MISTRAL is a millimetric camera working in the W-band (78–103 GHz) which will take data from the Sardinia Radio Telescope, the Italian 64-m radio telescope located 50 km form Cagliari, at 600m above the sea level, in Sardinia. It is being built as a facility instrument by the Sapienza University for INAF, that manages the radio telescope, under a PON contract. It will consist of a compact cryostat hosting the re–imaging optics, cooled at 4K, and a 408–pixel array of photon–noise limited lumped element kinetic inductance detectors fabricated at CNR-IFN and cooled at a base temperature lower than 300mK. MISTRAL will be able to investigate a long list of scientific targets spanning from extragalactic astrophysics to solar system science, with high angular resolution (~ 12 arcsec), including Sunyaev Zel’dovich effect measurements and the study of the Cosmic Web.

Millimetric Sardinia radio Telescope Receiver based on Array of Lumped elements kids / D'alessandro, G.; Barbarava, E.; Battistelli, E. S.; de Bernardis, P.; Cacciotti, F.; Capalbo, V.; Carretti, E.; Columbro, F.; Coppolecchia, A.; Cruciani, A.; De Petris, M.; Govoni, F.; Isopi, G.; Lamagna, L.; Marongiu, P.; Masi, S.; Mele, L.; Molinari, M.; Murgia, M.; Navarrini, A.; Orlati, A.; Paiella, A.; Pettinari, G.; Piacentini, F.; Pisanu, T.; Poppi, S.; Presta, G.; Radiconi, F.. - In: EPJ WEB OF CONFERENCES. - ISSN 2100-014X. - 257:(2022), p. 00012. [10.1051/epjconf/202225700012]

Millimetric Sardinia radio Telescope Receiver based on Array of Lumped elements kids

G. D'alessandro
Primo
;
E. S. Battistelli;P. de Bernardis;F. Cacciotti;V. Capalbo;F. Columbro;A. Coppolecchia;A. Cruciani;M. De Petris;G. Isopi;L. Lamagna;S. Masi;L. Mele;A. Paiella;F. Piacentini;G. Presta;F. Radiconi
2022

Abstract

MISTRAL is a millimetric camera working in the W-band (78–103 GHz) which will take data from the Sardinia Radio Telescope, the Italian 64-m radio telescope located 50 km form Cagliari, at 600m above the sea level, in Sardinia. It is being built as a facility instrument by the Sapienza University for INAF, that manages the radio telescope, under a PON contract. It will consist of a compact cryostat hosting the re–imaging optics, cooled at 4K, and a 408–pixel array of photon–noise limited lumped element kinetic inductance detectors fabricated at CNR-IFN and cooled at a base temperature lower than 300mK. MISTRAL will be able to investigate a long list of scientific targets spanning from extragalactic astrophysics to solar system science, with high angular resolution (~ 12 arcsec), including Sunyaev Zel’dovich effect measurements and the study of the Cosmic Web.
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11573/1603628
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