Number of the records: 1
Prospects for Galactic transient sources detection with the Cherenkov Telescope Array
- 1.
SYSNO ASEP 0567962 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Prospects for Galactic transient sources detection with the Cherenkov Telescope Array Author(s) Abdalla, H. (ZA)
Abe, H. (JP)
Abe, S. (JP)
Araudo, Anabella Teresa (FZU-D) ORCID
Blažek, Jiří (FZU-D) ORCID, RID
Boháčová, Martina (FZU-D) RID, ORCID
Chudoba, Jiří (FZU-D) RID, ORCID
Ebr, Jan (FZU-D) RID, ORCID
Hamal, Petr (FZU-D) ORCID
Havelka, Matěj (FZU-D)
Janeček, Petr (FZU-D) RID, ORCID
Mandát, Dušan (FZU-D) RID, ORCID
Palatka, Miroslav (FZU-D) RID, ORCID, SAI
Pech, Miroslav (FZU-D) RID, ORCID
Prouza, Michael (FZU-D) RID, ORCID
Schovánek, Petr (FZU-D) RID, ORCID
Trávníček, Petr (FZU-D) RID, ORCID
Vícha, Jakub (FZU-D) RID, ORCID
Vraštil, Michal (FZU-D)Number of authors 1344 Article number 784 Source Title Proceedings of Science, International Cosmic Ray Conference (ICRC2021), 395. - Trieste : Sissa Medilab srl, 2022 - ISSN 1824-8039 Number of pages 19 s. Publication form Online - E Action International Cosmic Ray Conference (ICRC2021) /37./ Event date 12.07.2021 - 23.07.2021 VEvent location Berlin Country DE - Germany Event type WRD Language eng - English Country IT - Italy Keywords CTA ; galactic transient ; very-high-energy Subject RIV BF - Elementary Particles and High Energy Physics OECD category Particles and field physics R&D Projects EF18_046/0016007 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) EF16_013/0001403 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) LM2018105 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) LTT17006 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) LM2015046 GA MŠMT - Ministry of Education, Youth and Sports (MEYS) Institutional support FZU-D - RVO:68378271 DOI https://doi.org/10.22323/1.395.0784 Annotation 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. Workplace Institute of Physics Contact Kristina Potocká, potocka@fzu.cz, Tel.: 220 318 579 Year of Publishing 2023 Electronic address https://pos.sissa.it/395/784/pdf
Number of the records: 1