{"paper":{"title":"HERMES: a Monte Carlo Code for the Propagation of Ultra-High Energy Nuclei","arxiv_id":"1307.4356","primary_cat":"astro-ph.HE","submitted_at":"2013-07-16T17:47:03+00:00","version_compiled":"v1"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13-20260917 on the question bank abstract-p1-20260923, exactly as returned. 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Galactic magnetic fields and nuclear interactions with relic photons of the extragalactic background radiation.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.94,"main_claim_p":0.23,"quantitative":true,"quantitative_p":0.98,"role_probabilities":{"gap":0.0,"method":0.18,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.82,"interpretation":0.0}},{"i":2,"p":0.57,"id":"s2","own":true,"role":"result","text":"In order to show the potential applications of HERMES for astroparticle studies, we estimate the expected flux of UHE nuclei in different astrophysical scenarios, the GZK horizons and we show the expected arrival direction distributions in the presence of turbulent extragalactic magnetic 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