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The model takes into account a rigidity-dependent magnetic field blurring and an energy-dependent evolution of the catalog contribution shaped by interactions during propagation.\n\n  We find that a model containing a flux contribution from the starburst galaxy catalog of around 20% at 40 EeV with a magnetic field blurring of around 20\u00b0 for a rigidity of 10 EV provides a fair simultaneous description of all three observables.\n  The starburst galaxy model is favored with a significance of 4.5\u03c3 (considering experimental systematic effects) compared to a reference model with only homogeneously distributed background sources. By investigating a scenario with Centaurus A as a single source in combination with the homogeneous background, we confirm that this region of the sky provides the dominant contribution to the observed anisotropy signal. Models containing a catalog of jetted active galactic nuclei whose flux scales with the \u03b3-ray emission are, however, disfavored as they cannot adequately describe the measured arrival directions.<\/jats:p>","DOI":"10.1088\/1475-7516\/2024\/01\/022","type":"journal-article","created":{"date-parts":[[2024,1,11]],"date-time":"2024-01-11T15:22:47Z","timestamp":1704986567000},"page":"022","update-policy":"https:\/\/doi.org\/10.1088\/crossmark-policy","source":"Crossref","is-referenced-by-count":31,"title":["Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger Observatory"],"prefix":"10.1088","volume":"2024","author":[{"given":"A.","family":"Abdul 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