Article révisé par les pairs
Résumé : Evidence of an energy dependent intermediate-scale anisotropy has been found in the arrival directions of ultra-high energy cosmic rays in the northern hemisphere, using 7 years of TA surface detector data. The previously reported "hot spot" excess E ≥ 1019.75 EeV is found to correspond to a deficit, or "cold spot," of events for 1019.2 ≤ E < 1019.75 EeV. This feature suggests energy dependent magnetic deflection of cosmic-rays. The global post-trial significance of the energy spectrum deviation is found to be 3.74σ.