Towards the ASTRI mini-array

The Cherenkov Telescope Array (CTA) will consist of an array of three types of telescopes covering a wide energy range, from tens of GeV up to more than 100 TeV. The high energy section (> 3 TeV) will be covered by the Small Size Telescopes (SST). ASTRI (Astrofisica con Specchi a Tecnologia Repli...

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Hauptverfasser: Di Pierro, F, Bigongiari, C, Morello, C, Stamerra, A, Vallania, P, Agnetta, G, Antonelli, L. A, Bastieri, D, Bellassai, G, Belluso, M, Billotta, S, Biondo, B, Bonanno, G, Bonnoli, G, Bruno, P, Bulgarelli, A, Canestrari, R, Capalbi, M, Caraveo, P, Carosi, A, Cascone, E, Catalano, O, Cereda, M, Conconi, P, Conforti, V, Cusumano, G, De Caprio, V, De Luca, A, Di Paola, A, Fantinel, D, Fiorini, M, Fugazza, D, Gardiol, D, Ghigo, M, Gianotti, F, Giarrusso, S, Giro, E, Grillo, A, Impiombato, D, Incorvaia, S, La Barbera, A, La Palombara, N, La Parola, V, La Rosa, G, Lessio, L, Leto, G, Lombardi, S, Lucarelli, F, Maccarone, M. C, Malaguti, G, Malaspina, G, Mangano, V, Marano, D, Martinetti, E, Millul, R, Mineo, T, Misto, A, Morlino, G, Panzera, M. R, Pareschi, G, Rodeghiero, G, Romano, P, Russo, F, Sacco, B, Sartore, N, Schwarz, J, Segreto, A, Sironi, G, Sottile, G, Strazzeri, E, Stringhetti, L, Tagliaferri, G, Testa, V, Timpanaro, M. C, Toso, G, Tosti, G, Trifoglio, M, Vercellone, S, Zitelli, V, Consortium, The Cta
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Zusammenfassung:The Cherenkov Telescope Array (CTA) will consist of an array of three types of telescopes covering a wide energy range, from tens of GeV up to more than 100 TeV. The high energy section (> 3 TeV) will be covered by the Small Size Telescopes (SST). ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) is a flagship project of the Italian Ministry of Research and Education led by INAF, aiming at the design and construction of a prototype of the Dual Mirror SST. In a second phase the ASTRI project foresees the installation of the first elements of the SST array at the CTA southern site, a mini-array of 5-7 telescopes. The optimization of the layout of this mini-array embedded in the SST array of the CTA Observatory has been the object of an intense simulation effort. In this work we present the expected mini-array performance in terms of energy threshold, angular and energy resolution and sensitivity.
DOI:10.48550/arxiv.1307.3992