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Research Institutions

  • Waveguide

    Waveguide

    We manufacture waveguides in several material according to customer design

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  • SRT

    SRT

     The Sardinia Radio Telescope is the largest Italian Telescope, located in San Basilio near Cagliari. This telescope was built after…

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  • 18-26 GHz MultiFeed Receiver

    18-26 GHz MultiFeed Receiver

    This cryogenic 22hz Multi – Feed receiver (completed and tested on the 32m antenna of Medicina) is now being used…

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  • DUAL FEED 18-26 GHz RECEIVER

    DUAL FEED 18-26 GHz RECEIVER

    The Dual Feed receiver is an exact replica of the Multifeed receiver; it is cryogenic too and has the same…

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  • 43GHz RECEIVER

    43GHz RECEIVER

    43Ghz cryogenic receiver. This receiver is at the moment being used in the secondary focus of the Noto Antenna at…

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  • OMT 43GHz

    OMT 43GHz

    The OMTs (OrthoMode Transducers) are passive components of front-ends of radio receivers, used in radio astronomy to separate orthogonal components…

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  • OMT 100 GHz

    OMT 100 GHz

    The OMTs (OrthoMode Transducers) are passive components of front-ends of radio receivers, used in radio astronomy to separate orthogonal components…

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  • LSPE

    LSPE

    The LSPE (Large Scale Polarization Explorer ) is a balloon-borne mission aimed at measuring the polarization of the Cosmic Microwave…

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  • FEED

    FEED

    Feeds are the first passive components of the front end of radio receivers used to join the receiver with the…

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  • DEWAR

    DEWAR

    An example of cubic vacuum chamber made by Cloema for the cryogenic microwave testing and operative at the radio laboratories…

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