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The experimental data were taken from
(1) L. Kolesniková, I. Peña, E. R. Alonso,
B. Tercero, J. Cernicharo, S. Mata, and J. L. Alonso,
2018, Astron. Astrophys. 619, Art. No. A67.
A small fraction of lines were taken from
(2) H. Hirono, J. Shibano, A. Mitani, T. Sakaizumi,
M. Onda, O. Ohashi, and I. Yamaguchi,
1987, J. Mol. Struct. 162, 359.
The predictions are probably sufficient for all
needs of astronomers. Predictions with uncertainties
larger than 0.3 MHz should be viewed with
caution.
The dipole moment was determined in (2).
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