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The future of ground-based gamma-ray astronomy

  • Patrizia A. CaraveoEmail author
A decade of AGILE
  • 38 Downloads
Part of the following topical collections:
  1. A Decade of AGILE: Results, Challenges and Prospects of Gamma-Ray Astrophysics

Abstract

Ground-based gamma-ray astronomy is a young branch of high-energy astrophysics, addressing the highest energies in the electromagnetic spectrum. TeV photons cannot be produced by “ordinary” stars since they require quite extreme conditions, thus they allow the study of extreme astrophysical objects such as supernova remnants, neutron stars, black holes, both stellar and supermassive, as well as the elusive dark matter. To make it possible to go a step further in this exciting field, a world-wide collaboration is building the Cherenkov telescope array, an ambitious global observatory, to which the Italian community is strongly committed. The foreseen contribution of the Istituto Nazionale di Astrofisca (INAF) will be briefly outlined.

Keywords

High-energy astrophysics High-energy gamma-ray astronomy Cherenkov telescopes Cherenkov telescope array 

Notes

Compliance with ethical standards

Conflict of interest

I hereby declare that I have no conflict of interest.

References

  1. De Angelis A et al (2018) Science with e-ASTROGAM. A space mission for MeV-GeV gamma-ray astrophysics. J High Energy Astrophys 19:1CrossRefGoogle Scholar
  2. Giro E et al (2017) First optical validation of a Schwarzschild Couder telescope: the ASTRI SST-2 M Cherenkov telescope. Astron Astrophys 608:86CrossRefGoogle Scholar
  3. Pareschi G et al (2016) The ASTRI SST-2 M prototype and mini-array for the Cherenkov Telescope Array (CTA). Proc SPIE 9906:99065TCrossRefGoogle Scholar

Copyright information

© Accademia Nazionale dei Lincei 2019

Authors and Affiliations

  1. 1.IASF INAFMilanItaly

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