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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"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"astro-ph/9308040","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1993-08-27T11:53:55Z","cross_cats_sorted":[],"title_canon_sha256":"380be9c9f0dff0f28afe308b9f583a03b158c5aa606533a4fbfca08fc98f61e8","abstract_canon_sha256":"760fcdb5881d61441e5b22edbdda73a596a91912b54794d2168694af7e36a524"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:12:44.303711Z","signature_b64":"6xO/D8MmZUHU1ANW9muMoosxH1SAZpeOL/AncF5/V0frfegEKIaJpoxi89p8e8WVZnXiVw5oADC2GoixjlLeCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9e0b22cc2bf5fe9f9dcbc322f55ef473e9e1bb5e91b4e253a7fa0d5b5da3a60a","last_reissued_at":"2026-05-18T01:12:44.303342Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:12:44.303342Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"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). 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