Prospects for Galactic transient sources detection with the Cherenkov Telescope Array

Autor: López-Oramas, Alicia, Bulgarelli, Andrea, Mestre, Enrique, Di Piano, Ambra, Romano, Patrizia, Sadeh, Iftach, Sergijenko, Olga, Sidoli, Lara, Spolon, Alessia, de Oña Wilhelmi, Emma, Piano, Giovanni, Zampieri, Luca, Chaty, Sylvain, Consortium, CTA, Chernyakova, Maria, Gnatyk, Roman, Hnatyk, Bodhan, Kantzas, Dimitris, Markoff, Sera, McKeague, Samuel, Mereghetti, Sandro
Přispěvatelé: API (FNWI), High Energy Astrophys. & Astropart. Phys (API, FNWI), Faculty of Science, GRAPPA (ITFA, IoP, FNWI), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), CTA Consortium, Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Jazyk: angličtina
Rok vydání: 2021
Předmět:
Zdroj: Proceedings of Science / International School for Advanced Studies (ICRC2021), 784 (2021). doi:10.22323/1.395.0784
37th International Cosmic Ray Conference, ICRC 2021, Berlin, Germany, 2021-07-15-2021-07-22
Proceedings of Science, 395:784. Sissa Medialab Srl
PoS
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.784, ⟨10.22323/1.395.0784⟩
ISSN: 1824-8039
DOI: 10.22323/1.395.0784
Popis: 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 different array configurations and observing strategies.
37th International Cosmic Ray Conference (ICRC2021)
Databáze: OpenAIRE
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