Journal article
A search for correlations of TeV gamma rays with ultra-high-energy cosmic rays
- 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
Actions
Access Document
- Publisher copy:
- 10.1086/367825
Why is the content I wish to access not available via ORA?
Bibliographic data (the information relating to research outputs) and full-text items (e.g. articles, theses, reports, etc.) arrive in ORA from several different sources. Unfortunately we are not able to make available the full-text for every research output.
Please contact the ORA team (
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
Content may be unavailable for the following four reasons
-
Version unsuitable
-
We have not obtained a suitable full-text for a given research output. See this page for more information.
-
Recently completed
-
Sometimes content is held in ORA but is unavailable for a fixed period of time to comply with the policies and wishes of rights holders.
-
Permissions
-
All content made available in ORA should comply with relevant rights, such as copyright. See this page for more information.
-
Clearance
-
Some thesis volumes scanned as part of the digitisation scheme funded by Dr Leonard Polonsky are currently unavailable due to sensitive material or uncleared third-party copyright content. We are attempting to contact authors whose theses are affected.
Alternative access to the full-text
You may be able to access the full-text directly from the publisher's website using the 'Publisher Copy' link in the 'Links & Downloads' box from a research output's ORA record page. This method may require an institutional or individual subscription to the journal/resource.
Authors
Bibliographic Details
- 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
- Source identifiers:
-
324756
Item Description
- Language:
- English
- Keywords:
- Pubs id:
-
pubs:324756
- UUID:
-
uuid:8c25ad5a-53f5-40bc-bdb2-a5d52d72dc1d
- Local pid:
- pubs:324756
- Deposit date:
- 2012-12-19
Terms of use
- Copyright date:
- 2003
If you are the owner of this record, you can report an update to it here: Report update to this record