Abstract A balloon-borne, 1.2 meter Cassegrain telescope with a servo-controlled chopping secondary mirror has been developed and used to survey the Galactic Plane at submillimeter wavelengths. The telescope pointing system uses a gyroscope as the primary stabilization reference and makes use of microprocessors for pointing control, on-board data collection, and telemetry formatting. A description of the telescope, multi-channel liquid-helium-cooled focal plane and the aspect and orientation subsystems are presented.


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    Title :

    A large aperture balloon-borne telescope for a submillimeter wavelength survey of the galactic plane


    Contributors:
    Silverberg, R.F. (author) / Hauser, M.G. (author) / Walser, D.W. (author) / Flanick, A. (author) / Silver, A.D. (author) / Smith, J. (author) / Gezari, D.Y. (author) / Kelsall, T. (author) / Cheung, L.H. (author) / Skillman, T.L. Jr. (author)

    Published in:

    Publication date :

    1983-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



    A large aperture balloon-borne telescope for a submillimeter wavelength survey of the galactic plane

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