Expected performance of the K-EUSO space-based observatory

The JEM-EUSO Collaboration

Expected performance of the K-EUSO space-based observatory

The JEM-EUSO Collaboration

École Polytechnique

University of Turin
Tlemcen University
Nihon University
University of Alabama in Huntsville
Astroparticule and Cosmol APC
Universidad Politécnica de Madrid
Lehman College
INFN Sezione di Catania
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
INFN Sezione di Torino
University of Tokyo
Université Badji Mokhtar - Annaba
Centre de Développement des Technologies Avancées
Universidad de Alcalá
College of Computing
Institute of Experimental Physics Slovak Academy of Sciences
INFN Roma Tor Vergata
University of Tübingen
Instituto Nacional de Técnica Aeroespacial (CSIC/INTA)
INFN Sezione di Bari
Università degli studi di Bari Aldo Moro
Moscow State University
NASA Marshall Space Flight Center
Institute of Meteorology and Climate Research
Riken
Centre Suisse d'Electronique et de Microtechnique SA
University of Sofia
KTH Royal Institute of Technology
University of Geneva
University of Chicago
Universidad Autónoma de Chiapas
University of Rome “Tor Vergata”
INFN Sezione di Napoli
Technical University of Munich
Institute of Space Sciences
Università degli Studi di Catania
Istituto di Astrofisica e Planetologia Spaziali (IAPS)
Joint Laboratory of Optics
Kindai University
University of Naples Federico II
UTIU
University of California, Space Sciences Laboratory
IRAP/CNRS
Astrophysics Division
University of León
Colorado School of Mines
Algiers Observatory
LNF-INFN
Kyoto University
Technical University of Kosice
University of Maryland
Saitama University
Nagoya University
Sungkyunkwan University
Instituto de Astrofisica de Canarias
Konan University
National Astronomical Observatory
University of M’sila
Korea Astronomy and Space Science Institute
Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
University of Maryland Baltimore County
High Energy Accelerator Research Organization (KEK)
Research Unit on Optics and Photonics
Institute of Physics of the Czech Academy of Sciences
Benemerita Universidad Autonoma de Puebla
Chiba University
University of Utah
Univ. Mentouri de Constantine
Universidad Nacional Autónoma de México
University of Iowa
Osaka City University
ETH Zurich
University of Warsaw
Space Regatta Consortium
Hokkaido University
ISAS/JAXA
Osaka Electro-Communication University
Centro Mesoamericano de Física Teórica (MCTP)
Joint Institute for Nuclear Research, Dubna
Shinshu University
National Institutes for Quantum and Radiological Science and Technology
NASA Goddard Space Flight Center
Universidad Michoacana de San Nicolás de Hidalgo
Fairfield University
Kanazawa University

Résultats de recherche: Contribution à un journal › Article de conférence › Revue par des pairs

Résumé

K-EUSO is a planned mission of the JEM-EUSO program for the study of ultra-high energy cosmic rays (UHECR) from space, to be deployed on the International Space Station. The K-EUSO observatory consists of a UV telescope with a wide field of view, which aims at the detection of fluorescence light emitted by extensive air showers (EAS) in the atmosphere. The EAS events will be sampled with a time resolution of 1-2.5 μs to reconstruct the entire shower profile with high precision. The detector consisting of ∼ 10⁵ independent pixels will allow a spatial resolution of ∼700 m on ground. From a 400 km altitude, K-EUSO will achieve a large and full sky exposure to sample the highest energy range of the UHECR spectrum. In this contribution, we present estimates of the performance of the observatory: an estimation of the expected exposure and triggered event rate as a function of energy and the event reconstruction performance, including resolution of arrival directions and energy of UHECRs.

langue originale	Anglais
Numéro d'article	409
journal	Proceedings of Science
Volume	395
état	Publié - 18 mars 2022
Evénement	37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Allemagne Durée: 12 juil. 2021 → 23 juil. 2021

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@article{87137715733f4c149c6b3c46b64058eb,

title = "Expected performance of the K-EUSO space-based observatory",

abstract = "K-EUSO is a planned mission of the JEM-EUSO program for the study of ultra-high energy cosmic rays (UHECR) from space, to be deployed on the International Space Station. The K-EUSO observatory consists of a UV telescope with a wide field of view, which aims at the detection of fluorescence light emitted by extensive air showers (EAS) in the atmosphere. The EAS events will be sampled with a time resolution of 1-2.5 μs to reconstruct the entire shower profile with high precision. The detector consisting of ∼ 105 independent pixels will allow a spatial resolution of ∼700 m on ground. From a 400 km altitude, K-EUSO will achieve a large and full sky exposure to sample the highest energy range of the UHECR spectrum. In this contribution, we present estimates of the performance of the observatory: an estimation of the expected exposure and triggered event rate as a function of energy and the event reconstruction performance, including resolution of arrival directions and energy of UHECRs.",

author = "\{The JEM-EUSO Collaboration\} and Marta Bianciotto and G. Abdellaoui and S. Abe and Adams, \{J. H.\} and D. Allard and G. Alonso and L. Anchordoqui and A. Anzalone and E. Arnone and K. Asano and R. Attallah and H. Attoui and \{Ave Pernas\}, M. and M. Bagheri and J. Bal{\'a}z and M. Bakiri and D. Barghini and S. Bartocci and M. Battisti and J. Bayer and B. Beldjilali and T. Belenguer and N. Belkhalfa and R. Bellotti and Belov, \{A. A.\} and K. Benmessai and Mario Bertaina and Bertone, \{P. F.\} and Biermann, \{P. L.\} and F. Bisconti and C. Blaksley and N. Blanc and S. Blin-Bondil and P. Bobik and M. Bogomilov and K. Bolmgren and E. Bozzo and S. Briz and A. Bruno and Caballero, \{K. S.\} and F. Cafagna and G. Cambi{\'e} and D. Campana and Capdevielle, \{J. N.\} and F. Capel and A. Caramete and L. Caramete and P. Carlson and R. Caruso and \{de la Taille\}, C.",

note = "Publisher Copyright: {\textcopyright} 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); 37th International Cosmic Ray Conference, ICRC 2021 ; Conference date: 12-07-2021 Through 23-07-2021",

year = "2022",

month = mar,

day = "18",

language = "English",

volume = "395",

journal = "Proceedings of Science",

issn = "1824-8039",

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T1 - Expected performance of the K-EUSO space-based observatory

AU - The JEM-EUSO Collaboration

AU - Bianciotto, Marta

AU - Abdellaoui, G.

AU - Abe, S.

AU - Adams, J. H.

AU - Allard, D.

AU - Alonso, G.

AU - Anchordoqui, L.

AU - Anzalone, A.

AU - Arnone, E.

AU - Asano, K.

AU - Attallah, R.

AU - Attoui, H.

AU - Ave Pernas, M.

AU - Bagheri, M.

AU - Baláz, J.

AU - Bakiri, M.

AU - Barghini, D.

AU - Bartocci, S.

AU - Battisti, M.

AU - Bayer, J.

AU - Beldjilali, B.

AU - Belenguer, T.

AU - Belkhalfa, N.

AU - Bellotti, R.

AU - Belov, A. A.

AU - Benmessai, K.

AU - Bertaina, Mario

AU - Bertone, P. F.

AU - Biermann, P. L.

AU - Bisconti, F.

AU - Blaksley, C.

AU - Blanc, N.

AU - Blin-Bondil, S.

AU - Bobik, P.

AU - Bogomilov, M.

AU - Bolmgren, K.

AU - Bozzo, E.

AU - Briz, S.

AU - Bruno, A.

AU - Caballero, K. S.

AU - Cafagna, F.

AU - Cambié, G.

AU - Campana, D.

AU - Capdevielle, J. N.

AU - Capel, F.

AU - Caramete, A.

AU - Caramete, L.

AU - Carlson, P.

AU - Caruso, R.

AU - de la Taille, C.

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 - K-EUSO is a planned mission of the JEM-EUSO program for the study of ultra-high energy cosmic rays (UHECR) from space, to be deployed on the International Space Station. The K-EUSO observatory consists of a UV telescope with a wide field of view, which aims at the detection of fluorescence light emitted by extensive air showers (EAS) in the atmosphere. The EAS events will be sampled with a time resolution of 1-2.5 μs to reconstruct the entire shower profile with high precision. The detector consisting of ∼ 105 independent pixels will allow a spatial resolution of ∼700 m on ground. From a 400 km altitude, K-EUSO will achieve a large and full sky exposure to sample the highest energy range of the UHECR spectrum. In this contribution, we present estimates of the performance of the observatory: an estimation of the expected exposure and triggered event rate as a function of energy and the event reconstruction performance, including resolution of arrival directions and energy of UHECRs.

AB - K-EUSO is a planned mission of the JEM-EUSO program for the study of ultra-high energy cosmic rays (UHECR) from space, to be deployed on the International Space Station. The K-EUSO observatory consists of a UV telescope with a wide field of view, which aims at the detection of fluorescence light emitted by extensive air showers (EAS) in the atmosphere. The EAS events will be sampled with a time resolution of 1-2.5 μs to reconstruct the entire shower profile with high precision. The detector consisting of ∼ 105 independent pixels will allow a spatial resolution of ∼700 m on ground. From a 400 km altitude, K-EUSO will achieve a large and full sky exposure to sample the highest energy range of the UHECR spectrum. In this contribution, we present estimates of the performance of the observatory: an estimation of the expected exposure and triggered event rate as a function of energy and the event reconstruction performance, including resolution of arrival directions and energy of UHECRs.

UR - https://www.scopus.com/pages/publications/85144597312

M3 - Conference article

AN - SCOPUS:85144597312

SN - 1824-8039

VL - 395

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 409

T2 - 37th International Cosmic Ray Conference, ICRC 2021

Y2 - 12 July 2021 through 23 July 2021

ER -

Expected performance of the K-EUSO space-based observatory

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