4.2 Article

ASTRI Mini-Array core science at the Observatorio del Teide

Journal

JOURNAL OF HIGH ENERGY ASTROPHYSICS
Volume 35, Issue -, Pages 1-42

Publisher

ELSEVIER
DOI: 10.1016/j.jheap.2022.05.005

Keywords

ASTRI; Imaging atmospheric Cherenkov arrays; Very high-energy gamma ray astrophysics; Astroparticle

Funding

  1. Italian Ministry of Education, University and Research (MIUR)
  2. Brazilian Funding Agency FAPESP [2013/10559-5]
  3. South African Department of Science and Technology [0227/2014]
  4. H2020-ASTERICS - European Commission Framework Programme Horizon 2020 Research and Innovation action [653477]
  5. Spanish Ministry of Science and Innovation (MICIU)
  6. European Union's Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant [847523]
  7. Villum Fonden [18994]
  8. European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme [865637, 847648, LCF/BQ/PI21/11830030]
  9. la Caixa Foundation [100010434]

Ask authors/readers for more resources

The ASTRI Project led by INAF is developing the ASTRI Mini-Array, a small telescope array consisting of nine telescopes similar to ASTRI-Horn. The Mini-Array will surpass the current Cherenkov telescope array's sensitivity and extend the energy band well above hundreds of TeV.
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/).

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