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Large scale distribution of arrival directions of cosmic rays detected above $10^{18}$ eV at the Pierre Auger Observatory

Abstract:
A thorough search for large scale anisotropies in the distribution of arrival directions of cosmic rays detected above $10^{18}$ eV at the Pierre Auger Observatory is presented. This search is performed as a function of both declination and right ascension in several energy ranges above $10^{18}$ eV, and reported in terms of dipolar and quadrupolar coefficients. Within the systematic uncertainties, no significant deviation from isotropy is revealed. Assuming that any cosmic ray anisotropy is dominated by dipole and quadrupole moments in this energy range, upper limits on their amplitudes are derived. These upper limits allow us to challenge an origin of cosmic rays above $10^{18}$ eV from stationary galactic sources densely distributed in the galactic disk and emitting predominantly light particles in all directions.
Publication status:
Published

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Publisher copy:
10.1088/0067-0049/203/2/34

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Journal:
ApJS More from this journal
Volume:
203
Issue:
2
Pages:
34
Publication date:
2012-10-13
DOI:
EISSN:
1538-4365
ISSN:
0067-0049


Keywords:
Pubs id:
pubs:358087
UUID:
uuid:ae368279-3237-4238-9aee-814f206ba561
Local pid:
pubs:358087
Source identifiers:
358087
Deposit date:
2013-11-16

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