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

Povzetek

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.

Ključne besede

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

Podatki

Jezik: Angleški jezik
Leto izida:
Tipologija: 1.08 - Objavljeni znanstveni prispevek na konferenci
Organizacija: UNG - Univerza v Novi Gorici
UDK: 539.1
COBISS: 215237123 Povezava se bo odprla v novem oknu
ISSN: 1824-8039
Št. ogledov: 178
Št. prenosov: 4
Ocena: 0 (0 glasov)
Metapodatki: JSON JSON-RDF JSON-LD TURTLE N-TRIPLES XML RDFA MICRODATA DC-XML DC-RDF RDF

Ostali podatki

Strani: 8 str.
Čas izdaje: 2019
DOI: 10.22323/1.358.0708
ID: 25396072
Priporočena dela:
, ǂthe ǂworld’s largest VHE gamma-ray observatory
, layout, design and performance