Paper
30 November 2017 A sub-millimetre wave SIS receiver for the James Clerk Maxwell Telescope
Author Affiliations +
Proceedings Volume 2250, International Conference on Millimeter and Submillimeter Waves and Applications 1994; 22507N (2017) https://doi.org/10.1117/12.2303292
Event: Millimeter and Submillimeter Waves and Applications: International Conference, 1994, San Diego, CA, United States
Abstract
We describe a Pb alloy superconducting (SIS) tunnel junction heterodyne receiver that has been constructed and tested over the frequency range 450 to 540 GHz and installed on the James Clerk Maxwell Telescope, Hawaii. The receiver uses a reduced height waveguide mount and a Pb alloy tunnel junction as the detecting element. Performance measurements made with the receiver installed on the telescope show a noise temperature (DSB) of 165 K at 460 GHz and 220 K at 490 GHz, measured in a 1 GHz instantaneous IF bandwidth centred at 4 GHz. The receiver demonstrates that Pb alloy junctions are sufficiently stable and reliable to allow use at a remote observing site at sub-millimetre wavelengths.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
B. N. Ellison "A sub-millimetre wave SIS receiver for the James Clerk Maxwell Telescope", Proc. SPIE 2250, International Conference on Millimeter and Submillimeter Waves and Applications 1994, 22507N (30 November 2017); https://doi.org/10.1117/12.2303292
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Receivers

Telescopes

Lead

Oscillators

Space telescopes

Niobium

Superconductors

RELATED CONTENT

Sis-mixers around the gap frequency
Proceedings of SPIE (January 01 1994)
A sub-millimetre wave SIS receiver
Proceedings of SPIE (August 30 1993)
A 275 to 370 GHz SIS mixer for the...
Proceedings of SPIE (October 08 2004)

Back to Top