ASTRI Mini-Array core science at the Observatorio del Teide

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Vercellone, S. ; Bigongiari, C. ; Burtovoi, A. ; Cardillo, M. ; Catalano, O. ; Franceschini, A. ; Lombardi, S. ; Nava, L. ; Pintore, F. ; Stamerra, A. ; Tavecchio, F. ; Zampieri, L. ; Batista, R. Alves ; Amato, E. ; Antonelli, L. A. ; Arcaro, C. ; Gonzalez, J. Becerra ; Bonnoli, G. ; Boettcher, M. ; Brunetti, G. ; Compagnino, A. A. ; Crestan, S. ; D'Ai, A. ; Fiori, M. ; Galanti, G. ; Giuliani, A. ; Dal Pino, E. M. de Gouveia ; Green, J. G. ; Lamastra, A. ; Landoni, M. ; Lucarelli, F. ; Morlino, G. ; Olmi, B. ; Peretti, E. ; Piano, G. ; Ponti, G. ; Poretti, E. ; Romano, P. ; Saturni, F. G. ; Scuderi, S. ; Tutone, A. ; Umana, G. ; Acosta-Pulido, J. A. ; Barai, P. ; Bonanno, A. ; Bonanno, G. ; Bruno, P. ; Bulgarelli, A. ; Conforti, V. ; Costa, A. ; Cusumano, G. ; Del Santo, M. ; del Valle, M. V. ; Della Ceca, R. ; Falceta-Goncalves, D. A. ; Fioretti, V. ; Germani, S. ; Garcia-Lopez, R. J. ; Ghedina, A. ; Gianotti, F. ; Giordano, V. ; Kreter, M. ; Incardona, F. ; Iovenitti, S. ; La Barbera, A. ; La Palombara, N. ; La Parola, V. ; Leto, G. ; Longo, F. ; Lopez-Oramas, A. ; Maccarone, M. C. ; Mereghetti, S. ; Millul, R. ; Naletto, G. ; Pagliaro, A. ; Parmiggiani, N. ; Righi, C. ; Rodriguez-Ramirez, J. C. ; Romeo, G. ; Sangiorgi, P. ; de Lima, R. Santos ; Tagliaferri, G. ; Testa, V. ; Tosti, G. ; Acosta, M. Vazquez ; Zywucka, N. ; Caraveo, P. A. ; Pareschi, G.

• Document type: Journal article
• Source: JOURNAL OF HIGH ENERGY ASTROPHYSICS; v. 35, p. 42-pg., 2022-06-10.

Abstract

The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the Observatorio del Teide a mini-array (ASTRI Mini-Array) composed of nine telescopes similar to the small-size dual-mirror Schwarzschild-Couder telescope (ASTRI-Horn) currently operating on the slopes of Mt. Etna in Sicily. The ASTRI Mini-Array will surpass the current Cherenkov telescope array differential sensitivity above a few teraelectronvolt (TeV), extending the energy band well above hundreds of TeV. This will allow us to explore a new window of the electromagnetic spectrum, by convolving the sensitivity performance with excellent angular and energy resolution figures. In this paper we describe the Core Science that we will address during the first four years of operation, providing examples of the breakthrough results that we will obtain when dealing with current open questions, such as the acceleration of cosmic rays, cosmology and fundamental physics and the new window, for the TeV energy band, of the time-domain astrophysics. (c) 2022 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/). (AU)

• FAPESP's process: 13/10559-5 - Investigation of high energy and plasma astrophysics phenomena: theory, numerical simulations, observations, and instrument development for the Cherenkov Telescope Array (CTA)
• Grantee: Elisabete Maria de Gouveia Dal Pino
• Support Opportunities: Special Projects