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ǂThe ǂCherenkov Telescope Array
Daniel Mazin, Christopher Eckner, Gašper Kukec Mezek, Samo Stanič, Serguei Vorobiov, Lili Yang, Gabrijela Zaharijas, Danilo Zavrtanik, Marko Zavrtanik, Lukas Zehrer
Objavljeni znanstveni prispevek na konferenci
Oznake: very-high-energy gamma-ray astronomy;Cherenkov Telescope Array;CTA sensitivity;gamma-ray bursts;POpulation Synthesis Theory Integrated project for very high-energy emission;
The Cherenkov Telescope Array (CTA) is the next generation ground-based observatory for gamma-ray astronomy at very-high energies. It will be capable of detecting gamma rays in the energy range from 20 GeV to more than 300 TeV with unprecedented precision in energy and directional reconstruction. ...
Leto: 2019 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
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