The data are from astronomical observations in
(1) C. Cabezas, M. Agúndez, N. Marcelino, B. Tercero, Y. Endo,
R. Fuentetaja, J. R. Pardo, P. de Vincente, and J. Cernicharo,
2022, Astron. Astrophys. 657, Art. No. L4.
The data set is somewhat limited. Therefore, transitions were
truncated at 302 GHz and at N = 20. The calculations
are sufficient for observations in cold environments, possibly
not in warm ones. Transition frequencies with calculated
uncertainties exceeding 0.1 MHz should be viewed with caution.
The dipole moment is from a coupled cluster quantum-chemical
calculation by
(2) C. Puzzarini,
2008, Chem. Phys. 346, 45.
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