Research Institutions

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

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

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

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

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

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

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

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

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