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Juan Carlos Díaz Vélez (Universidad de Guadalajara)10/10/2017, 08:20
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Segev BenZvi (o=rochester,ou=Institutions,dc=icecube,dc=wisc,dc=edu)10/10/2017, 08:50
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Paolo Desiati (o=uwmad,ou=Institutions,dc=icecube,dc=wisc,dc=edu)10/10/2017, 09:35Invited TalkThis is a summary of the cosmic ray anisotropy observed with the IceCube Observatory. Comparisons with similar experiments are also shown, along with the future perspectives.Go to contribution page
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Zig Hampel-Arias (o=ulb,ou=Institutions,dc=icecube,dc=wisc,dc=edu)10/10/2017, 10:05With its high duty cycle and large field of view ($\sim2$ sr), the High-Altitude Water Cherenkov (HAWC) Observatory continuously surveys the cosmic ray arrival distribution at very high energies ($100$ GeV $-$ $1$ PeV) in the Northern Sky. Previous measurements by other air shower experiments at the TeV scale reveal energy-dependent angular features of the cosmic-ray anisotropy at both...Go to contribution page
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Juan Carlos Díaz Vélez (Universidad de Guadalajara)10/10/2017, 10:35Invited TalkIndividual observations of the sidereal anisotropy in the arrival direction distribution of Galactic cosmic rays are restricted by limited sky coverage. As a result, the power spectrum of the anisotropy obtained from any one measurement displays a systematic correlation between different multipole modes $C_\ell$. We describe the methods used to combine the IceCube and HAWC data, address the...Go to contribution page
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