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From the following article:
An excess of cosmic ray electrons at energies of 300–800 GeV
J. Chang, J. H. Adams, H. S. Ahn, G. L. Bashindzhagyan, M. Christl, O. Ganel, T. G. Guzik, J. Isbert, K. C. Kim, E. N. Kuznetsov, M. I. Panasyuk, A. D. Panov, W. K. H. Schmidt, E. S. Seo, N. V. Sokolskaya, J. W. Watts, J. P. Wefel, J. Wu & V. I. Zatsepin
Nature 456, 362-365(20 November 2008)
doi:10.1038/nature07477
Figure 1
Separation of electrons from protons in the ATIC instrument.
Full size figure and legend (95K)Download Power Point slide (474K)Figure 2
ATIC-1 and ATIC-2 spectra at balloon altitude, showing good agreement with each other.
Full size figure and legend (97K)Download Power Point slide (476K)Figure 3
ATIC results showing agreement with previous data at lower energy and with the imaging calorimeter PPB-BETS at higher energy.
Full size figure and legend (114K)Download Power Point slide (492K)Figure 4
Assuming an annihilation signature of Kaluza–Klein dark matter, all the data can be reproduced.
Full size figure and legend (92K)Download Power Point slide (471K)Slides may be downloaded for educational use, according to the terms described in Nature Publishing Group's licensing policy.
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