TY - JOUR
T1 - Self-trigger radio prototype array for GRAND
AU - GRAND Collaboration
AU - Zhang, Yi
AU - He, Haoning
AU - Zhang, Pengfei
AU - Álvarez-Muñiz, Jaime
AU - Batista, Rafael Alves
AU - Benoit-Lévy, Aurélien
AU - Bolmont, Julien
AU - Brans, Henk
AU - Bustamante, Mauricio
AU - Charrier, Didier
AU - Cheng, Ling Mei
AU - Chiche, Simon
AU - Dai, Zigao
AU - de Almeida, Rogerio M.
AU - Decoene, Valentin
AU - Denton, Peter B.
AU - de Errico, Beatriz
AU - De Jong, Sijbrand
AU - de Mello Neto, João R.T.
AU - De Vries, Krijn D.
AU - Duan, Kaikai
AU - Duan, Ran
AU - Engel, Ralph
AU - Fan, Yizhong
AU - Fang, Ke
AU - Gou, Quan Bu
AU - Gu, Junhua
AU - Guépin, Claire
AU - Guo, Jianhua
AU - Guo, Yiqing
AU - Habraken, Rene
AU - Haungs, Andreas
AU - He, Haoning
AU - Hivon, Eric
AU - Hu, Hongbo
AU - Huang, Xiaoyuan
AU - Huang, Yan
AU - Huege, Tim
AU - Oliveira, Marcelo Ismerio
AU - Koirala, Ramesh
AU - Kotera, Kumiko
AU - Jiang, Wen
AU - Lago, Bruno L.
AU - Le Coz, Sandra
AU - Lenain, Jean Philippe
AU - Liu, Bo
AU - Liu, Cheng
AU - Liu, Ruoyu
AU - Mostafá, Miguel
AU - Murase, Kohta
N1 - Publisher Copyright:
© Copyright owned by the author(s).
PY - 2022/3/18
Y1 - 2022/3/18
N2 - The GRANDProto300 (GP300) array is a pathfinder for the Giant Radio Array for Neutrino Detection (GRAND) project. The deployment of the array, consisting of 300 antennas, will start in 2021 in a radio-quiet area of ∼ 200 km2 near Lenghu (∼ 3000m a.s.l.) in China. Serving as a test bench, the GP300 array is expected to pioneer techniques of autonomous radio detection including identification and reconstruction of nearly horizontal cosmic-ray (CR) air showers. In addition, the GP300 array is at a privileged position to study the transition between Galactic and extragalactic origins of cosmic rays, due to its large effective area and the precise measurements of both energy and mass composition for CRs with energies ranging from 30 PeV to 1 EeV. Using the GP300 array we will also investigate the potential sensitivity for radio transients such as Giant Radio Pulses and Fast Radio Bursts in the 50-200 MHz range.
AB - The GRANDProto300 (GP300) array is a pathfinder for the Giant Radio Array for Neutrino Detection (GRAND) project. The deployment of the array, consisting of 300 antennas, will start in 2021 in a radio-quiet area of ∼ 200 km2 near Lenghu (∼ 3000m a.s.l.) in China. Serving as a test bench, the GP300 array is expected to pioneer techniques of autonomous radio detection including identification and reconstruction of nearly horizontal cosmic-ray (CR) air showers. In addition, the GP300 array is at a privileged position to study the transition between Galactic and extragalactic origins of cosmic rays, due to its large effective area and the precise measurements of both energy and mass composition for CRs with energies ranging from 30 PeV to 1 EeV. Using the GP300 array we will also investigate the potential sensitivity for radio transients such as Giant Radio Pulses and Fast Radio Bursts in the 50-200 MHz range.
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M3 - Conference article
AN - SCOPUS:85145007891
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 1035
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -