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Self-trigger radio prototype array for GRAND

Zhang, Y. ; He, H.; Zhang, P.; Álvarez-Muñiz, J.; Batista, R. A.; Benoit-Lévy, A.; Bolmont, J.; Brans, H.; Bustamante, M.; Charrier, D.; Cheng, L.; Chiche, S.; Dai, Z.; Almeida, R. M. de; Decoene, V.; Denton, P. B.; Errico, B. de; De Jong, S.; Mello Neto, J. R. T. de; ... mehr

Abstract:

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 (~3000 m 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.


Verlagsausgabe §
DOI: 10.5445/IR/1000156088
Veröffentlicht am 03.03.2023
Originalveröffentlichung
DOI: 10.22323/1.395.1035
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Zitationen: 3
Cover der Publikation
Zugehörige Institution(en) am KIT Institut für Astroteilchenphysik (IAP)
Institut für Experimentelle Teilchenphysik (ETP)
Publikationstyp Proceedingsbeitrag
Publikationsjahr 2022
Sprache Englisch
Identifikator ISSN: 1824-8039
KITopen-ID: 1000156088
HGF-Programm 51.13.04 (POF IV, LK 01) Kosmische Strahlung Technologien
Erschienen in 37th International Cosmic Ray Conference (ICRC2021): 12–23 July 2021, Berlin, Germany – Online
Veranstaltung 37th International Cosmic Ray Conference (ICRC 2021), Online, 12.07.2021 – 23.07.2021
Verlag Scuola Internazionale Superiore di Studi Avanzati (SISSA)
Seiten Art.-Nr.: 1035
Serie Proceedings of Science (PoS) ; 395
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