Phys. Rev. Lett.
101,
221101
(2008)
[5 pages]
Discovery of Localized Regions of Excess 10-TeV Cosmic Rays
A. A. Abdo et al. Milagro Collaboration
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A. A. Abdo1, B. Allen2, T. Aune3, D. Berley4, E. Blaufuss4, S. Casanova5, C. Chen6, B. L. Dingus7, R. W. Ellsworth8, L. Fleysher9, R. Fleysher9, M. M. Gonzalez10, J. A. Goodman4, C. M. Hoffman7, P. H. Hüntemeyer7, B. E. Kolterman9, C. P. Lansdell11, J. T. Linnemann12, J. E. McEnery13, A. I. Mincer9, P. Nemethy9, D. Noyes4, J. Pretz7, J. M. Ryan14, P. M. Saz Parkinson3, A. Shoup15, G. Sinnis7, A. J. Smith4, G. W. Sullivan4, V. Vasileiou4, G. P. Walker16, D. A. Williams3, and G. B. Yodh6 (Milagro Collaboration)
1Naval Research Laboratory, Washington, D.C., USA 2Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts, USA 3University of California, Santa Cruz, California, USA 4University of Maryland, College Park, Maryland, USA 5Max Planck Institut für Kernphysik, Heidelberg, Germany 6University of California, Irvine, California, USA 7Los Alamos National Laboratory, Los Alamos, New Mexico, USA 8George Mason University, Fairfax, Virginia, USA 9New York University, New York, New York, USA 10Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, D.F., Mexico 11Institute for Defense Analyses, Alexandria, Virginia, USA 12Michigan State University, East Lansing, Michigan, USA 13NASA Goddard Space Flight Center, Greenbelt, Maryland, USA 14University of New Hampshire, Durham, New Hampshire, USA 15Ohio State University, Lima, Ohio, USA 16National Security Technologies, Las Vegas, Nevada, USA

Received 23 January 2008; revised 29 September 2008; published 24 November 2008
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The 7 year data set of the Milagro TeV observatory contains 2.2×1011 events of which most are due to hadronic cosmic rays. These data are searched for evidence of intermediate scale structure. Excess emission on angular scales of ∼10° has been found in two localized regions of unknown origin with greater than 12σ significance. Both regions are inconsistent with pure gamma-ray emission with high confidence. One of the regions has a different energy spectrum than the isotropic cosmic-ray flux at a level of 4.6σ, and it is consistent with hard spectrum protons with an exponential cutoff, with the most significant excess at ∼10 TeV. Potential causes of these excesses are explored, but no compelling explanations are found.
© 2008 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevLett.101.221101
DOI:
10.1103/PhysRevLett.101.221101
PACS:
95.85.Ry, 96.50.Xy, 98.35.Eg, 98.70.Sa
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