Počet záznamů: 1  

Status of the large size telescopes and medium size telescopes for the Cherenkov Telescope Array observatory

  1. 1.
    0538422 - FZÚ 2021 RIV NL eng J - Článek v odborném periodiku
    Barrio, J.A. - Abdalla, H. - Acero, F. - Blažek, Jiří - Boháčová, Martina - Chudoba, Jiří - Ebr, Jan - Hamal, Petr - Janeček, Petr - Juryšek, Jakub - Mandát, Dušan - Palatka, Miroslav - Pech, Miroslav - Prouza, Michael - Schovánek, Petr - Trávníček, Petr - Vraštil, Michal - Vícha, Jakub … celkem 1251 autorů
    Status of the large size telescopes and medium size telescopes for the Cherenkov Telescope Array observatory.
    Nuclear Instruments & Methods in Physics Research Section A. Roč. 952, Feb (2020), s. 1-4, č. článku 161588. ISSN 0168-9002. E-ISSN 1872-9576
    Grant CEP: GA MŠMT(CZ) EF18_046/0016007; GA MŠMT EF16_013/0001403; GA MŠMT(CZ) LM2018105; GA MŠMT LTT17006; GA MŠMT LM2015046
    Grant ostatní: OP VVV - CTA-CZ II(XE) CZ.02.1.01/0.0/0.0/18_046/0016007; OP VVV - CTAO-CZ(XE) CZ.02.1.01/0.0/0.0/16_013/0001403
    Institucionální podpora: RVO:68378271
    Klíčová slova: astroparticle physics * gamma-ray astronomy * Imaging Atmospheric Cherenkov Telescopes
    Obor OECD: Astronomy (including astrophysics,space science)
    Impakt faktor: 1.455, rok: 2020
    Způsob publikování: Omezený přístup
    https://doi.org/10.1016/j.nima.2018.11.047

    The Cherenkov Telescope Array (CTA) is the next generation of ground-based observatory in the Very High Energy (VHE) gamma-ray domain. The observatory, operating in an open, all-sky mode, will consist of two sites, one in the Northern Hemisphere, at Observatorio Roque de los Muchachos (La Palma, Spain), and another in the Southern Hemisphere. CTA will implement Imaging Atmospheric Cherenkov Telescopes (IACTs) of large, medium and small size, mapping the VHE sky with an unprecedented sensitivity in an extended energy range. In its baseline design, 4 Large Size Telescopes (LSTs) will operate in coincidence in each site, dominating the CTA sensitivity in the 20 GeV – 150 GeV gamma-ray band, while the CTA core energy range, from 150 GeV to 5000 GeV, will be best covered by Medium Size Telescopes (MSTs), 25 in CTA-South and 15 in CTA-North.
    Trvalý link: http://hdl.handle.net/11104/0316501

     
     
Počet záznamů: 1  

  Tyto stránky využívají soubory cookies, které usnadňují jejich prohlížení. Další informace o tom jak používáme cookies.