Paper
3 July 2000 The IRAM 230-GHz multibeam SIS receiver
Karl-Friedrich Schuster, Jaques Blondell, Yves Bortolotti, Matthew Carter, Bernard Fouilleux, Bernard Lazareff, Francois Mattiocco, Francis Morel, Alain Perrigouard, Jean-Louis Pollet
Author Affiliations +
Abstract
Heterodyne Multibeam receivers will boost the mapping performances of millimeter and submillimeter telescopes. The IRAM 30 m telescope will be equipped with an 18 channel SIS receiver for frequencies between 210 to 270 GHz. In this paper we discus the receiver system design and give arguments for the specific technological choices and their impacts on various observing modes. The electrical and cryogenic design of the receiver is presented and we discuss the theoretical and experimental performance of the receiver optics.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Karl-Friedrich Schuster, Jaques Blondell, Yves Bortolotti, Matthew Carter, Bernard Fouilleux, Bernard Lazareff, Francois Mattiocco, Francis Morel, Alain Perrigouard, and Jean-Louis Pollet "The IRAM 230-GHz multibeam SIS receiver", Proc. SPIE 4015, Radio Telescopes, (3 July 2000); https://doi.org/10.1117/12.390419
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Receivers

Telescopes

Mirrors

Polarization

Space telescopes

Cryogenics

Heterodyning

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