An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic 
Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray Sources

Aab, A.; Abreu, P.; Aglietta, M.; Albuquerque, I.F.M.; Allekotte, I.; Almela, A.; Alvarez Castillo, J.; Alvarez-Muńiz, J.; Anastasi, G.A.; Anchordoqui, L.; et, al.; Biermann, P.

doi:10.3847/2041-8213/aaa66d

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An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray Sources

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Biermann, P.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Aab, A., Abreu, P., Aglietta, M., Albuquerque, I., Allekotte, I., Almela, A., et al. (2018). An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray Sources. Astrophysical Journal, Letters, 853: L29, pp. L29. doi:10.3847/2041-8213/aaa66d.

Cite as: https://hdl.handle.net/21.11116/0000-0004-3C8C-C

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