An excess of cosmic ray electrons at energies of 300–800 GeV

By Johan Chang, J. Adams, H. Ahn, G. Bashindzhagyan, M. Christl, O. Ganel, T. Guzik, J. Isbert, K. C. Kim, E. Kuznetsov and 9 more. Nature, 2008

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Dark matter direct detection signals inferred from a cosmological N-body simulation with baryons (2009, methodology): “The positron and electron peak seen by ATIC [21] has been attened by HESS [31] and FERMI [32] measurements.”
Abelian hidden sectors at a GeV (2009, methodology): “The PAMELA [18], ATIC [19], and PPB-BETS [20] experiments observe excesses in cosmic ray positrons and electrons at energies above 10 GeV.”
GIANT GAMMA-RAY BUBBLES FROM FERMI-LAT: ACTIVE GALACTIC NUCLEUS ACTIVITY OR BIPOLAR GALACTIC WIND? (2010, background): “In this case, while the lowest energy bin in the gammarays is better fitted, the lack of low-energy CRs means 15 However, note that the large peak observed by ATIC -2 and ATIC -4 appears to be in conflict with the Fermi measurement of the spectrum, which contains no such feature. that synchrotron ca”
Probing the ATIC peak in the cosmic-ray electron spectrum with H.E.S.S. (2009, methodology): “Recently, the ATIC collaboration reported the measurement of an excess in the electron spectrum (Chang et al. 2008).”
Double-Disk Dark Matter (2013, background): “Furthermore, a large flux of high-energy electrons and positrons recently observed in cosmic rays by PAMELA and subsequent experiments [83–87] also requires large boost factors to explain in terms of dark matter annihilation [88] (though it is plausibly due to pulsars).”