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    Wyświetlanie 1-5 z 5
    Tytuł:
    The SST-1M project for the Cherenkov Telescope Array
    Autorzy:
    Hamal, P.
    Niemiec, J.
    Barbano, A. M.
    Renier, Y.
    Michalowski, J.
    Travnicek, P.
    Mach, E.
    Grudzińska, M.
    Pech, M.
    Blazek, J.
    Świerblewski, J.
    Nagai, A.
    Cadoux, F. R.
    Bulik, T.
    Alispach, C. M.
    Samarai, I. Al
    Jurysek, J.
    Palatka, M.
    Kotarba, A.
    Heller, M.
    Ostrowski, Michał
    Seweryn, K.
    Favre, Y.
    Kasperek, J.
    Njoh Ekoume, T. R.
    Walter, R.
    Troyano Pujadas, I.
    Błocki, J.
    Lyard, É.
    Stawarz, Łukasz
    Borkowski, J.
    Moderski, R.
    Balbo, M.
    Świerk, P.
    Beshley, V.
    Della Volpe, D.
    Michal, S.
    Pasko, P.
    Przybilski, H.
    Smakulska, D.
    Sobczyńska, D.
    Wiecek, M.
    Koncewicz, K.
    Rajda, P.
    Ziętara, Krzysztof
    Schovanek, P.
    Sliusar, V.
    De Angelis, N.
    Montaruli, T.
    Biland, A.
    Pilszyk, B.
    Coco, V.
    Gieras, T.
    Rozwadowski, P.
    Neise, D.
    Mandat, D.
    Hrabovsky, M.
    Chytka, L.
    Zagdański, Aleksander
    Opis:
    The SST-1M project, run by a Consortium of institutes from Czech Republic, Poland and Switzerland, has been proposed as a solution for implementing the small-size telescope array of the southern site of the Cherenkov Telescope Array. The technology is a pathfinder for efficient production of cost-effective imaging air Cherenkov telescopes. We report on the main system features and recent upgrades, the performances validation and the operation campaign carried out in 2018.
    Dostawca treści:
    Repozytorium Uniwersytetu Jagiellońskiego
    Inne
    Tytuł:
    The SST-1M imaging atmospheric Cherenkov telescope for gamma-ray astrophysics
    Autorzy:
    Rajda, P.
    Montaruli, T.
    Stodulska, M.
    Prouza, M.
    Gieras, T.
    Balbo, M.
    Chytka, L.
    Gibaud, L.
    Nikołajuk, M.
    Vacula, M.
    Favre, Y.
    Pech, M.
    Araudo, A.
    Bulik, T.
    Garczarczyk, M.
    Novotný, V.
    Štrobl, J.
    Walter, R.
    Heller, M.
    Casanova, S.
    Della Volpe, D.
    Michal, S.
    Stawarz, Łukasz
    Chudoba, J.
    Niemiec, J.
    Neise, D.
    Seweryn, K.
    Świerk, P.
    Trávníček, P.
    Nalewajski, K.
    Christov, A.
    Ostrowski, Michał
    Troyano Pujadas, I.
    Hamal, P.
    Cadoux, F.
    Marek, W.
    Schovanek, P.
    Tavernier, T.
    Blažek, J.
    Lacave, B.
    Mandát, D.
    Ziętara, Krzysztof
    Juryšek, J.
    Müller, A.L.
    Beshley, V.
    Janeček, P.
    Świerblewski, J.
    Moderski, R.
    Biland, A.
    Lyard, E.
    Hrabovský, M.
    Jelínek, M.
    Mach, E.
    Vícha, J.
    Palatka, M.
    Muthyala, S.
    Sliusar, V.
    Sternberger, R.
    Michałowski, J.
    Borkowski, J.
    Dědič, P.
    Nagai, A.
    Alispach, C.
    Muraczewski, A.
    Karas, V.
    Jílek, V.
