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Title:Updates of the surface detector array of the TAx4 experiment
Authors:ID Kido, Eiji (Author)
ID Abbasi, R. U. (Author)
ID Abe, Y. (Author)
ID Abu-Zayyad, T. (Author)
ID Allen, M. (Author)
ID Arai, Yasuhiko (Author)
ID Arimura, R. (Author)
ID Barcikowski, E. (Author)
ID Belz, J. W. (Author)
ID Bergman, Douglas R. (Author)
ID Lundquist, Jon Paul (Author)
Files:.pdf ICRC2023_239.pdf (2,39 MB)
MD5: 4FE8493B978385146E2EA92E22585E2F
 
URL https://pos.sissa.it/444/239/
 
URL https://pos.sissa.it/444/239/pdf
 
Language:English
Work type:Unknown
Typology:1.08 - Published Scientific Conference Contribution
Organization:UNG - University of Nova Gorica
Abstract:The TAx4 experiment plans to realize an Ultra High Energy Cosmic Rays (UHECR) detection area four times larger than that of the TA experiment. TAx4 will include five hundreds new surface detectors (SD) spaced at 2.08 km and two new fluorescence detectors (FD), which provides hybrid observation of UHECRs. We deployed 257 SDs in 2019 and completed building 2 FD stations in 2020, all operating stably. The data acquisition of the SDs is made via six communication towers, and inter-tower triggers have been recently implemented.
Keywords:Telescope Array, TAx4, indirect detection, hybrid detection
Publication date:01.01.2023
Year of publishing:2023
Number of pages:str. 1-7
PID:20.500.12556/RUNG-8566-d687daa4-8391-4e38-e860-13bde6b2e768 New window
COBISS.SI-ID:167761923 New window
UDC:539.1
ISSN on article:1824-8039
DOI:10.22323/1.444.0239 New window
NUK URN:URN:SI:UNG:REP:RRJEL1G7
Publication date in RUNG:10.10.2023
Views:1428
Downloads:7
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Record is a part of a proceedings

Title:38th International Cosmic Ray Conference [also] ICRC2023
COBISS.SI-ID:162195971 New window

Record is a part of a journal

Title:Proceedings of science
Shortened title:Pos proc. sci.
Publisher:Sissa
ISSN:1824-8039
COBISS.SI-ID:20239655 New window

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License:CC BY-NC-ND 4.0, Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
Link:http://creativecommons.org/licenses/by-nc-nd/4.0/
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