Add to ORKGWe describe a search for diffuse emission from several candidate sources of gamma-rays with energies ≳ 100 TeV, using the Chicago Air Shower Array / Michigan Muon Array (CASA-MIA) experiment. Since March 1990, CASA-MIA has recorded over 2.0 × 109 air shower events. Searches for diffuse emission are based upon the muon content of air showers. Candidate source regions include molecular clouds in the galaxy and the galactic plane. Results from CASA-MIA are compared to predicted diffuse emission
The Utah-Michigan-Chicago array addresses the need for greater measurement sensitivity in searches f...
© 2020. The American Astronomical Society. All rights reserved. The measurement of diffuse PeV gamma...
We have attempted to determine diffuse gamma ray flux using very large area (560m2) and compact muon...
Diffuse gamma‐rays from molecular clouds are excellent tracers of cosmic rays in the galaxy over a w...
Extensive air shower data collected using the CASA-MIA detector are examined for evidence of gamma r...
Ultra high energy (UHE) cosmic rays are particles reaching Earth that have energies greater than 101...
The CASA‐MIA experiment is a very large extensive air shower detector with good angular resolution. ...
The Chicago Air Shower Array (CASA) is a large area surface array designed to detect extensive air s...
We have searched for γ‐rays in the cosmic radiation above 200 TeV using a two‐level array of scintil...
We present the current status of the search for possible diffuse orlocalized gamma-ray emission at e...
Data from the Utah-Michigan (UM) extensive air shower (EAS) array at Dugway, Utah are examined for e...
Abstract. Isotropic gamma ray flux is expected as a result of interactions of ultra high energy cosm...
Results from the Utah-Michigan extensive air shower array are presented. We describe the array and r...
Journal ArticleDiffuse ultrahigh energy g radiation can arise from a variety of astrophysical source...
The Utah‐Michigan‐Chicago array addresses the need for greater measurement sensitivity in searches f...
The Utah-Michigan-Chicago array addresses the need for greater measurement sensitivity in searches f...
© 2020. The American Astronomical Society. All rights reserved. The measurement of diffuse PeV gamma...
We have attempted to determine diffuse gamma ray flux using very large area (560m2) and compact muon...
Diffuse gamma‐rays from molecular clouds are excellent tracers of cosmic rays in the galaxy over a w...
Extensive air shower data collected using the CASA-MIA detector are examined for evidence of gamma r...
Ultra high energy (UHE) cosmic rays are particles reaching Earth that have energies greater than 101...
The CASA‐MIA experiment is a very large extensive air shower detector with good angular resolution. ...
The Chicago Air Shower Array (CASA) is a large area surface array designed to detect extensive air s...
We have searched for γ‐rays in the cosmic radiation above 200 TeV using a two‐level array of scintil...
We present the current status of the search for possible diffuse orlocalized gamma-ray emission at e...
Data from the Utah-Michigan (UM) extensive air shower (EAS) array at Dugway, Utah are examined for e...
Abstract. Isotropic gamma ray flux is expected as a result of interactions of ultra high energy cosm...
Results from the Utah-Michigan extensive air shower array are presented. We describe the array and r...
Journal ArticleDiffuse ultrahigh energy g radiation can arise from a variety of astrophysical source...
The Utah‐Michigan‐Chicago array addresses the need for greater measurement sensitivity in searches f...
The Utah-Michigan-Chicago array addresses the need for greater measurement sensitivity in searches f...
© 2020. The American Astronomical Society. All rights reserved. The measurement of diffuse PeV gamma...
We have attempted to determine diffuse gamma ray flux using very large area (560m2) and compact muon...