CaltechAUTHORS
  A Caltech Library Service

A Low Noise Receiver for Submillimeter Astronomy

Wengler, M. J. and Woody, D. P. and Miller, R. E. and Phillips, T. G. (1986) A Low Noise Receiver for Submillimeter Astronomy. In: Instrumentation for Submillimeter Spectroscopy. Proceedings of SPIE. No.598. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, pp. 27-32. ISBN 0892526335. https://resolver.caltech.edu/CaltechAUTHORS:20200311-161942632

[img] PDF - Published Version
See Usage Policy.

3410Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20200311-161942632

Abstract

A broadband, low noise heterodyne receiver, suitable for astronomical use, has been built using a Pb alloy superconducting tunnel junction (SIS). The RF coupling is quasioptical via a bowtie antenna on a quartz lens and is accomplished without any tuning elements. In its preliminary version the double sideband receiver noise temperature rises from 205 K at 116 GHz to 815 K at 466 GHz. This is the most sensitive broadband receiver yet reported for sub-mm wavelengths. Its multi-octave sensitivity and low local oscillator power requirements make this receiver ideal for remote ground observatories or space-borne telescopes such as NASA's Large Deployable Reflector. A version of this receiver is now being built for NASA's Kuiper Airborne Observatory.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.952315DOIArticle
Additional Information:© 1986 Society of Photo-Optical Instrumentation Engineers (SPIE). We are indebted to Dean Neikirk of the University of Texas and David Rutledge of Caltech for discussions about bowties which stimulated this project. At AT &T Bell Labs we thank A. A. Stark for help with SIS mask construction and M. V. Schneider and P. Verlangieri for Schottky diodes used in the LO multipliers. At Caltech we are pleased to acknowledge G. A. Blake's help in the lab and at the Owens Valley Radio Observatory.
Series Name:Proceedings of SPIE
Issue or Number:598
Record Number:CaltechAUTHORS:20200311-161942632
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200311-161942632
Official Citation:M. J. Wengler, D. P. Woody, R. E. Miller, and T. G. Phillips "A Low Noise Receiver for Submillimeter Astronomy", Proc. SPIE 0598, Instrumentation for Submillimeter Spectroscopy, (21 April 1986); https://doi.org/10.1117/12.952315
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:101887
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:12 Mar 2020 17:06
Last Modified:12 Mar 2020 17:06

Repository Staff Only: item control page