In this work, the effective fourth order Hamiltonian parameters of C-1
3 substituted methanol were determined using microwave (MW), millimete
rvave (MMW) and Fourier transform far-infrared (FIR) assigned transiti
ons in the ground and first excited torsional states. The data set con
sisted of 1060 transitions with the rotational angular momentum J < 13
(with 416 FIR lines). The data set was fitted with a recently develop
ed effective Hamiltonian model to derive the molecular parameters. The
results indicate that the model developed for the parent methanol spe
cies is valid for the C-13 substituted species also. The results will
allow the energy levels of the molecule to be calculated with improved
precision which will be of use for the discovery of new FIR laser emi
ssion in C-13 methanol and the discovery of this molecular species in
interstellar space. (C) 1997 Elsevier Science B.V.