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Nine very accurate low-N (≤ 2), low energy
MW transition frequencies are from
(2) R. Fuentetaja, C. Cabezas, Y. Endo, M. Agúndez,
A. Godard Palluet, F. Lique, B. Tercero, N. Marcelino,
P. de Vicente, and J. Cernicharo,
2025, Astron. Astrophys. 702, Art. No. A23.
Spectroscopic parameter were interpolated from CCS and CC34S,
except for B and the 33S hyperfine structure parameters.
Transition frequencies with calculated uncertainties exceeding
0.1 MHz should be viewed with great caution, higher-N
transitions with some additional caution.
The dipole moment is assumed to agree with that of the
main isotopolog, see e056002.cat.
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