Issue |
A&A
Volume 691, November 2024
|
|
---|---|---|
Article Number | A328 | |
Number of page(s) | 16 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361/202450889 | |
Published online | 26 November 2024 |
A new method of reconstructing images of gamma-ray telescopes applied to the LST-1 of CTAO
1
Department of Physics, Tokai University,
4-1-1, Kita-Kaname,
Hiratsuka,
Kanagawa
259-1292,
Japan
2
Institute for Cosmic Ray Research, University of Tokyo,
5-1-5, Kashiwa-no-ha, Kashiwa,
Chiba
277-8582,
Japan
3
INFN and Università degli Studi di Siena, Dipartimento di Scienze Fisiche, della Terra e dell’Ambiente (DSFTA),
Sezione di Fisica, Via Roma 56,
53100
Siena,
Italy
4
Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM,
91191
Gif-sur-Yvette Cedex,
France
5
FSLAC IRL 2009, CNRS/IAC,
La Laguna,
Tenerife,
Spain
6
Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos, Universitat de Barcelona,
IEEC-UB, Martí i Franquès, 1,
08028
Barcelona,
Spain
7
Instituto de Astrofísica de Andalucía-CSIC,
Glorieta de la Astronomía s/n,
18008
Granada,
Spain
8
Department of Astronomy, University of Geneva,
Chemin d’Ecogia 16,
1290
Versoix,
Switzerland
9
IPARCOS-UCM, Instituto de Física de Partículas y del Cosmos, and EMFTEL Department, Universidad Complutense de Madrid,
Plaza de Ciencias, 1. Ciudad Universitaria,
28040
Madrid,
Spain
10
INFN Sezione di Napoli,
Via Cintia, ed. G,
80126
Napoli,
Italy
11
INAF – Osservatorio Astronomico di Roma,
Via di Frascati 33,
00040
Monteporzio Catone,
Italy
12
Max-Planck-Institut für Physik,
Föhringer Ring 6,
80805
München,
Germany
13
INFN Sezione di Padova and Università degli Studi di Padova,
Via Marzolo 8,
35131
Padova,
Italy
14
Univ. Savoie Mont Blanc, CNRS, Laboratoire d’Annecy de Physique des Particules – IN2P3,
74000
Annecy,
France
15
Universität Hamburg, Institut für Experimentalphysik,
Luruper Chaussee 149,
22761
Hamburg,
Germany
16
Graduate School of Science, University of Tokyo,
7-3-1 Hongo,
Bunkyo-ku, Tokyo
113-0033,
Japan
17
Faculty of Science and Technology, Universidad del Azuay,
Cuenca,
Ecuador
18
Centro Brasileiro de Pesquisas Físicas,
Rua Xavier Sigaud 150,
22290-180,
Rio de Janeiro,
Brazil
19
Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de La Laguna,
C. Vía Láctea, s/n,
38205
La Laguna,
Santa Cruz de Tenerife,
Spain
20
CIEMAT,
Avda. Complutense 40,
28040
Madrid,
Spain
21
University of Geneva – Département de physique nucléaire et corpusculaire,
24 Quai Ernest Ansernet,
1211
Genève 4,
Switzerland
22
INFN Sezione di Bari and Politecnico di Bari,
via Orabona 4,
70124
Bari,
Italy
23
Institut de Fisica d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology,
Campus UAB,
08193
Bellaterra (Barcelona),
Spain
24
INAF – Osservatorio Astronomico di Brera,
Via Brera 28,
20121
Milano,
Italy
25
Faculty of Physics and Applied Informatics, University of Lodz,
ul. Pomorska 149-153,
90-236
Lodz,
Poland
26
INAF – Osservatorio di Astrofisica e Scienza dello spazio di Bologna,
Via Piero Gobetti 93/3,
40129
Bologna,
Italy
27
INFN Sezione di Trieste and Università degli studi di Udine,
via delle scienze 206,
33100
Udine,
Italy
28
INFN Sezione di Catania,
Via S. Sofia 64,
95123
Catania,
Italy
29
INAF – Istituto di Astrofisica e Planetologia Spaziali (IAPS),
Via del Fosso del Cavaliere 100,
00133
Roma,
Italy
30
Aix Marseille Univ, CNRS/IN2P3, CPPM,
Marseille,
France
31
University of Alcalá UAH, Departamento de Physics and Mathematics,
Pza. San Diego,
28801
Alcalá de Henares,
Madrid,
Spain
32
INFN Sezione di Bari and Università di Bari,
via Orabona 4,
70126
Bari,
Italy
33
INFN Sezione di Torino,
Via P. Giuria 1,
10125
Torino,
Italy
34
Palacky University Olomouc, Faculty of Science,
17. listopadu 1192/12,
771 46
Olomouc,
Czech Republic
35
