PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Cosmic-Ray Indirect. CRI-properties of CRs at high energies (anisotropy, energy, mass)
Report of the Telescope Array - Pierre Auger Observatory Working Group on Energy Spectrum
D. Ivanov*  on behalf of the Pierre Auger Collaboration and  On behalf of the Telescope Array collaboration
Full text: pdf
Pre-published on: September 26, 2017
Published on: August 03, 2018
The Telescope Array and Pierre Auger Collaborations have formed a working group to examine the similarities and differences in their measurements of the spectrum of ultra-high energy cosmic rays. The method chosen is for each experiment to measure the spectrum in the declination band of -15.7 < delta < +24.8 degrees, where both experiments have sensitivity. A second step chosen is to correct for the weighting in declination over each experiment's range of sensitivity in the common band of declinations. The results will be shown and interpretations given.
DOI: https://doi.org/10.22323/1.301.0498
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