Abstract
A 220–280 GHz prototype SIS receiver system is currently being constructed, which will be tested on the JCMT in January 1989. The prototype receiver will act as a test-bed for developing a dualchannel common-user SIS receiver for the JCMT, tunable from 280–360 GHz, in a collaborative project between UKC, RAL and the Herzberg Institute of Astrophysics, Ottawa.
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References
Davies, S.R., Little, L.T., and Cunningham, C.T.: Electronics Letters 23, 946 (1987).
Davies, S.R., and Little, L.T.: (in preparation).
Tucker, J.R., and Feldman, M.J.: Rev. Mod. Phys. 57, 1055 (1985).
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© 1990 Springer Science+Business Media Dordrecht
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Davies, S.R., Cunningham, C.T., Little, L.T., Matheson, D.N. (1990). An SIS Receiver for the JCMT. In: Watt, G.D., Webster, A.S. (eds) Submillimetre Astronomy. Astrophysics and Space Science Library, vol 158. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-6850-0_27
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DOI: https://doi.org/10.1007/978-94-015-6850-0_27
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