The measurements of the lower spin component were
taken from
(1) M. C. McCarthy, A. L. Cooksy, S. Mohamed,
V. D. Gordon, and P. Thaddeus,
2003, Astrophys. J. Suppl. Ser. 144, 287.
One unresolved HFS doublet was omitted because of a larger
residual. All other unresolved HFS doublets were treated
with 2 kHz uncertainties instead of the reported 5.
The calculation should be viewed with caution
above 80 GHz. In addition, the hyperfine
structure splitting should be viewed with some
caution below 7 GHz.
The partition function takes into account the higher
spin component as far as possible at present.
The dipole moment is from a quantum chemical
calculation in (1).
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