Transition frequencies were taken
from
(1) G. Cazzoli, C. Degli Esposti, and F. Scappini,
1992, Chem. Phys. Lett., 194, 297.
Predictions should be sufficiently reliable for all
radio astronomical observations. They should be viewed
with some caution beyond 600 GHz.
The dipole moment was assumed to agree with that of
the main species, see e053519.cat.
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