100 GHz Room-Temperature Laboratory Emission Spectrometer
Autor: | Daniel R. Higgins, Urs U. Graf, Bettina Heyne, Marius Hermanns, Stephan Schlemmer, Bernhard Schmidt, Nadine Wehres, Christian P. Endres, Frank Lewen |
---|---|
Rok vydání: | 2017 |
Předmět: |
Heterodyne
Physics 010304 chemical physics Spectrometer business.industry Superheterodyne receiver FOS: Physical sciences Astronomy and Astrophysics 01 natural sciences law.invention 010309 optics Radio telescope Optics Space and Planetary Science law 0103 physical sciences Emission spectrum Astrophysics - Instrumentation and Methods for Astrophysics Spectroscopy business Compatible sideband transmission Instrumentation and Methods for Astrophysics (astro-ph.IM) Emission Spectrometer |
Zdroj: | Proceedings of the International Astronomical Union. 13:332-345 |
ISSN: | 1743-9221 1743-9213 |
DOI: | 10.1017/s1743921317007803 |
Popis: | We present first results of a new heterodyne spectrometer dedicated to high-resolution spectroscopy of molecules of astrophysical importance. The spectrometer, based on a roomtemperature 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. Comment: 14 pages, 7 figures, IAUS-332 Astrochemistry VII, Through the Cosmos from Galaxies to Planets, 2017 |
Databáze: | OpenAIRE |
Externí odkaz: | |
Nepřihlášeným uživatelům se plný text nezobrazuje | K zobrazení výsledku je třeba se přihlásit. |