Dipartimento di Fisica e Chimica “E. Segrè”, Università degli Studi di Palermo,
Via Archirafi 36,
90123
Palermo,
Italy
36
IRFU, CEA, Université Paris-Saclay,
Bât 141,
91191
Gif-sur-Yvette,
France
37
Port d’Informació Científica,
Edifici D, Carrer de l’Albareda,
08193
Bellaterrra (Cerdanyola del Vallès),
Spain
38
Department of Physics, TU Dortmund University,
Otto-Hahn-Str. 4,
44227
Dortmund,
Germany
39
University of Rijeka, Department of Physics,
Radmile Matejcic 2,
51000
Rijeka,
Croatia
40
Institute for Theoretical Physics and Astrophysics, Universität Würzburg,
Campus Hubland Nord, Emil-Fischer-Str. 31,
97074
Würzburg,
Germany
41
Department of Physics and Astronomy, University of Turku,
FI- 20014
University of Turku,
Finland
42
INFN Sezione di Roma La Sapienza,
P.le Aldo Moro 2,
00185
Rome,
Italy
43
ILANCE, CNRS – University of Tokyo International Research Laboratory, University of Tokyo,
5-1-5 Kashiwa-no-Ha Kashiwa City,
Chiba
277-8582,
Japan
44
Physics Program, Graduate School of Advanced Science and Engineering, Hiroshima University,
1-3-1 Kagamiyama, Higashi-Hiroshima City,
Hiroshima
739-8526,
Japan
45
INFN Sezione di Roma Tor Vergata,
Via della Ricerca Scientifica 1,
00133
Rome,
Italy
46
University of Split,
FESB, R. Boškovića 32,
21000
Split,
Croatia
47
Department of Physics, Yamagata University,
1-4-12 Kojirakawamachi,
Yamagata-shi
990-8560,
Japan
48
Institut für Theoretische Physik, Lehrstuhl IV: Plasma- Astroteilchenphysik, Ruhr-Universität Bochum,
Universitätsstraße 150,
44801
Bochum,
Germany
49
Sendai College, National Institute of Technology,
4-16-1 Ayashi- Chuo, Aoba-ku, Sendai city,
Miyagi
989-3128,
Japan
50
Josip Juraj Strossmayer University of Osijek, Department of Physics,
Trg Ljudevita Gaja 6,
31000
Osijek,
Croatia
51
INFN Dipartimento di Scienze Fisiche e Chimiche – Università degli Studi dell’Aquila and Gran Sasso Science Institute,
Via Vetoio 1, Viale Crispi 7,
67100
L’Aquila,
Italy
52
Chiba University,
1-33, Yayoicho, Inage-ku, Chiba-shi,
Chiba
263-8522,
Japan
53
Kitashirakawa Oiwakecho,
Sakyo Ward,
Kyoto
606-8502,
Japan
54
FZU – Institute of Physics of the Czech Academy of Sciences,
Na Slovance 1999/2,
182 21
Praha 8,
Czech Republic
55
Laboratory for High Energy Physics, École Polytechnique Fédérale,
CH-1015
Lausanne,
Switzerland
56
Astronomical Institute of the Czech Academy of Sciences,
Bocni II 1401,
14100
Prague,
Czech Republic
57
Faculty of Science, Ibaraki University,
2 Chome-1-1 Bunkyo,
Mito,
Ibaraki
310-0056,
Japan
58
Faculty of Science and Engineering, Waseda University,
3 Chome- 4-1 Okubo, Shinjuku City,
Tokyo
169-0072,
Japan
59
Sorbonne Université, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies, LPNHE,
4 place Jussieu,
75005
Paris,
France
60
Institute of Particle and Nuclear Studies, KEK (High Energy Accelerator Research Organization),
1-1 Oho,
Tsukuba,
305-0801,
Japan
61
INFN Sezione di Trieste and Università degli Studi di Trieste,
Via Valerio 2 I,
34127
Trieste,
Italy
62
Escuela Politécnica Superior de Jaén, Universidad de Jaén,
Campus Las Lagunillas s/n, Edif. A3,
23071
Jaén,
Spain
63
Saha Institute of Nuclear Physics,
Sector 1, AF Block, Bidhan Nagar, Bidhannagar,
Kolkata,
West Bengal
700064,
India
64
Institute for Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences,
72 boul. Tsarigradsko chaussee,
1784
Sofia,
Bulgaria
65
Dipartimento di Fisica e Chimica ’E. Segrè’ Università degli Studi di Palermo,
via delle Scienze,
90128
Palermo
Italy
66
Grupo de Electronica, Universidad Complutense de Madrid,
Av. Complutense s/n,
28040
Madrid,
Spain
67
Institute of Space Sciences (ICE, CSIC), and Institut d’Estudis Espacials de Catalunya (IEEC), and Institució Catalana de Recerca I Estudis Avançats (ICREA),
Campus UAB, Carrer de Can Magrans, s/n
08193
Bellatera,
Spain
