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Wide-Band Tunerless Mixer Mounts for 100 GHz and 150 GHz SIS receivers

Published online by Cambridge University Press:  12 April 2016

K. Sunada ,
R. Kawabe  and
J. Inatani
K. Sunada
Affiliation:
Nobeyama Radio Observatory, Nobeyaina, Minamimaki, Minamisaku, Nagano, 384-13, Japan
R. Kawabe
Affiliation:
Nobeyama Radio Observatory, Nobeyaina, Minamimaki, Minamisaku, Nagano, 384-13, Japan
J. Inatani
Affiliation:
Nobeyama Radio Observatory, Nobeyaina, Minamimaki, Minamisaku, Nagano, 384-13, Japan

Abstract

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The performance of the new SIS receiver systems at the Nobeyama Millimeter Array are described. These receivers operate at 100 GHz and 150 GHz bands and tunerless mixer mounts have been adopted. These receivers show very low noise temperature (< 50 K) over a very wide frequency range because of the large embedding impedance range.

Type
2. Technical Innovations
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 78 - 81
Copyright
Copyright © Astronomical Society of the Pacific 1994

References

D’Addano, L.R., 1984, Int. J. of IR and MM Waves, vol. 5,1419 Google Scholar
Hicks, R.G., Feldman, M.J., and Kerr, A.R., 1986, NASA Technical Memorandum 86145 Google Scholar
Tucker, J.R., 1979, IEEE Jnl. Quantum Electronics, vol. QE-15, 1234 Google Scholar