TY - JOUR
T1 - Reconstruction of stereoscopic CTA events using deep learning with CTLearn
AU - the CTA Consortium
AU - Miener, T.
AU - Nieto, D.
AU - Brill, A.
AU - Spencer, S.
AU - Contreras, J. L.
AU - Abdalla, H.
AU - Abe, H.
AU - Abe, S.
AU - Abusleme, A.
AU - Acero, F.
AU - Acharyya, A.
AU - Acín Portella, V.
AU - Ackley, K.
AU - Adam, R.
AU - Adams, C.
AU - Adhikari, S. S.
AU - Aguado-Ruesga, I.
AU - Agudo, I.
AU - Aguilera, R.
AU - Aguirre-Santaella, A.
AU - Aharonian, F.
AU - Alberdi, A.
AU - Alfaro, R.
AU - Alfaro, J.
AU - Alispach, C.
AU - Aloisio, R.
AU - Alves Batista, R.
AU - Amans, J. P.
AU - Amati, L.
AU - Amato, E.
AU - Ambrogi, L.
AU - Ambrosi, G.
AU - Ambrosio, M.
AU - Ammendola, R.
AU - Anderson, J.
AU - Anduze, M.
AU - Angüner, E. O.
AU - Antonelli, L. A.
AU - Antonuccio, V.
AU - Antoranz, P.
AU - Anutarawiramkul, R.
AU - Aragunde Gutierrez, J.
AU - Aramo, C.
AU - Araudo, A.
AU - Araya, M.
AU - Arbet-Engels, A.
AU - Arcaro, C.
AU - Arendt, V.
AU - Armand, C.
AU - Armstrong, T.
AU - Arqueros, F.
AU - Arrabito, L.
AU - Arsioli, B.
AU - Artero, M.
AU - Asano, K.
AU - Ascasíbar, Y.
AU - Aschersleben, J.
AU - Ashley, M.
AU - Attinà, P.
AU - Aubert, P.
AU - Singh, C. B.
AU - Baack, D.
AU - Babic, A.
AU - Backes, M.
AU - Baena, V.
AU - Bajtlik, S.
AU - Baktash, A.
AU - Balazs, C.
AU - Balbo, M.
AU - Ballester, O.
AU - Ballet, J.
AU - Balmaverde, B.
AU - Bamba, A.
AU - Bandiera, R.
AU - Baquero Larriva, A.
AU - Barai, P.
AU - Barbier, C.
AU - Barbosa Martins, V.
AU - Barcelo, M.
AU - Barkov, M.
AU - Barnard, M.
AU - Baroncelli, L.
AU - Barres de Almeida, U.
AU - Barrio, J. A.
AU - Bastieri, D.
AU - Batista, P. I.
AU - Batkovic, I.
AU - Bauer, C.
AU - Bautista-González, R.
AU - Baxter, J.
AU - Becciani, U.
AU - Becerra González, J.
AU - Becherini, Y.
AU - Beck, G.
AU - Becker Tjus, J.
AU - Bednarek, W.
AU - Belfiore, A.
AU - Bellizzi, L.
AU - Belmont, R.
AU - Benbow, W.
AU - Berge, D.
AU - Bernardini, E.
AU - Bernardos, M. I.
AU - Bernlöhr, K.
AU - Berti, A.
AU - Berton, M.
AU - Bertucci, B.
AU - Beshley, V.
AU - Bhatt, N.
AU - Bhattacharyya, S.
AU - Bhattacharyya, W.
AU - Bhattacharyya, S.
AU - Bi, B.
AU - Bicknell, G.
AU - Biederbeck, N.
AU - Bigongiari, C.
AU - Biland, A.
AU - Bird, R.
AU - Bissaldi, E.
AU - Biteau, J.
AU - Bitossi, M.
AU - Blanch, O.
AU - Blank, M.
AU - Blazek, J.
AU - Bobin, J.
AU - Boccato, C.
AU - Bocchino, F.
AU - Boehm, C.
AU - Bohacova, M.
AU - Boisson, C.
AU - Boix, J.
AU - Bolle, J. P.
AU - Bolmont, J.
AU - Bonanno, G.
AU - Bonavolontà, C.
AU - Bonneau Arbeletche, L.
AU - Bonnoli, G.
AU - Bordas, P.
AU - Borkowski, J.
