 per cent more than any other list) and it is also the most accurate (over 90 per cent of all known experimental energy levels are within 0.3 cm−1 of the BT2 values). Its accuracy has been confirmed by extensive testing against astronomical and laboratory data. The line list has been used to identify individual water lines in a variety of objects including comets, sunspots, a brown dwarf and the nova-like object V838 Mon. Comparison of the observed intensities with those generated by BT2 enables water abundances and temperatures to be derived for these objects. The line list can also be used to provide an opacity for models of the atmospheres of M dwarf stars and assign previously unknown water lines in laboratory spectra.
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Cites
Hauschildt, P. H., Allard, F., & Baron, E. (1999) · The Astrophysical Journal · doi:10.1086/306745 · Cited by 1,207
Partridge, H., & Schwenke, D. W. (1997) · The Journal of Chemical Physics · doi:10.1063/1.473987 · Cited by 1,155
Spectra of Atoms and Molecules
Bernath, P. F., & Dalgarno, A. (1996) · Physics Today · doi:10.1063/1.2807548 · Cited by 423
Mumma, M. J., DiSanti, M. A., Russo, N. D., Fomenkova, M., Magee-Sauer, K., Kaminski, C. D., & Xie, D. X. (1996) · Science · doi:10.1126/science.272.5266.1310 · Cited by 319
DVR3D: a program suite for the calculation of rotation–vibration \nspectra of triatomic molecules
Tennyson, J., Kostin, M. A., Barletta, P., Harris, G. J., B, O. L. P. A., Ramanlal, J., & Zobov, N. F. (2004) · UCL Discovery (University College London) · Cited by 296
Self-citationSchwenke, D. W., & Partridge, H. (2000) · The Journal of Chemical Physics · doi:10.1063/1.1311392 · Cited by 276
Spectra of atoms and molecules
(2005) · Choice Reviews Online · doi:10.5860/choice.43-1624 · Cited by 265
Dust in the Photospheric Environment: Unified Cloudy Models of M, L, and T Dwarfs
Tsuji, T. (2002) · The Astrophysical Journal · doi:10.1086/341262 · Cited by 165
Hot H 2 O Emission and Evidence for Turbulence in the Disk of a Young Star
Carr, J. S., Tokunaga, A. T., & Najita, J. (2004) · The Astrophysical Journal · doi:10.1086/381356 · Cited by 146
Synthetic Spectra and Mass Determination of the Brown Dwarf Gliese 229B
Allard, F. C., Hauschildt, P. H., Baraffe, I., & Chabrier, G. (1996) · The Astrophysical Journal · doi:10.1086/310143 · Cited by 137
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The HITRAN2016 molecular spectroscopic database
Gordon, I. E., Rothman, L. S., Hill, C., Kochanov, R. V., Tan, Y., Bernath, P. F., Birk, M., Boudon, V., Campargue, A., Chance, K. V., et al. (2017) · Journal of Quantitative Spectroscopy and Radiative Transfer · doi:10.1016/j.jqsrt.2017.06.038 · Cited by 7,721
“vapor was implemented, thanks to the ab initio calculations from the BT2 line list [15] and, in selected spectral intervals, Lodi et al.”
Self-citationThe HITRAN 2008 molecular spectroscopic database
Rothman, L. S., Gordon, I. E., Barbe, A., Benner, D. C., Bernath, P. F., Birk, M., Boudon, V., Brown, L. R., Campargue, A., Champion, J.-P., et al. (2009) · Journal of Quantitative Spectroscopy and Radiative Transfer · doi:10.1016/j.jqsrt.2009.02.013 · Cited by 3,335
Self-citationThe HITRAN2012 molecular spectroscopic database
Rothman, L. S., Gordon, I. E., Babikov, Y., Barbe, A., Chris Benner, D., Bernath, P. F., Birk, M., Bizzocchi, L., Boudon, V., Brown, L. R., et al. (2013) · Journal of Quantitative Spectroscopy and Radiative Transfer · doi:10.1016/j.jqsrt.2013.07.002 · Cited by 3,255
Self-citationModels of very-low-mass stars, brown dwarfs and exoplanets
Allard, F., Homeier, D., & Freytag, B. (2012) · Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences · doi:10.1098/rsta.2011.0269 · Cited by 921
The ExoMol database: Molecular line lists for exoplanet and other hot atmospheres
Tennyson, J., Yurchenko, S. N., Al-Refaie, A. F., Barton, E. J., Chubb, K. L., Coles, P. A., Diamantopoulou, S., Gorman, M. N., Hill, C., Lam, A. Z., et al. (2016) · Journal of Molecular Spectroscopy · doi:10.1016/j.jms.2016.05.002 · Cited by 538
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Metadata
- Authors
- Barber, R. J., Tennyson, J., Harris, G. J., & Tolchenov, R. N.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2006-04-13
- Volume
- 368
- Issue
- 3
- Pages
- 1087-1094
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2170742148
- Cited by
- 709
- References
- 23
- FWCI
- 13.91
- Type
- journal article
- Language
- en
- Open access
- bronze
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