Laboratory and astronomical lines were reported by
(1) H. Gupta, P. B. Changala, J. Cernicharo, J. R. Pardo, M. Agúndez, C. Cabezas, B. Tercero, M. Guélin, and M. C. McCarthy, 2024, Astrophys. J. Lett. 966, Art. No. L28.
P. B. Changala is thanked for providing initial spectroscopic parameters. The quantum number J was limited to 15 because of the limited experimental data. The calculations are sufficient for observations in cold sources and somewhat sufficient in luke warm sources. Transition frequencies with calculated uncertainties exceeding 0.3 MHz should be viewed with some caution.
The dipole moment was taken from a quantum-chemical calculation in (1).