68
Hiroshima Astrophysical Science Center, Hiroshima University
1-3-1 Kagamiyama, Higashi-Hiroshima,
Hiroshima
739-8526,
Japan
69
School of Allied Health Sciences, Kitasato University,
Sagamihara,
Kanagawa
228-8555,
Japan
70
RIKEN, Institute of Physical and Chemical Research,
2-1 Hirosawa, Wako,
Saitama
351-0198,
Japan
71
Charles University, Institute of Particle and Nuclear Physics,
V Holešovičkách 2,
180 00
Prague 8,
Czech Republic
72
Division of Physics and Astronomy, Graduate School of Science, Kyoto University,
Sakyo-ku,
Kyoto
606-8502,
Japan
73
Institute for Space-Earth Environmental Research, Nagoya University,
Chikusa-ku,
Nagoya
464-8601,
Japan
74
Kobayashi-Maskawa Institute (KMI) for the Origin of Particles and the Universe, Nagoya University,
Chikusa-ku,
Nagoya
464-8602,
Japan
75
Graduate School of Technology, Industrial and Social Sciences, Tokushima University,
2-1 Minamijosanjima,
Tokushima
770-8506,
Japan
76
INFN Sezione di Pisa, Edificio C – Polo Fibonacci
Largo Bruno Pontecorvo 3,
56127
Pisa
Italy
77
INFN Dipartimento di Scienze Fisiche e Chimiche – Università degli Studi dell’Aquila and Gran Sasso Science Institute,
Via Vetoio 1, Viale Crispi 7,
67100
L’Aquila,
Italy
78
Gifu University, Faculty of Engineering,
1-1 Yanagido,
Gifu
501-1193,
Japan
79
Department of Physical Sciences, Aoyama Gakuin University,
Fuchinobe,
Sagamihara,
Kanagawa
252-5258,
Japan
80
Graduate School of Science and Engineering, Saitama University,
255 Simo-Ohkubo, Sakura-ku, Saitama city,
Saitama
338-8570,
Japan
81
Dipartimento di Fisica – Universitá degli Studi di Torino,
Via Pietro Giuria 1,
10125
Torino,
Italy
82
Department of Physics, Konan University,
8-9-1 Okamoto,
Higashinada-ku Kobe
658-8501,
Japan
★ Corresponding author; gabriel.emery@cta-consortium.org
Received:
28
May
2024
Accepted:
27
September
2024
Context. Imaging atmospheric Cherenkov telescopes (IACTs) are used to observe very high-energy photons from the ground. Gamma rays are indirectly detected through the Cherenkov light emitted by the air showers they induce. The new generation of experiments, in particular the Cherenkov Telescope Array Observatory (CTAO), sets ambitious goals for discoveries of new gamma-ray sources and precise measurements of the already discovered ones. To achieve these goals, both hardware and data analysis must employ cuttingedge techniques. This also applies to the LST-1, the first IACT built for the CTAO, which is currently taking data on the Canary island of La Palma.
Aims. This paper introduces a new event reconstruction technique for IACT data, aiming to improve the image reconstruction quality and the discrimination between the signal and the background from misidentified hadrons and electrons.
Methods. The technique models the development of the extensive air shower signal, recorded as a waveform per pixel, seen by CTAO telescopes’ cameras. Model parameters are subsequently passed to random forest regressors and classifiers to extract information on the primary particle.
Results. The new reconstruction was applied to simulated data and to data from observations of the Crab Nebula performed by the LST-1. The event reconstruction method presented here shows promising performance improvements. The angular and energy resolution, and the sensitivity, are improved by 10 to 20% over most of the energy range. At low energy, improvements reach up to 22%, 47%, and 50%, respectively. A future extension of the method to stereoscopic analysis for telescope arrays will be the next important step.
Key words: methods: data analysis / techniques: image processing / telescopes / gamma rays: general
© The Authors 2024
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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