Spectroscopy of CH3OD (Ilyushin+, 2024) ================================================================================ Rotational spectroscopy of CH3OD with a re-analysis of CH3OD toward IRAS 16293 - 2422 V.V. Ilyushin, H.S.P. Muller, M.N. Drozdovskaya, J.K. Jorgensen, S. Bauerecker, C. Maul, R. Porohovoi, E.A. Alekseev, O. Dorovskaya, O. Zakharenko, F. Lewen, S. Schlemmer, L.-H. Xu, and R.M. Lees ================================================================================ ADC_Keywords: Interstellar medium; Spectra, millimetric/submm; Spectroscopy Keywords: Molecular data - Methods: laboratory: molecular - Techniques: spectroscopic - ISM: molecules - Astrochemistry - ISM: individual objects: IRAS 16293 - 2422 Abstract: We have started a measurement campaign of numerous methanol isotopologs in low-lying torsional states in order to provide extensive line lists for radio astronomical observations from an adequate spectroscopic model and to investigate how the intricate vibration-torsion-rotation interactions manifest themselves in the spectra of different isotopic species. After CD3OH and CD3OD, we turn our focus to CH3OD, which is an important species for studying deuteration in prestellar cores and envelopes that enshroud protostars. Deuteration, in turn, is frequently viewed as a diagnostic tool for star formation. The present measurements were obtained in two spectroscopic laboratories and cover large fractions of the 34 GHz-1.35 THz range. We employed a torsion-rotation Hamiltonian model for our analysis that is based on the rho-axis method as in previous studies. The resulting model describes the ground and first excited torsional states of CH3OD well up to quantum numbers J