Phys. Rev. Lett.
92,
151101
(2004)
[4 pages]
Measurement of the Flux of Ultrahigh Energy Cosmic Rays from Monocular Observations by the High Resolution Fly’s Eye Experiment
R. U. Abbasi et al. High Resolution Fly’s Eye Collaboration
Show All Authors/Affiliations
Hide All Authors/Affiliations
R. U. Abbasi1, T. Abu-Zayyad1, J. F. Amann2, G. Archbold1, J. A. Bellido3, K. Belov1, J. W. Belz4, D. R. Bergman5, Z. Cao1, R. W. Clay3, M. D. Cooper2, H. Dai1, B. R. Dawson3, A. A. Everett1, Yu. A. Fedorova1, J. H. V. Girard1, R. C. Gray1, W. F. Hanlon1, C. M. Hoffman2, M. H. Holzscheiter2, P. Hüntemeyer1, B. F Jones1, C. C. H. Jui1, D. B. Kieda1, K. Kim1, M. A. Kirn4, E. C. Loh1, N. Manago6, L. J. Marek2, K. Martens1, G. Martin7, J. A. J. Matthews7, J. N. Matthews1, J. R. Meyer1, S. A. Moore1, P. Morrison1, A. N. Moosman1, J. R. Mumford1, M. W. Munro4, C. A. Painter2, L. Perera5, K. Reil1, R. Riehle1, M. Roberts7, J. S. Sarracino2, M. Sasaki6, S. R. Schnetzer5, P. Shen1, K. M. Simpson3, G. Sinnis2, J. D. Smith1, P. Sokolsky1, C. Song8, R. W. Springer1, B. T. Stokes1, S. F. Taylor1, S. B. Thomas1, T. N. Thompson2, G. B. Thomson5, D. Tupa2, S. Westerhoff8, L. R. Wiencke1, T. D. VanderVeen1, A. Zech5, and X. Zhang8 (High Resolution Fly’s Eye Collaboration)
1Department of Physics and High Energy Astrophysics Institute, University of Utah, Salt Lake City, Utah 84112, USA 2Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA 3Department of Physics, University of Adelaide, 5005 Adelaide, South Australia, Australia 4Department of Physics and Astronomy, University of Montana, Missoula, Montana 59812, USA 5Department of Physics and Astronomy, Rutgers-The State University of New Jersey, Piscataway, New Jersey 08854, USA 6Institute for Cosmic Ray Research, University of Tokyo, 277-8582 Kashiwa, Japan 7Department of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico 87131, USA 8Department of Physics and Nevis Laboratory, Columbia University, New York, New York 10533, USA
Received 12 August 2002; revised 28 May 2003; published 15 April 2004
We have measured the cosmic ray spectrum above 1017.2 eV using the two air-fluorescence detectors of the High Resolution Fly’s Eye observatory operating in monocular mode. We describe the detector, phototube, and atmospheric calibrations, as well as the analysis techniques for the two detectors. We fit the spectrum to a model consisting of galactic and extragalactic sources.
© 2004 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevLett.92.151101
DOI:
10.1103/PhysRevLett.92.151101
PACS:
98.70.Sa, 95.85.Ry, 96.40.De, 96.40.Pq
|
|