Upgrading of the L-P Band Cryogenic Receiver of the Sardinia Radio Telescope: A Feasibility Study

The Sardinia Radio Telescope is a quasi-Gregorian system with a shaped 64 m diameter primary reflector and a 7.9 m diameter secondary reflector. It was designed to operate with high efficiency across the 0.3–116 GHz frequency range. The telescope is equipped with a cryogenic coaxial dual-frequency L...

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Detalles Bibliográficos
Autores principales: Ladu, Adelaide, Schirru, Luca, Gaudiomonte, Francesco, Marongiu, Pasqualino, Angius, Gianmarco, Perini, Federico, Vargiu, Gian Paolo
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2022
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9185563/
https://www.ncbi.nlm.nih.gov/pubmed/35684881
http://dx.doi.org/10.3390/s22114261

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9185563/
https://www.ncbi.nlm.nih.gov/pubmed/35684881
http://dx.doi.org/10.3390/s22114261

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