Submillimeter-wave receiver system for the large binocular telescope

Christian Y Drouet d'Aubigny, Christopher K. Walker, Christopher Groppi, John M. Hill, John H. Bieging, Steven M. Pompea

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

4 Scopus citations

Abstract

The Large Binocular Telescope (LBT) will consist of two, 8.417 m, spin-cast, optical quality primary mirrors on a common azimuth-elevation mount. The center-to-center distance between the primaries is 14.417 m. The LBT is being constructed on a site known to have relatively low atmospheric opacity at submillimeter wavelengths. In this paper we describe a unique 350 μm heterodyne receiver system designed for use on the LBT. The optical quality of the primaries and their size will give the LBT a light gathering power more than twice that of existing submillimeter-wave telescopes.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
PublisherSociety of Photo-Optical Instrumentation Engineers
Pages268-277
Number of pages10
Volume4015
StatePublished - 2000
EventRadio Telescopes - Munich, Ger
Duration: Mar 27 2000Mar 30 2000

Other

OtherRadio Telescopes
CityMunich, Ger
Period3/27/003/30/00

ASJC Scopus subject areas

  • Electrical and Electronic Engineering
  • Condensed Matter Physics

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  • Cite this

    d'Aubigny, C. Y. D., Walker, C. K., Groppi, C., Hill, J. M., Bieging, J. H., & Pompea, S. M. (2000). Submillimeter-wave receiver system for the large binocular telescope. In Proceedings of SPIE - The International Society for Optical Engineering (Vol. 4015, pp. 268-277). Society of Photo-Optical Instrumentation Engineers.