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The lines have been reported in
(1) A. J. Apponi, M. C. McCarthy, C. A. Gottlieb, and P. Thaddeus,
2000, Astrophys. J. 536, L55;
and in
(2) M. C. McCarthy, A. J. Apponi, C. A. Gottlieb, and P. Thaddeus,
2001, J. Chem. Phys. 115, 870.
The fit has been carried out using constants and quantum numbers
of Hund's case (b). The prediction of the
14N hyperfine splitting for the
high lying Π3/2 substate should be
viewed with some caution because no low N transition with
resolved hyperfine splitting has been observed for this substate.
The dipole moment is from an ab initio calculation
mentioned in (1).
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