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Maria Grazia Bernardini, 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;very high-energy emission;
One of the central scientific goals of the next-generation Cherenkov Telescope Array (CTA) is the detection and characterization of gamma-ray bursts (GRBs). CTA will be sensitive to gamma rays with energies from about 20 GeV, up to a few hundred TeV. The energy range below 1 TeV is particularly ...
Leto: 2019 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
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