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  4. The high-frequency upgrade of the Sardinia Radio Telescope
 
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The high-frequency upgrade of the Sardinia Radio Telescope

Author(s)
Govoni, F.
Bolli, P.
Buffa, F.
Caito, L.
Carretti, E.
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Date Issued
2021
Publisher
Institute of Electrical and Electronics Engineers Inc.
Abstract
We present the status of the Sardinia Radio Telescope (SRT) and its forthcoming update planned in the next few years. The post-process scenario of the upgraded infrastructure will allow the national and international scientific community to use the SRT for the study of the Universe at high radio frequencies (up to 116 GHz), both in single dish and in interferometric mode. A telescope like SRT, operating at high frequencies, represents a unique resource for the scientific community. The telescope will be ideal for mapping quickly and with relatively high angular resolution extended radio emissions characterized by low surface brightness. It will also be essential for spectroscopic and polarimetric studies of both Galactic and extragalactic radio sources. With the use of the interferometric technique, SRT and the other Italian antennas (Medicina and Noto) will operate within the national and international radiotelescope network, allowing astronomers to obtain images of radio sources at very high angular resolution. © 2021 URSI.
URI
https://hdl.handle.net/20.500.13025/6325
ISSN
9789463968027 (ISBN)
Journal
34th General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2021
DOI
10.23919/URSIGASS51995.2021.9560570
URL
https://ieeexplore.ieee.org/document/9560570/authors#authors
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