Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Department of Physics, University of Wisconsin-Madison
The Milagro Collaboration
University of Wuppertal
University of California, Santa Cruz
260 authors
University of California, Santa Cruz, California 95064
University of California, Santa Cruz, CA 95064
University of California, Santa Cruz, CA 95064, USA
BUGH Wuppertal, Fachbereich Physik, D-42119 Wuppertal, Germany
University of California, Santa Cruz, CA 95064; Columbia University, New York, NY 10027.
BUGH Wuppertal, Fachbereich Physik, Gausssstr. 20, Wuppertal D-42119, Germany
Dept. of Physics, University of Wisconsin, Madison, WI 53706, USA
Universität Wuppertal, Fachbereich Physik, Gaussstr.20, 42097 Wuppertal, Germany
Department of Physics, University of Wisconsin, Madison, WI 53706, USA
Los Alamos National Laboratory, Los Alamos, NM 87545; Columbia University, New York, NY 10027.
Department of Physics and Nevis Laboratories, Columbia University
Physics Department, University of Wuppertal, D-42097 Wuppertal, Germany
Columbia
Department of Physics, Columbia University
Department of Physics, University of Wisconsin, 1150 University Ave, Madison, Wisconsin 53706, USA
Columbia University
HiRes
Columbia University, New York, New York
Department of Physics, Columbia University, New York, NY
Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, California 95064
A Bayesian Approach to Comparing Cosmic Ray Energy Spectra
A Cluster of Ultrahigh Energy Cosmic Rays: Interpretation and Implications
A measurement of time-averaged aerosol optical depth using air-showers observed in stereo by HiRes The High Resolution Fly's Eye Collaboration, R.U. Abbasi, T. Abu-Zayyad, J.F. Amann, G. Archbold, R. Atkins, K. Belov, J.W. Belz,
A Prototype PCI-based Data Acquisition System for Cosmic Ray Detection Below 10^18 eV
A Search for a Diffuse Flux of Astrophysical Muon Neutrinos with the IceCube 40-String Detector
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