Speaker
Frank McNally
Description
The complete IceCube Observatory has collected over 620 billion cosmic-ray induced muon events from May 2011 to May 2021. These unprecedented statistics make it possible to observe significant structure in the cosmic-ray arrival direction distribution at both higher cosmic-ray energies and smaller angular scales. Combined with improved simulation and systematics, we can provide a newly detailed assessment of the energy- and time-dependence of the cosmic-ray anisotropy in the Southern Hemisphere. We present the preliminary results from a study with the extended event sample.
Collaboration name | IceCube Collaboration |
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Primary authors
Rasha Abbasi
(Loyola University Chicago)
Paolo Desiati
(University of Wisconsin - Madison)
Juan Carlos Diaz Velez
(Universidad de Guadalajara-CUValles)
Frank McNally