Description

Transition frequencies with microwave accuracy were determined by
(1) D. Dangoisse, E. Willemot, and J. Bellet, 1978, J. Mol. Spectrosc. 71, 414;
and by
(2) O. Zakharenko, R. A. Motiyenko, L. Margulès, and T. R. Huet, 2015, J. Mol. Spectrosc. 317, 41.
Some higher order parameters were estimated from the D2CO parameters.
The uncertainties of (2) appeared to be quite conservative. Therefore, we decreased these uncertainties by a factor of 1.5. The data from (1) have not been merged.
The predictions of very high lying rotational states have been improved with respect to the first entry. The predictions should be adequate throughout not only for astronomical observations but also for laboratory spectroscopy.
At low temperatures, it may be necessary to discern between ortho-D2CO and para-D2CO. The ortho states are described by Ka even, the para states by Ka odd. The nuclear spin-weight ratio is 2:1 for ortho-D213CO : para-D213CO. The JKaKc = 111 is the lowest para state. It is 5.5608cm–1 above ground.
The dipole moment was assumed to agree with that of D2CO, see e032502.cat.