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Proceedings Paper

Millimetre And Submillimetre Receivers For The United Kingdom Infrared Telescope (UKIRT)
Author(s): R. W. Barker; D. W. J. Bly; M. J. Cox; R. E. Hills; J. A. Murphy; R. Padman; A. P. G. Russell; D. M. A . Wilson; S. Withington; D. R. Vizard
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Paper Abstract

Two receiver systems are described. The first is a 220-280 GHz dual-polarization system using cryogenically cooled Schottky-diode mixers pumped with a frequency-multiplied IMPATT local oscillator. The second is a 350 GHz indium antimonide array receiver which uses a novel quasi-optical LO injection scheme.

Paper Details

Date Published: 21 April 1986
PDF: 6 pages
Proc. SPIE 0598, Instrumentation for Submillimeter Spectroscopy, (21 April 1986); doi: 10.1117/12.952344
Show Author Affiliations
R. W. Barker, Mullard Radio Astronomy Observatory (England)
D. W. J. Bly, Mullard Radio Astronomy Observatory (England)
M. J. Cox, Mullard Radio Astronomy Observatory (England)
R. E. Hills, Mullard Radio Astronomy Observatory (England)
J. A. Murphy, Mullard Radio Astronomy Observatory (England)
R. Padman, Mullard Radio Astronomy Observatory (England)
A. P. G. Russell, Mullard Radio Astronomy Observatory (England)
D. M. A . Wilson, Mullard Radio Astronomy Observatory (England)
S. Withington, Mullard Radio Astronomy Observatory (England)
D. R. Vizard, Rutherford Appleton Laboratory (England)


Published in SPIE Proceedings Vol. 0598:
Instrumentation for Submillimeter Spectroscopy
Erik L. Kollberg, Editor(s)

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