Abstract
Context. Astronomical surveys of interstellar molecules, such as those that will be available with the very sensitive ALMA telescope, require preliminary laboratory investigations of the microwave and submillimeter-wave spectra of new molecular species to identify these in the interstellar media. Aims. We build a linelist that should allow us to detect HCOOCD2H, provided it is present in the interstellar media in a suitable concentration. Methods. The experimental spectra of HCOOCD2H have been recorded in the microwave and submillimeter-wave energy range. Line frequencies were analyzed using an internal axis method-like treatment taking into account the CD2H internal rotation. Results. 5933 lines of HCOOCD2H have been assigned and their frequencies were reproduced with a unitless standard deviation of 1.6. A linelist with calculated frequencies and intensities was built and spans the 50-660 GHz spectral region. The frequency accuracy is better than 0.1 MHz. Conclusions. The pure rotation spectrum of the CD2H-methyl formate isotopolog (HCOOCD2H) has been observed in laboratory for the first time. © 2012 ESO.
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Coudert, L. H., Margulès, L., Huet, T. R., Motiyenko, R. A., Møllendal, H., & Guillemin, J. C. (2012). The submillimeter-wave spectrum of the doubly deuterated species of methyl formate HCOOCD2H. Astronomy and Astrophysics, 543. https://doi.org/10.1051/0004-6361/201219120
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