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An alternative method to finding patterns in HiRes stereo data

delete2007-12-01
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OA
AI
R
Rasha Abbasi *
T
T. Abu‐Zayyad
J
J. F. Amman
S
Samuel Blake
S
S. BenZvi
D
D. R. Bergman
J
J. Boyer
Z
Z. Cao
B
B. Connolly
W
Wei-Tian Deng
J
Joseph R. Findlay
C
C. Finley
W
W. Hanlon
M
M. H. Holzscheiter
G
Gareth Hughes
P
P. Hüntemeyer
B
Bernard Jones
C
C. C. H. Jui
K
K. Kim
B
B. Knapp
M
M. M. Maestas
N
Naohiro Manago
E
E. J. Mannel
L
Lukáš Marek
K
Kennedy A. Martins
J
J. Matthews
J
J. N. Matthews
A
A. P. O’Neill
C
C. A. Painter
L
L. Perera
K
K. Reil
M
M. S. Roberts
D
D. Rodriguez
M
M. Sasaki
L
L. M. Scott
M
M. Seman
G
G. Sinnis
J
J. D. Smith
P
P. Sokolsky
C
C. Song
R
R. W. Springer
B
B. T. Stokes
S
S. B. Thomas
G
G. B. Thomson
D
D. Tupa
S
S. Westerhoff
L
Lawrence Weincke
A
A. Zech
X
X. Zhang
DOI:10.1016/j.astropartphys.2007.08.005delete
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Abstract

Abstract

En 中文
In this paper ultra-high energy cosmic rays UHECRs data observed by the HiRes fluorescence detector in stereo mode is analyzed to search for events in the sky with an arrival direction lying on a great circle. Such structure is known as the arc structure. The arc structure is expected when the charged cosmic rays pass through the galactic magnetic field. The arcs searched for could represent a broad or a small scale anisotropy depending on the proposed source model for the UHECRs. The arcs in this paper are looked for using Hough transform were Hough transform is a technique used to looking for patterns in images. No statistically significant arcs were found in this study. (c) 2007 Elsevier B.V. All rights reserved.
Keywords:
anisotropy
Hough transform
ultra-high energy cosmic rays
HiRes
AGASA
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Astroparticle Physics cover
Astroparticle Physics
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University of Utah
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Utah System of Higher Education
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