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Title:Cosmic Ray Shower Profile Track Finding for Telescope Array Fluorescence Detectors
Authors:Lundquist, J. P. (Author)
Files:.pdf ICRC2015_442.pdf (1,59 MB)
 
Language:English
Work type:Not categorized (r6)
Tipology:1.08 - Published Scientific Conference Contribution
Organization:UNG - University of Nova Gorica
Abstract:A simple cosmic ray track finding pattern recognition analysis (PRA) method for fluorescence detectors (FD) has been developed which significantly improves Xmax resolution and its dependence on energy. Events which have a clear rise and fall in the FD view contain information on Xmax that can be reliably reconstructed. Shower maximum must be extrapolated for events with Xmax outside the field of view of the detector, which creates a systematic dependence on the fitting function. The PRA method is a model and detector independent approach to removing these events, by fitting shower profiles to a set of triangles and applying limits on the allowable geometry.
Keywords:UHECR, cosmic rays, fluorescence detector, track finding, pattern recognition
Year of publishing:2016
Number of pages:8
Numbering:236, 236
COBISS_ID:13193987 Link is opened in a new window
URN:URN:SI:UNG:REP:EISU3VYD
DOI:10.22323/1.236.0442 Link is opened in a new window
License:CC BY-NC-ND 4.0
This work is available under this license: Creative Commons Attribution Non-Commercial No Derivatives 4.0 International
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Downloads:63
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Record is a part of a proceedings

Title:34th International Cosmic Ray Conference 2015

Record is a part of a journal

Title:Proceedings of Science ICRC 2015
Year of publishing:2016

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