- Abstract:
- A search was conducted for TeV γ-rays emitted from the direction of the ultra-high-energy cosmic ray detected by the Fly's Eye experiment with energy E ∼ 3 × 1020 eV. No enhancement was found at a level of 10-10 cm-2 s-1 for E > 350 GeV. A steady source of ultra-high-energy cosmic ray protons or photons would be expected to produce a γ-ray flux above this level. An upper limit was also set for the flux of TeV γ-rays from 3C 147, the most prominent active galactic nucleus in the error box.
- Publication status:
- Published
- Publisher copy:
- 10.1086/367825
-
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- Publisher:
- Institute of Physics Publishing
- Journal:
- ASTROPHYSICAL JOURNAL
- Volume:
- 586
- Issue:
- 2
- Pages:
- 1232-1237
- Publication date:
- 2003-04-01
- DOI:
- EISSN:
-
1538-4357
- ISSN:
-
0004-637X
- URN:
-
uuid:8c25ad5a-53f5-40bc-bdb2-a5d52d72dc1d
- Source identifiers:
-
324756
- Local pid:
- pubs:324756
- Language:
- English
- Keywords:
- Copyright date:
- 2003
Journal article
A search for correlations of TeV gamma rays with ultra-high-energy cosmic rays
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