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Telescope Array

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TA correlations with the large-scale structurematter in the Universe distributed anisotropicallyat the scales of UHECR propagationastrophysical sources should follow the matter distribution• arrival directions follow the matter distribution?‣ trace the distribution of galaxies (2MASS XSCz)‣ assume injection spectrum‣ account for propagation‣ get expected skymap‣ compare with data• first observed in 1990s in Yakutsk data• may explain Auger AGN correlations without AGNs

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