{"paper":{"title":"A Possible Explanation for the Peculiar Correlations in the Angular Distribution of Gamma-Ray Bursts","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Eyal Maoz","submitted_at":"1993-08-27T11:53:55Z","abstract_excerpt":"It has been recently discovered that the angular autocorrelation function of gamma-ray bursts exhibits sharp peaks at angular separations of $\\lesssim 4\\deg$ (Quashnock and Lamb 1993), and at $\\gtrsim 176\\deg$ (Narayan and Piran 1993). While an excess of very close pairs of bursts can naturally arise from burst repetition or from a spatial correlation of the burst sources, a physical explanation for an angular correlation on a scale of $\\simeq 180\\deg$ seems inconceivable.\n  We show that both sharp peaks in the correlation function can be explained by a possible bias in the determination of th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9308040","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}