    Opis:
    The SST-1M (webpage: https://sst-1m.space) is a Small-Sized Telescope (SST) designed to provide a cost-effective and high-performance solution for gamma-ray astrophysics, particularly for energies beyond a few TeV. The goal is to integrate this telescope into an array of similar instruments, leveraging its lightweight design, earthquake resistance, and established Davies-Cotton configuration. Additionally, its optical system is designed to function without a protective dome, allowing it to withstand the harsh atmospheric conditions typical of mountain environments above 2000 m a.s.l. The SST-1M utilizes a fully digitizing camera system based on silicon photomultipliers (SiPMs). This camera is capable of digitizing all signals from the UV-optical light detectors, allowing for the implementation of various triggers and data analysis methods. We detail the process of designing, prototyping, and validating this system, ensuring that it meets the stringent requirements for gamma-ray detection and performance. An SST-1M stereo system is currently operational and collecting data at the Ondřejov observatory in the Czech Republic, situated at 500 m a.s.l. Preliminary results from this system are promising. A forthcoming paper will provide a comprehensive analysis of the telescope's performance in detecting gamma rays and operating under real-world conditions.
    Dostawca treści:
    Repozytorium Uniwersytetu Jagiellońskiego
    Artykuł
    Tytuł:
    Observation of the Crab Nebula with the Single-Mirror Small-Size Telescope stereoscopic system at low altitude
    Autorzy:
    Ziętara, Krzysztof
    Sternberger, R.
    Müller, A. L.
    Hamal, P.
    Muthyala, S. R.
    Favre, Y.
    Neise, D.
    Moderski, R.
    Palatka, M.
    della Volpe, D.
    Świerk, P.
    Świerblewski, J.
    Cadoux, F.
    Beshley, V.
    Novotný, V.
    Jelínek, M.
    Lyard, E.
    Stawarz, Łukasz
    Vícha, J.
    Borkowski, J.
    Heller, M.
    Muraczewski, A.
    Glowacki, E.
    Mach, E.
    Michałowski, J.
    Nalewajski, K.
    Marek, W.
    Janeček, P.
    Pech, M.
    Trávníček, P.
    Walter, R.
    Chudoba, J.
    Boula, S.
    Blažek, J.
    Lacave, B.
    Bulik, T.
    Hrabovský, M.
    Nikołajuk, M.
    Prouza, M.
    Christov, A.
    Casanova, S.
    Niemiec, J.
    Ostrowski, Michał
    Araudo, A.
    Dědic, P.
    Gieras, T.
    Štrobl, J.
    Alispach, C.
    Chytka, L.
    Jílek, V.
    Troyano Pujadas, I.
    Montaruli, T.
    Balbo, M.
    Nagai, A.
    Gibaud, L.
    Mandát, D.
    Miroń, M.
    Sliusar, V.
    Tavernier, T.
    Karas, V.
    Stodulska, M.
    Čechvala, P.
    Juryšek, J.
    Schovanek, P.
    Garczarczyk, M.
    Michal, S.
    Opis:
    The Single-Mirror Small-Size Telescope (SST-1M) stereoscopic system is composed of two Imaging Atmospheric Cherenkov Telescopes (IACTs) designed to deliver optimal performance for gamma-ray astronomy in the multi-TeV energy range. It features a 4-m diameter tessellated mirror dish and an innovative SiPM-based camera. Its optical system features a 4-m diameter spherical mirror dish based on the Davies-Cotton design, maintaining a good image quality over a large field of view (FoV), while minimizing optical aberrations. In 2022, two SST-1M telescopes were installed at the Ondřejov Observatory, Czech Republic at an altitude of 510 meters above sea level, collecting data for commissioning and astronomical observations since then. We present the first SST-1M observations of the Crab Nebula, conducted between September 2023 and March 2024 in both mono and stereoscopic modes. During this observation period, 46 hours for the SST-1M-1 and 52 hours for the SST-1M-2 were collected (of which 33 hours were in stereoscopic mode). In this work, we used the Crab Nebula observation to validate the expected performance of the instrument, as evaluated by Monte Carlo (MC) simulations that were carefully tuned to account for instrumental and atmospheric effects. We determined that the energy threshold at the analysis level for the zenith angles below 30° is 1 TeV for mono mode and 1.3 TeV for stereo mode. The energy and angular resolutions were approximately 20% and 0.18° for mono mode and 10% and 0.10° for stereo mode, respectively. We present an off-axis performance assessment of the instrument and a detailed study of the systematic uncertainties. The full simulation results for the telescope and its camera are compared to the data for the first time, enabling a deeper understanding of the SST-1M array performance.
    Dostawca treści:
    Repozytorium Uniwersytetu Jagiellońskiego
    Artykuł
      Wyświetlanie 1-5 z 5

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