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The transitions frequencies were taken
from
(1) G. Cazzoli, C. Degli Esposti, and F. Scappini,
1992, J. Chem. Phys., 97, 6187.
Predictions should be sufficiently reliable for all
radio astronomical observations. They should be viewed
with some caution beyond 400 GHz.
14N hyperfine splitting may be resolvable
at low quantum numbers. The pattern should be quite similar
to that of the main isotopolog.
The dipole moment was assumed to agree with that of
the main species, see e053519.cat.
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