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We show that future Ultra-High Energy Cosmic Ray samples should be able todistinguish whether the sources of UHECRs are hosted by galaxy clusters orordinary galaxies, or whether the sources are uncorrelated with the large-scalestructure of the universe. Moreover, this is true independently of arrivaldirection uncertainty due to magnetic deflection or measurement error. Thereason for this is the simple property that the strength of large-scaleclustering for extragalactic sources depends on their mass, with more massiveobjects, such as galaxy clusters, clustering more strongly than lower massobjects, such as ordinary galaxies.

Large-Angular-Scale Clustering as a Clue to the Source of UHECRs