Imidogen, azanydene, X 3Σ
Species tag 015501
Date of EntryMay 2004
ContributorH. S. P. Müller

The observed transitions were taken from
(1) T. Klaus, S. Takano, and G. Winnewisser, 1997, Astron. Astrophys. 322, L1;
(2) J. Flores-Mijangos, J. M. Brown, F. Matsushima, H. Odashima, K. Takagi, L. R. Zink, and K. M. Evenson, 2004, J. Mol. Spectrosc. 225, 189
; and from
(3) F. Lewen, S. Brünken, G. Winnewisser, M. Simecková, and S. Urban, 2004, J. Mol. Spectrosc. 226, 113.
Note: Overlapping features have been treated specially in (2) and (3). In (2), the frequency of the overlapping hyperfine feature was corrected so that the frequency could be attributed to the strongest hyperfine component. In (3), the weights of the hyperfine components were adjusted according to their contribution to the measured frequency of the overlapping lines.
Transitions with uncertainties larger than 100 and 200 kHz for the N = 1 – 0 and all other transitions, respectively, have not been merged.
Also used in the fit were ground state combination differences from an infrared emission spectrum by
(4) R. S. Ram, P. F. Bernath, and K. H. Hinkle, 1999, J. Chem. Phys. 110, 5557. They have been provided by M. S.; see (3).
The dipole moment was taken from
(5) E. A. Scarl and F. W. Dalby, 1974, Can. J. Phys. 52, 1429.

Lines Listed1948
Frequency / GHz< 16489
Max. J18
log STR0-12.0
log STR1-12.0
Isotope Corr.-0.0
Egy / cm–10.0
 µa / D1.389
 µb / D 
 µc / D 
 A / MHz 
 B / MHz489959.1
 C / MHz 
detected in ISM/CSMyes

Database maintained by Holger S. P. Müller and Sven Thorwirth, programming by D. Roth and F. Schloeder