TY - JOUR
T1 - Status and results of the prototype LST of CTA
AU - for the CTA LST project
AU - Mazin, D.
AU - Abe, H.
AU - Aguasca, A.
AU - Agudo, I.
AU - Antonelli, L. A.
AU - Aramo, C.
AU - Armstrong, T.
AU - Artero, M.
AU - Asano, K.
AU - Ashkar, H.
AU - Aubert, P.
AU - Baktash, A.
AU - Bamba, A.
AU - Baquero Larriva, A.
AU - Baroncelli, L.
AU - Barres de Almeida, U.
AU - Barrio, J. A.
AU - Batkovic, I.
AU - Becerra González, J.
AU - Bernardos, M. I.
AU - Berti, A.
AU - Biederbeck, N.
AU - Bigongiari, C.
AU - Blanch, O.
AU - Bonnoli, G.
AU - Bordas, P.
AU - Bose, D.
AU - Bulgarelli, A.
AU - Burelli, I.
AU - Buscemi, M.
AU - Cardillo, M.
AU - Caroff, S.
AU - Carosi, A.
AU - Cassol, F.
AU - Cerruti, M.
AU - Chai, Y.
AU - Cheng, K.
AU - Chikawa, M.
AU - Chytka, L.
AU - Contreras, J. L.
AU - Cortina, J.
AU - Costantini, H.
AU - Dalchenko, M.
AU - De Angelis, A.
AU - de Bony de Lavergne, M.
AU - Deleglise, G.
AU - Delgado, C.
AU - Delgado Mengual, J.
AU - della Volpe, D.
AU - Murase, K.
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons.
PY - 2022/3/18
Y1 - 2022/3/18
N2 - The Large-Sized Telescopes (LSTs) of Cherenkov Telescope Array (CTA) are designed for gamma-ray studies focusing on low energy threshold, high flux sensitivity, rapid telescope repositioning speed and a large field of view. Once the CTA array is complete, the LSTs will be dominating the CTA performance between 20 GeV and 150 GeV. During most of the CTA Observatory construction phase, however, the LSTs will be dominating the array performance until several TeVs. In this presentation we will report on the status of the LST-1 telescope inaugurated in La Palma, Canary islands, Spain in 2018. We will show the progress of the telescope commissioning, compare the expectations with the achieved performance, and give a glance of the first physics results.
AB - The Large-Sized Telescopes (LSTs) of Cherenkov Telescope Array (CTA) are designed for gamma-ray studies focusing on low energy threshold, high flux sensitivity, rapid telescope repositioning speed and a large field of view. Once the CTA array is complete, the LSTs will be dominating the CTA performance between 20 GeV and 150 GeV. During most of the CTA Observatory construction phase, however, the LSTs will be dominating the array performance until several TeVs. In this presentation we will report on the status of the LST-1 telescope inaugurated in La Palma, Canary islands, Spain in 2018. We will show the progress of the telescope commissioning, compare the expectations with the achieved performance, and give a glance of the first physics results.
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M3 - Conference article
AN - SCOPUS:85125758931
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 872
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -