The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC 2023)

Fuente: arXiv
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Autores principales: GRAND Collaboration, Batista, Rafael Alves, Benoit-Lévy, Aurélien, Bister, Teresa, Bustamante, Mauricio, Chen, Yiren, Cheng, LingMei, Chiche, Simon, Colley, Jean-Marc, Correa, Pablo, Laurenciu, Nicoleta Cucu, Dai, Zigao, de Errico, Beatriz, de Jong, Sijbrand, Neto, João R. T. de Mello, de Vries, Krijn D., Denton, Peter B., Decoene, Valentin, Duan, Kaikai, Duan, Bohao, Engel, Ralph, Fan, Yizhong, Ferrière, Arsène, Gou, QuanBu, Gu, Junhua, Guelfand, Marion, Guo, Jianhua, Guo, Yiqing, Gupta, Vaidhai, Guépin, Claire, Gülzow, Lukas, Haungs, Andreas, He, Haoning, Hivon, Eric, Hu, Hongbo, Huang, Xiaoyuan, Huang, Yan, Huege, Tim, Jiang, Wen, Koirala, Ramesh, Kotera, Kumiko, Köhler, Jelena, Lago, Bruno L., Coz, Sandra Le, Legrand, François, Leisos, Antonios, Li, Rui, Liu, Cheng, Liu, Ruoyu, Liu, Wei, Ma, Pengxiong, Macias, Oscar, Magnard, Frédéric, Martineau-Huynh, Olivier, Mikhno, Ananstasiia, Mitra, Pragati, Mostafá, Miguel, Mottez, Fabrice, Mouette, Jean, Murase, Kohta, Niess, Valentin, Nonis, Stavros, Ogio, Shoichi, Oikonomou, Foteini, Pierog, Tanguy, Piotrowski, Lech Wiktor, Poisvert, Pierre, Prunet, Simon, Qian, Xiangli, Roth, Markus, Sako, Takashi, Schoorlemmer, Harm, Steeman, Bart, Szálas-Motesiczky, Dániel, Sławiński, Szymon, Timmermans, Anne, Timmermans, Charles, Tsirigotis, Apostolos, Tueros, Matías, Wang, Shen, Wang, Xiangyu, Wang, Xu, Wei, Daming, Wei, Feng, Wu, Xiangping, Wu, Xuefeng, Xu, Xin, Xu, Xing, Yang, Lili, Yang, Xuan, Yuan, Qiang, Zarka, Philippe, Zeng, Houdun, Zhang, Chao, Zhang, Jianli, Zhang, Kewen, Zhang, Pengfei, Zhang, Songbo, Zhou, Hao
Formato: Preprint
Publicado: 2023
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author GRAND Collaboration
Batista, Rafael Alves
Benoit-Lévy, Aurélien
Bister, Teresa
Bustamante, Mauricio
Chen, Yiren
Cheng, LingMei
Chiche, Simon
Colley, Jean-Marc
Correa, Pablo
Laurenciu, Nicoleta Cucu
Dai, Zigao
de Errico, Beatriz
de Jong, Sijbrand
Neto, João R. T. de Mello
de Vries, Krijn D.
Denton, Peter B.
Decoene, Valentin
Duan, Kaikai
Duan, Bohao
Engel, Ralph
Fan, Yizhong
Ferrière, Arsène
Gou, QuanBu
Gu, Junhua
Guelfand, Marion
Guo, Jianhua
Guo, Yiqing
Gupta, Vaidhai
Guépin, Claire
Gülzow, Lukas
Haungs, Andreas
He, Haoning
Hivon, Eric
Hu, Hongbo
Huang, Xiaoyuan
Huang, Yan
Huege, Tim
Jiang, Wen
Koirala, Ramesh
Kotera, Kumiko
Köhler, Jelena
Lago, Bruno L.
Coz, Sandra Le
Legrand, François
Leisos, Antonios
Li, Rui
Liu, Cheng
Liu, Ruoyu
Liu, Wei
Ma, Pengxiong
Macias, Oscar
Magnard, Frédéric
Martineau-Huynh, Olivier
Mikhno, Ananstasiia
Mitra, Pragati
Mostafá, Miguel
Mottez, Fabrice
Mouette, Jean
Murase, Kohta
Niess, Valentin
Nonis, Stavros
Ogio, Shoichi
Oikonomou, Foteini
Pierog, Tanguy
Piotrowski, Lech Wiktor
Poisvert, Pierre
Prunet, Simon
Qian, Xiangli
Roth, Markus
Sako, Takashi
Schoorlemmer, Harm
Steeman, Bart
Szálas-Motesiczky, Dániel
Sławiński, Szymon
Timmermans, Anne
Timmermans, Charles
Tsirigotis, Apostolos
Tueros, Matías
Wang, Shen
Wang, Xiangyu
Wang, Xu
Wei, Daming
Wei, Feng
Wu, Xiangping
Wu, Xuefeng
Xu, Xin
Xu, Xing
Yang, Lili
Yang, Xuan
Yuan, Qiang
Zarka, Philippe
Zeng, Houdun
Zhang, Chao
Zhang, Jianli
Zhang, Kewen
Zhang, Pengfei
Zhang, Songbo
Zhou, Hao
author_facet GRAND Collaboration
Batista, Rafael Alves
Benoit-Lévy, Aurélien
Bister, Teresa
Bustamante, Mauricio
Chen, Yiren
Cheng, LingMei
Chiche, Simon
Colley, Jean-Marc
Correa, Pablo
Laurenciu, Nicoleta Cucu
Dai, Zigao
de Errico, Beatriz
de Jong, Sijbrand
Neto, João R. T. de Mello
de Vries, Krijn D.
Denton, Peter B.
Decoene, Valentin
Duan, Kaikai
Duan, Bohao
Engel, Ralph
Fan, Yizhong
Ferrière, Arsène
Gou, QuanBu
Gu, Junhua
Guelfand, Marion
Guo, Jianhua
Guo, Yiqing
Gupta, Vaidhai
Guépin, Claire
Gülzow, Lukas
Haungs, Andreas
He, Haoning
Hivon, Eric
Hu, Hongbo
Huang, Xiaoyuan
Huang, Yan
Huege, Tim
Jiang, Wen
Koirala, Ramesh
Kotera, Kumiko
Köhler, Jelena
Lago, Bruno L.
Coz, Sandra Le
Legrand, François
Leisos, Antonios
Li, Rui
Liu, Cheng
Liu, Ruoyu
Liu, Wei
Ma, Pengxiong
Macias, Oscar
Magnard, Frédéric
Martineau-Huynh, Olivier
Mikhno, Ananstasiia
Mitra, Pragati
Mostafá, Miguel
Mottez, Fabrice
Mouette, Jean
Murase, Kohta
Niess, Valentin
Nonis, Stavros
Ogio, Shoichi
Oikonomou, Foteini
Pierog, Tanguy
Piotrowski, Lech Wiktor
Poisvert, Pierre
Prunet, Simon
Qian, Xiangli
Roth, Markus
Sako, Takashi
Schoorlemmer, Harm
Steeman, Bart
Szálas-Motesiczky, Dániel
Sławiński, Szymon
Timmermans, Anne
Timmermans, Charles
Tsirigotis, Apostolos
Tueros, Matías
Wang, Shen
Wang, Xiangyu
Wang, Xu
Wei, Daming
Wei, Feng
Wu, Xiangping
Wu, Xuefeng
Xu, Xin
Xu, Xing
Yang, Lili
Yang, Xuan
Yuan, Qiang
Zarka, Philippe
Zeng, Houdun
Zhang, Chao
Zhang, Jianli
Zhang, Kewen
Zhang, Pengfei
Zhang, Songbo
Zhou, Hao
contents The Giant Radio Array for Neutrino Detection (GRAND) is an envisioned observatory of ultra-high-energy particles of cosmic origin, with energies in excess of 100 PeV. GRAND uses large surface arrays of autonomous radio-detection units to look for the radio emission from extensive air showers that are triggered by the interaction of ultra-high-energy cosmic rays, gamma rays, and neutrinos in the atmosphere or underground. In particular, for ultra-high-energy neutrinos, the future final phase of GRAND aims to be sensitive enough to discover them in spite of their plausibly tiny flux. Presently, three prototype GRAND radio arrays are in operation: GRANDProto300, in China, GRAND@Auger, in Argentina, and GRAND@Nancay, in France. Their goals are to field-test the design of the radio-detection units, understand the radio background to which they are exposed, and develop tools for diagnostic, data gathering, and data analysis. This list of contributions to the 38th International Cosmic Ray Conference (ICRC 2023) presents an overview of GRAND, in its present and future incarnations, and a look at the first data collected by GRANDProto13, the first phase of GRANDProto300.
