Sensitivity of the Cherenkov Telescope Array to TeV photon emission from the large Magellanic Cloud

0577863 - FZÚ 2024 RIV US eng J - Článek v odborném periodiku
Acharyya, A. - Adam, R. - Aguasca-Cabot, A. - Hamal, Petr - Juryšek, Jakub - Karas, Vladimír - Mandát, Dušan - Palatka, Miroslav - Pech, Miroslav - Schovánek, Petr - Tavernier, Thomas … celkem 336 autorů
Sensitivity of the Cherenkov Telescope Array to TeV photon emission from the large Magellanic Cloud.
Monthly Notices of the Royal Astronomical Society. Roč. 523, č. 4 (2023), s. 5353-5387. ISSN 0035-8711. E-ISSN 1365-2966
Grant CEP: GA MŠMT LTT17006; GA MŠMT EF16_013/0001403; GA MŠMT(CZ) EF18_046/0016007
Výzkumná infrastruktura: CTA-CZ II - 90105
Institucionální podpora: RVO:68378271 ; RVO:67985815
Klíčová slova: acceleration of particles * Magellanic Clouds * dark matter * gamma-rays: general
Obor OECD: Particles and field physics; Particles and field physics (ASU-R)
Impakt faktor: 4.8, rok: 2022
Způsob publikování: Omezený přístup
https://doi.org/10.1093/mnras/stad1576

A deep survey of the Large Magellanic Cloud at & SIM:0.1-100 TeV photon energies with the Cherenkov Telescope Array is planned. We assess the detection prospects based on a model for the emission of the galaxy, comprising the four known TeV emitters, mock populations of sources, and interstellar emission on galactic scales. We also assess the detectability of 30 Doradus and SN 1987A, and the constraints that can be derived on the nature of dark matter. The survey will allow for fine spectral studies of N 157B, N 132D, LMC P3, and 30 Doradus C, and half a dozen other sources should be revealed, mainly pulsar-powered objects. The remnant from SN 1987A could be detected if it produces cosmic-ray nuclei with a flat power-law spectrum at high energies, or with a steeper index 2.3-2.4 pending a flux increase by a factor of >3-4 over & SIM:2015-2035.
Trvalý link: https://hdl.handle.net/11104/0346958