Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
University of Chicago
Enrico Fermi Institute and Dept. of Physics, University of Chicago, Chicago, IL, USA
Enrico Fermi Institute and Department of Physics, University of Chicago
Chicago, University, Chicago, IL
Chicago Univ., IL.
Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA
Department of Physics, Enrico Fermi Institute, University of Chicago, 5640 Ellis Avenue, 60637-1433, Chicago, IL, USA
Department of Physics and Astronomy, DePauw University, Greencastle, IN 46135.
Enrico Fermi Institute and Department of Physics, University of Chicago, IL 60637, USA
Enrico Fermi Institute, University of Chicago, Chicago, IL 60637.
Enrico Fermi Institute and Department of Physics, University of Chicago, Chicago, IL 60637, USA
Enrico Fermi Institute and Department of Physics, University of Chicago, Chicago, Illinois 60637
The University of Chicago, Chicago, IL 60637
Enrico Fermi Institute and Department of Physics, 933 E. 56th Street, University of Chicago, Chicago, IL 60637.
Department of Physics, University of California at Irvine, Irvine, California 92717
Harvard-Smithsonian Center for Astrophysics, P.O. Box 97, Amado, AZ 85645
Bristol, University, Bristol, England
H. H. Wills Physics Laboratory, University of Bristol, Tyndall Avenue, Bristol, UK
Chicago, University, IL
University of Chicago, USA
Chicago Univ., IL
Enrico Fermi Institute, University of Chicago, IL 60637, USA
Enrico Fermi Institute, University of Chicago, LASR, 933 E 56th St., Chicago, IL 60637
Enrico Fermi Institute, University of Chicago, LASR, 933 E56th St, Chicago, IL 60637
A connection between star formation activity and cosmic rays in the starburst galaxy M 82
A detector for cosmic-ray nuclei at very high energies
A High Resolution Method for Measuring Cosmic Ray Composition beyond 10 TeV
A Measurement of the Cosmic Ray Positron Fraction at Intermediate Energies
A New High-Resolution Method for Measuring Cosmic Ray Composition beyond 10 TeV
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