The experimental lines are from
(1) S. Yamamoto and S. Saito,
1994, Can. J. Phys. 72, 954,
and from
(2) M. Tanimoto, T. Klaus, H. S. P. Müller, and
G. Winnewisser,
2000, J. Mol. Spectrosc. 199, 73.
The sextic distortion term HK was kept
fixed to a value from
(3) S. H. Ashworth, K. M. Evenson, and J. M. Brown,
1995, J. Mol. Spectrosc. 172, 282.
The 1H hyperfine splitting is negligible
for most transitions. Because of significant splitting
occuring in different frequency regions and at various
quantum numbers we provide an entry with complete hfs
splitting.
Because of the small number od observed transitions with
hfs splitting and because of the setup of the input files,
no experimental lines have been merged.
Predictions of a-type transitions with predicted
uncertainties larger than 1 MHz or b-type
transitions with Ka >
3 2 should be viewed with caution.
The dipole moment is from an ab initio calculation
from
(4) K. A. Peterson, A. Mitrushchenkov, and J. S. Francisco,
2008, Chem. Phys. 346, 34.
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