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A field-deployed 810 GHz receiver incorporating a superconducting mixer developed for Herschel space telescope and a SiGe low noise amplifier

  • A. Hedden
  • , H. Li
  • , E. Tong
  • , S. Paine
  • , R. Blundell
  • , J. Kawamura
  • , C. Groppi
  • , C. Kulesa
  • , C. Walker
  • , G. De Lange
  • , H. Mani
  • , S. Weinreb

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

We have constructed an 810 GHz receiver system incorporating a HIFI Band-3 superconductor-insulator-superconductor (SIS) mixer developed for Herschel space observatory and a wide-band SiGe low noise amplifier (LNA) designed at Caltech. The instrument is currently installed at the RLT telescope (elevation 5500 m) in northern Chile. Hot/cold (280K/72K) load measurements performed at the telescope yield noise temperatures of 225 K (Y-factor = 1.7) including receiver optics. First-light observations indicate that the receiver is highly sensitive and functions stably. We present details of the receiver system, its performance at the telescope, and first-light observations with a Herschel mixer.

Original languageEnglish (US)
Title of host publicationIMS 2009 - 2009 IEEE MTT-S International Microwave Symposium Digest
Pages949-952
Number of pages4
DOIs
StatePublished - 2009
Event2009 IEEE MTT-S International Microwave Symposium, IMS 2009 - Boston, MA, United States
Duration: Jun 7 2009Jun 12 2009

Publication series

NameIEEE MTT-S International Microwave Symposium Digest
ISSN (Print)0149-645X

Other

Other2009 IEEE MTT-S International Microwave Symposium, IMS 2009
Country/TerritoryUnited States
CityBoston, MA
Period6/7/096/12/09

Keywords

  • IF amplifiers
  • Radio astronomy
  • Submillimeter wave measurements
  • Submillimeter wave receivers
  • Submillimeter wave spectroscopy
  • Superconductor insulator superconductor mixers

ASJC Scopus subject areas

  • Radiation
  • Condensed Matter Physics
  • Electrical and Electronic Engineering

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