J. Juryšek (Author), Christopher Eckner (Author), Gašper Kukec Mezek (Author), Samo Stanič (Author), Serguei Vorobiov (Author), Lili Yang (Author), Gabrijela Zaharijas (Author), Danilo Zavrtanik (Author), Marko Zavrtanik (Author), Lukas Zehrer (Author)

Abstract

The SST-1M telescope was developed as a prototype of a Small-Size-Telescope for the Cherenkov Telescope Array observatory and it has been extensively tested in Krakow since 2017. In this contribution we present validation of the Monte Carlo model of the prototype and expected performance in Krakow conditions. We focus on gamma/hadron separation and mono reconstruction of energy and gamma photon arrival direction using Machine learning methods.

Keywords

very-high-energy gamma rays;Cherenkov Telescope Array (CTA) Observatory;Small-Sized Telescopes (SSTs);SST-1M telescope prototype performance;Monte Carlo study;

Data

Language: English
Year of publishing:
Typology: 1.08 - Published Scientific Conference Contribution
Organization: UNG - University of Nova Gorica
UDC: 539.1
COBISS: 215237123 Link will open in a new window
ISSN: 1824-8039
Views: 178
Downloads: 4
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Other data

Pages: 8 str.
Chronology: 2019
DOI: 10.22323/1.358.0708
ID: 25396072
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