format Preprint
id arxiv_https___arxiv_org_abs_2308_00120
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC 2023)
GRAND Collaboration
Batista, Rafael Alves
Benoit-Lévy, Aurélien
Bister, Teresa
Bustamante, Mauricio
Chen, Yiren
Cheng, LingMei
Chiche, Simon
Colley, Jean-Marc
Correa, Pablo
Laurenciu, Nicoleta Cucu
Dai, Zigao
de Errico, Beatriz
de Jong, Sijbrand
Neto, João R. T. de Mello
de Vries, Krijn D.
Denton, Peter B.
Decoene, Valentin
Duan, Kaikai
Duan, Bohao
Engel, Ralph
Fan, Yizhong
Ferrière, Arsène
Gou, QuanBu
Gu, Junhua
Guelfand, Marion
Guo, Jianhua
Guo, Yiqing
Gupta, Vaidhai
Guépin, Claire
Gülzow, Lukas
Haungs, Andreas
He, Haoning
Hivon, Eric
Hu, Hongbo
Huang, Xiaoyuan
Huang, Yan
Huege, Tim
Jiang, Wen
Koirala, Ramesh
Kotera, Kumiko
Köhler, Jelena
Lago, Bruno L.
Coz, Sandra Le
Legrand, François
Leisos, Antonios
Li, Rui
Liu, Cheng
Liu, Ruoyu
Liu, Wei
Ma, Pengxiong
Macias, Oscar
Magnard, Frédéric
Martineau-Huynh, Olivier
Mikhno, Ananstasiia
Mitra, Pragati
Mostafá, Miguel
Mottez, Fabrice
Mouette, Jean
Murase, Kohta
Niess, Valentin
Nonis, Stavros
Ogio, Shoichi
Oikonomou, Foteini
Pierog, Tanguy
Piotrowski, Lech Wiktor
Poisvert, Pierre
Prunet, Simon
Qian, Xiangli
Roth, Markus
Sako, Takashi
Schoorlemmer, Harm
Steeman, Bart
Szálas-Motesiczky, Dániel
Sławiński, Szymon
Timmermans, Anne
Timmermans, Charles
Tsirigotis, Apostolos
Tueros, Matías
Wang, Shen
Wang, Xiangyu
Wang, Xu
Wei, Daming
Wei, Feng
Wu, Xiangping
Wu, Xuefeng
Xu, Xin
Xu, Xing
Yang, Lili
Yang, Xuan
Yuan, Qiang
Zarka, Philippe
Zeng, Houdun
Zhang, Chao
Zhang, Jianli
Zhang, Kewen
Zhang, Pengfei
Zhang, Songbo
Zhou, Hao
High Energy Physics - Experiment
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
High Energy Physics - Phenomenology
The Giant Radio Array for Neutrino Detection (GRAND) is an envisioned observatory of ultra-high-energy particles of cosmic origin, with energies in excess of 100 PeV. GRAND uses large surface arrays of autonomous radio-detection units to look for the radio emission from extensive air showers that are triggered by the interaction of ultra-high-energy cosmic rays, gamma rays, and neutrinos in the atmosphere or underground. In particular, for ultra-high-energy neutrinos, the future final phase of GRAND aims to be sensitive enough to discover them in spite of their plausibly tiny flux. Presently, three prototype GRAND radio arrays are in operation: GRANDProto300, in China, GRAND@Auger, in Argentina, and GRAND@Nancay, in France. Their goals are to field-test the design of the radio-detection units, understand the radio background to which they are exposed, and develop tools for diagnostic, data gathering, and data analysis. This list of contributions to the 38th International Cosmic Ray Conference (ICRC 2023) presents an overview of GRAND, in its present and future incarnations, and a look at the first data collected by GRANDProto13, the first phase of GRANDProto300.
title The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC 2023)
topic High Energy Physics - Experiment
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2308.00120