Fourier-transform far-infrared spectra of (CH3OH)-O-18 in the 15-470 cm(-1) region have been analyzed by means of the Ritz assignment program. The far-infrared data have been combined with the literature microwave and millimeter-wave measurements in a full global fitting of the first three torsional states (v(t) = 0, 1, and 2) of the (CH3OH)-O-18 ground vibrational state. The fitted dataset includes 550 microwave and millimeter-wave lines and more than 17 000 Fourier-transform transitions covering the quantum number ranges J <= 30, K <= 15, and v(t) <= 2. With incorporation of 79 adjustable parameters, the global fit achieved convergence with an overall weighted standard deviation of 1.072, essentially to within the assigned measurement uncertainties of +/- 50 kHz for almost all of the microwave and millimeter-wave lines and +/- 6 MHz (0.0002 cm(-1)) to +/- 15 MHz (0.0005 cm(-1)) for the Fourier-transform far-infrared measurements. Based on the global fit results, a database has been compiled containing transition frequencies, quantum numbers, lower state energies and transition strengths. This database will provide support for present and future astronomical studies, such as the on-going Orion surveys in preparation for the launch of the Herschel Space Observatory, in identifying isotopic methanol contributions to interstellar spectra. (c) 2007 Elsevier Inc. All rights reserved.
Torsion-rotation global analysis and database for the (CH3OH)-O-18 isotopomer of methanol
MORUZZI, GIOVANNI;
2007-01-01
Abstract
Fourier-transform far-infrared spectra of (CH3OH)-O-18 in the 15-470 cm(-1) region have been analyzed by means of the Ritz assignment program. The far-infrared data have been combined with the literature microwave and millimeter-wave measurements in a full global fitting of the first three torsional states (v(t) = 0, 1, and 2) of the (CH3OH)-O-18 ground vibrational state. The fitted dataset includes 550 microwave and millimeter-wave lines and more than 17 000 Fourier-transform transitions covering the quantum number ranges J <= 30, K <= 15, and v(t) <= 2. With incorporation of 79 adjustable parameters, the global fit achieved convergence with an overall weighted standard deviation of 1.072, essentially to within the assigned measurement uncertainties of +/- 50 kHz for almost all of the microwave and millimeter-wave lines and +/- 6 MHz (0.0002 cm(-1)) to +/- 15 MHz (0.0005 cm(-1)) for the Fourier-transform far-infrared measurements. Based on the global fit results, a database has been compiled containing transition frequencies, quantum numbers, lower state energies and transition strengths. This database will provide support for present and future astronomical studies, such as the on-going Orion surveys in preparation for the launch of the Herschel Space Observatory, in identifying isotopic methanol contributions to interstellar spectra. (c) 2007 Elsevier Inc. All rights reserved.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.