Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-27T10:46:48.837Z Has data issue: false hasContentIssue false
  • English
  • Français

100 GHz Room-Temperature Laboratory Emission Spectrometer

Published online by Cambridge University Press:  04 September 2018

Nadine Wehres ,
Bettina Heyne ,
Frank Lewen ,
Marius Hermanns ,
Bernhard Schmidt ,
Christian Endres ,
Urs U. Graf ,
Daniel R. Higgins  and
Stephan Schlemmer
Nadine Wehres
Affiliation:
I. Physics Institute, University of Cologne, Zülpicher Str. 77, 50937 Cologne, Germany email: wehres@ph1.uni-koeln.de; schlemmer@ph1.uni-koeln.de
Bettina Heyne
Affiliation:
I. Physics Institute, University of Cologne, Zülpicher Str. 77, 50937 Cologne, Germany email: wehres@ph1.uni-koeln.de; schlemmer@ph1.uni-koeln.de
Frank Lewen
Affiliation:
I. Physics Institute, University of Cologne, Zülpicher Str. 77, 50937 Cologne, Germany email: wehres@ph1.uni-koeln.de; schlemmer@ph1.uni-koeln.de
Marius Hermanns
Affiliation:
I. Physics Institute, University of Cologne, Zülpicher Str. 77, 50937 Cologne, Germany email: wehres@ph1.uni-koeln.de; schlemmer@ph1.uni-koeln.de
Bernhard Schmidt
Affiliation:
I. Physics Institute, University of Cologne, Zülpicher Str. 77, 50937 Cologne, Germany email: wehres@ph1.uni-koeln.de; schlemmer@ph1.uni-koeln.de
Christian Endres
Affiliation:
I. Physics Institute, University of Cologne, Zülpicher Str. 77, 50937 Cologne, Germany email: wehres@ph1.uni-koeln.de; schlemmer@ph1.uni-koeln.de
Urs U. Graf
Affiliation:
I. Physics Institute, University of Cologne, Zülpicher Str. 77, 50937 Cologne, Germany email: wehres@ph1.uni-koeln.de; schlemmer@ph1.uni-koeln.de
Daniel R. Higgins
Affiliation:
I. Physics Institute, University of Cologne, Zülpicher Str. 77, 50937 Cologne, Germany email: wehres@ph1.uni-koeln.de; schlemmer@ph1.uni-koeln.de
Stephan Schlemmer
Affiliation:
I. Physics Institute, University of Cologne, Zülpicher Str. 77, 50937 Cologne, Germany email: wehres@ph1.uni-koeln.de; schlemmer@ph1.uni-koeln.de
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present first results of a new heterodyne spectrometer dedicated to high-resolution spectroscopy of molecules of astrophysical importance. The spectrometer, based on a room-temperature heterodyne receiver, is sensitive to frequencies between 75 and 110 GHz with an instantaneous bandwidth of currently 2.5 GHz in a single sideband. The system performance, in particular the sensitivity and stability, is evaluated. Proof of concept of this spectrometer is demonstrated by recording the emission spectrum of methyl cyanide, CH3CN. Compared to state-of-the-art radio telescope receivers the instrument is less sensitive by about one order of magnitude. Nevertheless, the capability for absolute intensity measurements can be exploited in various experiments, in particular for the interpretation of the ever richer spectra in the ALMA era. The ease of operation at room-temperature allows for long time integration, the fast response time for integration in chirped pulse instruments or for recording time dependent signals. Future prospects as well as limitations of the receiver for the spectroscopy of complex organic molecules (COMs) are discussed.

Keywords

astrochemistrymolecular datamethods: laboratorytechniques: spectroscopic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S332: Astrochemistry VII: Through the Cosmos from Galaxies to Planets , March 2017 , pp. 332 - 345
Copyright
Copyright © International Astronomical Union 2018 

Footnotes

†

Present address: Max-Planck Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany

References

De Lucia, F. C., 2010, J. Molec. Spectrosc., 261, 1Google Scholar
Endres, C. P., Schlemmer, S., Schilke, P., Stutzki, J., & Müller, H. S. P., 2016, J. Molec. Spectrosc., 327, 95Google Scholar
Frisk, U., Hagström, M., Ala-Laurinaho, J., et al., 2003, A&A, 402, L27Google Scholar
Herbst, E. & van Dishoeck, E. F., 2009, ARAA, 47, 427Google Scholar
Higgins, R. D., Teyssier, D., Pearson, J. C., Risacher, C., & Trappe, N. A. 2010, Twenty-First International Symposium on Space Terahertz Technology, 390Google Scholar
Klein, B., Hochgürtel, S., Krämer, I., et al., 2012, A&A, 542, L3Google Scholar
Klein, B., Philipp, S. D., Krämer, I., et al., 2006, A&A, 454, L29Google Scholar
Medvedev, I. R. & De Lucia, F. C., 2007, ApJ, 656, 621Google Scholar
Müller, H. S. P., Schlöder, F., Stutzki, J., & Winnewisser, G., 2005, J. Mol. Struct., 742, 215Google Scholar
Müller, H. S. P., Thorwirth, S., Roth, D. A., & Winnewisser, G., 2001, A&A, 370, L49Google Scholar
Pickett, H. M., Poynter, R. L., Cohen, E. A., et al., 1998, JQSRT, 60, 883Google Scholar
Tanarro, I., Aleman, B., de Vicente, P., et al. 2017, submitted to A&A, private communicationGoogle Scholar
Teyssier, D., Dartois, E., Deboffle, D., et al. 2004, Fifteenth International Symposium on Space Terahertz Technology, 306Google Scholar
Tolls, V., Melnick, G. J., Ashby, M. L. N., et al., 2004, ApJS, 152, 137Google Scholar
Western, C. M., 2017, JQSRT, 186, 221Google Scholar