The experimental frequencies have been reported by
(1) R. L. de Zafra,
1971, Astrophys. J. 170, 165;
by
(2) R. A. Creswell, G. Winnewisser, and M. C. L. Gerry,
1977, J. Mol. Spectrosc. 65, 420;
by
(3) P. D. Mallinson and R. L. de Zafra,
1978, Mol. Phys. 36, 827;
by
(4) W. Chen, R. Bocquet, G. Wlodarczak, and D. Boucher,
1991, Int. J. Infrared Millimeter Waves 12, 987
by;
(5) K. M. T. Yamada, A. Moravec, and G. Winnewisser,
1995, Z. Naturforsch. 50a, 1179;
and by
(6) S. Thorwirth, H. S. P. Müller, and G. Winnewisser,
2000, J. Mol. Spectrosc. 204, 133.
The dipole moment was determined by
(7) R. L. DeLeon and J. S. Muenter,
1985, J. Chem. Phys. 82, 1702.
Predictions considering
hyperfine splitting
(J< 22) and related
partition functions
and selected vibrational contributions to the partition function are also available.
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