Interpretation of AMS-02 electrons and positrons data

@article{Mauro2014InterpretationOA,
  title={Interpretation of AMS-02 electrons and positrons data},
  author={Mattia di Mauro and Fiorenza Donato and Nicolao Fornengo and Roberto A Lineros and Andrea Vittino},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2014}
}
We perform a combined analysis of the recent AMS-02 data on electrons, positrons, electrons plus positrons and positron fraction, in a self-consistent framework where we realize a theoretical modeling of all the astrophysical components that can contribute to the observed fluxes in the whole energy range. The primary electron contribution is modeled through the sum of an average flux from distant sources and the fluxes from the local supernova remnants in the Green catalog. The secondary… 
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The Alpha Magnetic Spectrometer (AMS-02) experiment on board of the International Space Station is revolutionizing our understanding of cosmic rays. AMS-02 Collaboration has released the most precise
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TLDR
It is shown that in this approach, and accounting for AMS-02 results, the contribution of nearby accelerators to the fluxes at very high energy can be significantly reduced, thus avoiding any tension with anisotropy upper limits.
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