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Naslov:Detection methods for the Cherenkov Telescope Array at very-short exposure times
Avtorji:ID Di Piano, Ambra (Avtor)
ID Bhattacharyya, Saptashwa (Avtor)
ID MARČUN, Barbara (Avtor)
ID Pérez Romero, Judit (Avtor)
ID Stanič, Samo (Avtor)
ID Vodeb, Veronika (Avtor)
ID Vorobiov, Serguei (Avtor)
ID Zaharijas, Gabrijela (Avtor)
ID Zavrtanik, Marko (Avtor)
ID Zavrtanik, Danilo (Avtor)
ID Živec, Miha (Avtor), et al.
Datoteke:.pdf ICRC2021_694.pdf (1,08 MB)
MD5: 23C992A9A872D1D2CB8DBAD7461A322F
 
URL https://pos.sissa.it/395/
 
URL https://pos.sissa.it/395/694/pdf
 
Jezik:Angleški jezik
Vrsta gradiva:Delo ni kategorizirano
Tipologija:1.08 - Objavljeni znanstveni prispevek na konferenci
Organizacija:UNG - Univerza v Novi Gorici
Opis:The Cherenkov Telescope Array (CTA) will be the next generation ground-based observatory for very-high-energy (VHE) gamma-ray astronomy, with the deployment of tens of highly sensitive and fast-reacting Cherenkov telescopes. It will cover a wide energy range (20 GeV - 300 TeV) with unprecedented sensitivity. To maximize the scientific return, the observatory will be provided with an online software system that will perform the first analysis of scientific data in real-time. This study investigates the precision and accuracy of available science tools and analysis techniques for the short-term detection of gamma-ray sources, in terms of sky localization, detection significance and, if significant detection is achieved, a first estimation of the integral photon flux. The scope is to evaluate the feasibility of the algorithms’ implementation in the real-time analysis of CTA. In this contribution we present a general overview of the methods and some of the results for the test case of the short-term detection of a gamma-ray burst afterglow, as the VHE counterpart of a gravitational wave event.
Ključne besede:very-high-energy gamma-rays, Cherenkov Telescope Array, gamma-ray astronomy
Status publikacije:Objavljeno
Leto izida:2021
PID:20.500.12556/RUNG-8420 Novo okno
COBISS.SI-ID:164772355 Novo okno
NUK URN:URN:SI:UNG:REP:VNYTRLHW
Datum objave v RUNG:18.09.2023
Število ogledov:1408
Število prenosov:7
Metapodatki:XML DC-XML DC-RDF
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Skupna ocena:(0 glasov)
Vaša ocena:Ocenjevanje je dovoljeno samo prijavljenim uporabnikom.
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Gradivo je del monografije

Naslov:37th International Cosmic Ray Conference : ICRC2021
Kraj izida:Trst, Italija
Leto izida:2021

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Licenca:CC BY-NC-ND 4.0, Creative Commons Priznanje avtorstva-Nekomercialno-Brez predelav 4.0 Mednarodna
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