20 June 2000 GREAT: the first-generation German heterodyne receiver for SOFIA
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A consortium of German research laboratories has been established for the development of a modular dual-channel heterodyne instrument (GREAT: German Receiver for Astronomy at Terahertz Frequencies) for high-resolution spectroscopy aboard SOFIA. The receiver is scheduled to be available in time for SOFIA's very first astronomical mission in late 2002. The first-flight version will offer opportunities for parallel observations in two frequency bands. We will have a choice of backends, including an acousto-optic array (4 X 1 GHz) and a high-resolution chirp transform spectrometer.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rolf Guesten, Rolf Guesten, Paul Hartogh, Paul Hartogh, Heinz-Wilhelm Huebers, Heinz-Wilhelm Huebers, Urs U. Graf, Urs U. Graf, K. Jacobs, K. Jacobs, Hans-Peter Roeser, Hans-Peter Roeser, Frank Schaefer, Frank Schaefer, Rudolf T. Schieder, Rudolf T. Schieder, Ronald Stark, Ronald Stark, Juergen Stutzki, Juergen Stutzki, Peter Van der Wal, Peter Van der Wal, Achim Wunsch, Achim Wunsch, } "GREAT: the first-generation German heterodyne receiver for SOFIA", Proc. SPIE 4014, Airborne Telescope Systems, (20 June 2000); doi: 10.1117/12.389122; https://doi.org/10.1117/12.389122

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