| Naslov: | Prospects for Galactic transient sources detection with the Cherenkov Telescope Array |
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| Avtorji: | ID López-Oramas, Alicia (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. |
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| Datoteke: |  ICRC2021_784.pdf (1,57 MB)
MD5: EF7A2A7EA32FA4C68DBA219D7D244D44
 https://pos.sissa.it/395/
https://pos.sissa.it/395/784/pdf
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| Jezik: | Angleški jezik |
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| Vrsta gradiva: | Delo ni kategorizirano |
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| Tipologija: | 1.08 - Objavljeni znanstveni prispevek na konferenci |
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| Organizacija: | UNG - Univerza v Novi Gorici
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| Opis: | Several types of Galactic sources, like magnetars, microquasars, novae or pulsar wind nebulae flares, display transient emission in the X-ray band. Some of these sources have also shown emission at MeV–GeV energies. However, none of these Galactic transients have ever been detected in the very-high-energy (VHE; E>100 GeV) regime by any Imaging Air Cherenkov Telescope (IACT). The Galactic Transient task force is a part of the Transient Working group of the Cherenkov Telescope Array (CTA) Consortium. The task force investigates the prospects of detecting the VHE counterpart of such sources, as well as their study following Target of Opportunity (ToO) observations. In this contribution, we will show some of the results of exploring the capabilities of CTA to detect and observe Galactic transients; we assume di˙erent array configurations and observing strategies. |
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| Ključne besede: | Cherenkov Telescope Array, galactic transient sources, very-high energy gamma rays |
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| Status publikacije: | Objavljeno |
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| Leto izida: | 2021 |
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| PID: | 20.500.12556/RUNG-8429  |
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| COBISS.SI-ID: | 164863747 |
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| NUK URN: | URN:SI:UNG:REP:MNXUWFKD |
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| Datum objave v RUNG: | 18.09.2023 |
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| Število ogledov: | 1302 |
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| Število prenosov: | 5 |
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| Metapodatki: |     |
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