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Title:A study of analysis method for the identification of UHECR source type
Authors:ID Yoshida, F. (Author)
ID Lundquist, Jon Paul (Author), et al.
Files:.pdf ICRC2021_242.pdf (2,71 MB)
MD5: 5734646D4D6CBF7DD8224AB31FFEABFF
 
URL https://pos.sissa.it/395/242/
 
URL https://pos.sissa.it/395/242/pdf
 
Language:English
Work type:Not categorized
Typology:1.08 - Published Scientific Conference Contribution
Organization:UNG - University of Nova Gorica
Abstract:The autocorrelation analysis using the arrival direction of Ultra High Energy Cosmic Rays (UHECRs) has been previously reported by the Telescope Array (TA) experiment. It is expected that the autocorrelation function reflects the source distribution. We simulate the expected arrival direction distribution of the cosmic rays using the catalogs of candidate sources. We take into account random deflection in the magnetic fields, with the magnitude of deflection determined by the charge and energy of the cosmic rays, coherence length and magnitude of the extragalactic magnetic field (EGMF), and by distance to source. In addition, in order to compare with the results of TA experiment, we consider the TA exposure. We compare the autocorrelation of the arrival directions corresponding to different source catalogs with the isotropic distribution. We calculate the autocorrelation function for each type of source candidates using this procedure. We will discuss the ability of this method to identify the source type of UHECRs.
Keywords:Telescope Array, indirect detection, surface detection, ground array, ultra-high energy, cosmic rays, energy spectrum, composition, anisotropy, autocorrelation, source models, magnetic fields
Publication status:Published
Year of publishing:2022
PID:20.500.12556/RUNG-8536 New window
COBISS.SI-ID:167045891 New window
DOI:10.22323/1.395.0242 New window
NUK URN:URN:SI:UNG:REP:83XMZYM1
Publication date in RUNG:04.10.2023
Views:2308
Downloads:10
Metadata:XML DC-XML DC-RDF
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YOSHIDA, F. and LUNDQUIST, Jon Paul, 2022, A study of analysis method for the identification of UHECR source type. In : 37th International Cosmic Ray Conference [online]. Published Scientific Conference Contribution. Trieste, Italy. 2022. [Accessed 3 April 2025]. Retrieved from: https://repozitorij.ung.si/IzpisGradiva.php?lang=eng&id=8536
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Record is a part of a monograph

Title:37th International Cosmic Ray Conference : ICRC2023
Place of publishing:Trieste, Italy
Publisher:Proceedings of Science
Year of publishing:2022

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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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