| Title: | Supergalactic Structure of Energy-Angle Correlations |
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| Authors: | ID Lundquist, Jon Paul, UNG (Author)
ID Sokolsky, P. (Author), et al. |
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| Files: |  ICRC2019_343.pdf (1,66 MB)
MD5: C157261FCE8CDCDB5ADD280F7196F122
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| Language: | English |
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| Work type: | Not categorized |
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| Typology: | 1.08 - Published Scientific Conference Contribution |
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| Organization: | UNG - University of Nova Gorica
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| Abstract: | Evidence for the supergalactic structure of multiplets (energy-angle correlations) has previously been shown using ultra-high energy cosmic ray (UHECR) data from Telescope Array (TA) with energies above 10^19 eV. The supergalactic deflection hypothesis (that UHECR sources and intervening magnetic fields are correlated) is measured by the all-sky behavior of the strength of
intermediate-scale correlations. The multiplets are measured in spherical surface wedge bins of the field-of-view to account for uniform and random magnetic fields. The structure found is consistent with the previously published energy spectrum anisotropy results of TA and toy-model simulations of a supergalactic magnetic sheet. The 7 year data post-trial significance of this feature appearing by chance, on an isotropic sky, was found by Monte Carlo simulation to be ∼4σ. The analysis has now been applied to 10 years of data. |
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| Keywords: | Cosmic rays, UHECR, energy spectrum, magnetic deflection, large-scale structure, supergalactic, multiplets |
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| Publication status: | Published |
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| Year of publishing: | 2020 |
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| Number of pages: | 8 |
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| PID: | 20.500.12556/RUNG-5160-2e6331a1-99ad-1d05-78fa-651c7bb12858  |
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| COBISS.SI-ID: | 12844547 |
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| NUK URN: | URN:SI:UNG:REP:SAUQ2GYH |
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| Publication date in RUNG: | 27.04.2020 |
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| Views: | 3410 |
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| Downloads: | 89 |
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