Lines without 7Li hyperfine splitting were
reported by
(1) A. J. Apponi, M. A. Brewster, and L. M. Ziurys,
1998, Chem. Phys. Lett. 298, 161.
Lines with hyperfine splitting were reported by
(2) P. M. Sheridan, M. K. L. Binns, M. Sun, J. Min, M. P.
Bucchino, D. T. Halfen, L. M. Ziurys,
2011, J. Mol. Spectrosc. 269, 231.
The stated uncertainties in (1, 2) appear to be too
conservative; smaller values have been employed here.
Predictions may be reliable up to 900 GHz.
Hyperfine splitting is deemed to be irrelevant for
astronomical observations.
The dipole moment is from an ab initio calculation
by
(3) H. S. P. Müller, 2011, unpublished.
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