3 July 2000 Submillimeter-wave receiver system for the Large Binocular Telescope
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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 micrometer 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.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christian Y. Drouet d'Aubigny, Christian Y. Drouet d'Aubigny, Christopher K. Walker, Christopher K. Walker, Christopher E. Groppi, Christopher E. Groppi, John M. Hill, John M. Hill, John H. Bieging, John H. Bieging, Stephen M. Pompea, Stephen M. Pompea, } "Submillimeter-wave receiver system for the Large Binocular Telescope", Proc. SPIE 4015, Radio Telescopes, (3 July 2000); doi: 10.1117/12.390421; https://doi.org/10.1117/12.390421


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