The pure rotational spectra of all possible O-17-monosubstituted ozone
species have been investigated at selected frequencies in the range f
rom 49 to 393 GHz. Accurate rotational and centrifugal distortion para
meters up to the sextic terms have been determined using the Watson's
Hamiltonian in its A-reduced form. Comparisons are made between experi
mental values and those obtained from the force field calculations. (C
) 1995 Academic Press, Inc.