The hypothesis that there exists an excess of showers from the Galactic plane on the level 1 to 2% at energies just above 10 to the 16th power eV is explored. The excess shower from the Galactic plane seems to be very similar in properties to excess showers from the point sources/flat spectrum, deficit of low energy muons. Those facts suggest that the excess from the Galactic plane are probably due to summing up of the contribution from individual point sources. That in turn suggest that those sources are rather numerous
The arrival directions of the gamma-quanta with energies of about 10 to 15th power eV which were reg...
These lectures discuss the mysteries involving the production and extragalactic propagation of ultra...
A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...
We have searched for γ‐rays in the cosmic radiation above 200 TeV using a two‐level array of scintil...
The discovery of cosmic rays with energies greater than 1014e V has posed a question that has not, a...
The result of a calculation of the expected number of muons in gamma ray initiated and cosmic ray in...
Considerable interest has developed in the search for local sources of superhigh-energy gamma-rays. ...
Journal ArticleFrom April 1988 to February 1990 we used a two-level array of scintillators to search...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
It is crucial to identify the ultrahigh-energy cosmic-ray sources and probe their unknown properties...
The apparent lack of suitable astrophysical sources for cosmic rays with E > 10^{19.7} eV (UHECRs) i...
Theoretical aspects of potential astrophysical sources of the highest energy cosmic rays are discuss...
The EGRET results for gamma ray intensities in and near the Galactic Plane have been analysed in som...
Diffuse gamma‐rays from molecular clouds are excellent tracers of cosmic rays in the galaxy over a w...
The recently observed primary ultra high energy gamma-rays (UHEGR) testify to the cosmic ray (CR) ac...
The arrival directions of the gamma-quanta with energies of about 10 to 15th power eV which were reg...
These lectures discuss the mysteries involving the production and extragalactic propagation of ultra...
A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...
We have searched for γ‐rays in the cosmic radiation above 200 TeV using a two‐level array of scintil...
The discovery of cosmic rays with energies greater than 1014e V has posed a question that has not, a...
The result of a calculation of the expected number of muons in gamma ray initiated and cosmic ray in...
Considerable interest has developed in the search for local sources of superhigh-energy gamma-rays. ...
Journal ArticleFrom April 1988 to February 1990 we used a two-level array of scintillators to search...
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base...
It is crucial to identify the ultrahigh-energy cosmic-ray sources and probe their unknown properties...
The apparent lack of suitable astrophysical sources for cosmic rays with E > 10^{19.7} eV (UHECRs) i...
Theoretical aspects of potential astrophysical sources of the highest energy cosmic rays are discuss...
The EGRET results for gamma ray intensities in and near the Galactic Plane have been analysed in som...
Diffuse gamma‐rays from molecular clouds are excellent tracers of cosmic rays in the galaxy over a w...
The recently observed primary ultra high energy gamma-rays (UHEGR) testify to the cosmic ray (CR) ac...
The arrival directions of the gamma-quanta with energies of about 10 to 15th power eV which were reg...
These lectures discuss the mysteries involving the production and extragalactic propagation of ultra...
A re-examination of the energy cosmic ray spectrum above $10^{20}$ eV is presented. The overall data...