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Title: Cosmic Ray Shower Profile Track Finding for Telescope Array Fluorescence Detectors Authors: Lundquist, J. P. (Author) Files:  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  URN: URN:SI:UNG:REP:EISU3VYD DOI: 10.22323/1.236.0442  License: This work is available under this license: Creative Commons Attribution Non-Commercial No Derivatives 4.0 International Views: 2155 Downloads: 100 Metadata:     Categories: Document is not linked to any category. Cite this work Plain text BibTeX EndNote XML EndNote/Refer RIS ABNT ACM Ref AMA APA Chicago Harvard IEEE ISO 690 MLA Vancouver :

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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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