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http://hdl.handle.net/20.500.12386/34357
Title: | The high-frequency upgrade of the Sardinia Radio Telescope | Authors: | GOVONI, FEDERICA BOLLI, Pietro BUFFA, Franco CAITO, LETIZIA CARRETTI, ETTORE COMORETTO, Giovanni FIERRO, Davide MELIS, Andrea MURGIA, MATTEO NAVARRINI, Alessandro ORFEI, ALESSANDRO ORLATI, ANDREA PISANU, Tonino POPPI, Sergio POSSENTI, ANDREA ATTOLI, Alessandro BECCIANI, Ugo BELLI, Carolina Maria, Giuseppe Carboni Caria, Teresa CATTANI, ALESSANDRO CONCU, Raimondo CRESCI, Luca FARA, Antonietta Angela Rita FIOCCHI, FRANCO GAUDIOMONTE, Francesco LADU, Adelaide MACCAFERRI, ANDREA MARIOTTI, SERGIO MARONGIU, Pasqualino MIGONI, CARLO MOLINARI, Emilio Carlo MORSIANI, MARCO NESTI, Renzo OLMI, Luca PORCEDDU, Ignazio Enrico Pietro RIGHINI, SIMONA ORTU, Pierluigi PALMAS, STEFANO PILI, Mauro PODDIGHE, Antonio POLONI, MARCO RODA, JURI SCALAMBRA, ALESSANDRO SCHILLIRO', Francesco SCHIRRU , LUCA SERRA, Giampaolo SMAREGLIA, Riccardo VARGIU, GIAN PAOLO VITELLO, Fabio Roberto |
Issue Date: | 2021 | Journal: | ...URSI GENERAL ASSEMBLY AND SCIENTIFIC SYMPOSIUM | Volume: | 2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS) | First Page: | 1 | 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. | Conference Name: | 2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS) | Conference Place: | Rome, Italy | Conference Date: | 28 August 2021 - 04 September 2021 | URI: | http://hdl.handle.net/20.500.12386/34357 | URL: | https://api.elsevier.com/content/abstract/scopus_id/85118264581 https://ieeexplore.ieee.org/document/9560570 https://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=9560570 |
ISSN: | 2642-4339 | ISBN: | 9789463968027 | DOI: | 10.23919/URSIGASS51995.2021.9560570 | Fulltext: | open |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
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The_high-frequency_upgrade_of_the_Sardinia_Radio_Telescope.pdf | postprint | 212.37 kB | Adobe PDF | View/Open |
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