The data were taken from:
(1) G. Cazzoli and C. Puzzarini, 2008,
Astron. Astrophys. 487, 1197;
(2) H. S. P. Müller, S. Thorwirth, L. Bizzocchi, and G. Winnewisser,
2000, Z. Naturforsch. 55a, 491; and from
(3) H. S. P. Müller, P. Pracna, and V.-M. Horneman,
2002, J. Mol. Spectrosc. 216, 397.
Ground state combination loops published in Ref. 3 permit
A B and DK to
be determined; HK has been estimated.
There is little special in the files. The main aspect is that
the current version as well as fairly recent ones require the axis
of statistical weight to be coded as 6 to indicate C3v
symmetry. In the only option line (line 3:)
s -1 1 0 35 0 6 2 2 0 1 0the numbers 6 2 2 together control the spin-statistics.