AU - Bórquez, S.
AU - Bose, R.
AU - Bose, D.
AU - Bosnjak, Z.
AU - Bottacini, E.
AU - Böttcher, M.
AU - Botticella, M. T.
AU - Boutonnet, C.
AU - Bouyjou, F.
AU - Bozhilov, V.
AU - Bozzo, E.
AU - Brahimi, L.
AU - Braiding, C.
AU - Brau-Nogué, S.
AU - Breen, S.
AU - Bregeon, J.
AU - Breuhaus, M.
AU - Brisken, W.
AU - Brocato, E.
AU - Brown, A. M.
AU - Brügge, K.
AU - Brun, P.
AU - Brun, P.
AU - Brun, F.
AU - Brunetti, L.
AU - Brunetti, G.
AU - Bruno, P.
AU - Bruno, A.
AU - Bruzzese, A.
AU - Bucciantini, N.
AU - Buckley, J.
AU - Bühler, R.
AU - Bulgarelli, A.
AU - Bulik, T.
AU - Bünning, M.
AU - Bunse, M.
AU - Burton, M.
AU - Burtovoi, A.
AU - Buscemi, M.
AU - Buschjäger, S.
AU - Busetto, G.
AU - Buss, J.
AU - Byrum, K.
AU - Caccianiga, A.
AU - Cadoux, F.
AU - Calanducci, A.
AU - Calderón, C.
AU - Calvo Tovar, J.
AU - Cameron, R.
AU - Campaña, P.
AU - Canestrari, R.
AU - Cangemi, F.
AU - Cantlay, B.
AU - Capalbi, M.
AU - Capasso, M.
AU - Cappi, M.
AU - Caproni, A.
AU - Capuzzo-Dolcetta, R.
AU - Caraveo, P.
AU - Cárdenas, V.
AU - Errando, M.
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
PY - 2022/3/18
Y1 - 2022/3/18
N2 - The Cherenkov Telescope Array (CTA), conceived as an array of tens of imaging atmospheric Cherenkov telescopes (IACTs), is an international project for a next-generation ground-based gamma-ray observatory, aiming to improve on the sensitivity of current-generation instruments a factor of five to ten and provide energy coverage from 20 GeV to more than 300 TeV. Arrays of IACTs probe the very-high-energy gamma-ray sky. Their working principle consists of the simultaneous observation of air showers initiated by the interaction of very-high-energy gamma rays and cosmic rays with the atmosphere. Cherenkov photons induced by a given shower are focused onto the camera plane of the telescopes in the array, producing a multi-stereoscopic record of the event. This image contains the longitudinal development of the air shower, together with its spatial, temporal, and calorimetric information. The properties of the originating very-high-energy particle (type, energy, and incoming direction) can be inferred from those images by reconstructing the full event using machine learning techniques. In this contribution, we present a purely deep-learning driven, full-event reconstruction of simulated, stereoscopic IACT events using CTLearn. CTLearn is a package that includes modules for loading and manipulating IACT data and for running deep learning models, using pixel-wise camera data as input.
AB - The Cherenkov Telescope Array (CTA), conceived as an array of tens of imaging atmospheric Cherenkov telescopes (IACTs), is an international project for a next-generation ground-based gamma-ray observatory, aiming to improve on the sensitivity of current-generation instruments a factor of five to ten and provide energy coverage from 20 GeV to more than 300 TeV. Arrays of IACTs probe the very-high-energy gamma-ray sky. Their working principle consists of the simultaneous observation of air showers initiated by the interaction of very-high-energy gamma rays and cosmic rays with the atmosphere. Cherenkov photons induced by a given shower are focused onto the camera plane of the telescopes in the array, producing a multi-stereoscopic record of the event. This image contains the longitudinal development of the air shower, together with its spatial, temporal, and calorimetric information. The properties of the originating very-high-energy particle (type, energy, and incoming direction) can be inferred from those images by reconstructing the full event using machine learning techniques. In this contribution, we present a purely deep-learning driven, full-event reconstruction of simulated, stereoscopic IACT events using CTLearn. CTLearn is a package that includes modules for loading and manipulating IACT data and for running deep learning models, using pixel-wise camera data as input.
UR - https://www.scopus.com/pages/publications/85145019293
M3 - Conference article
AN - SCOPUS:85145019293
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 730
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -