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Title:Cosmic Ray Shower Profile Track Finding for Telescope Array Fluorescence Detectors
Authors:ID Lundquist, Jon Paul, UNG (Author)
Files:.pdf ICRC2015_442.pdf (1,59 MB)
MD5: E10AD5FFA402ADB0E42B21E5A77B111F
 
Language:English
Work type:Not categorized
Typology: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
Publication version:Version of Record
Year of publishing:2016
Number of pages:8
Numbering:236, 236
PID:20.500.12556/RUNG-5178-a2f82bf5-235f-dfc8-4c09-d2a57b15ddbd New window
COBISS.SI-ID:13193987 New window
DOI:10.22323/1.236.0442 New window
NUK URN:URN:SI:UNG:REP:EISU3VYD
Publication date in RUNG:29.04.2020
Views:2763
Downloads:107
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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

Licences

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/
Description:The most restrictive Creative Commons license. This only allows people to download and share the work for no commercial gain and for no other purposes.
Licensing start date:29.04.2020

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