{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:QQDKBF4IIQE5ZTATQSWMTCFL2V","short_pith_number":"pith:QQDKBF4I","schema_version":"1.0","canonical_sha256":"8406a097884409dccc1384acc988abd57afddd55efb337402b0a5100cc9505e0","source":{"kind":"arxiv","id":"0708.2106","version":1},"attestation_state":"computed","paper":{"title":"How common are long Gamma-Ray Bursts in the Local Universe?","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) University of Leicester, (3) University of Warwick), Andrew J. Levan (3) ((1) University of Hertfordshire, Nial R. Tanvir (2), Robert Chapman (1), Robert S. Priddey (1)","submitted_at":"2007-08-16T14:45:39Z","abstract_excerpt":"The two closest Gamma-Ray Bursts so far detected (GRBs 980425 & 060218) were both under-luminous, spectrally soft, long duration bursts with smooth, single-peaked light curves. Only of the order of 100 GRBs have measured redshifts, and there are, for example, 2704 GRBs in the BATSE catalogue alone. It is therefore plausible that other nearby GRBs have been observed but not identified as relatively nearby. Here we search for statistical correlations between BATSE long duration GRBs and galaxy samples with recession velocities v <= 11,000 km/s (z = 0.0367, ~ 155 Mpc) selected from two catalogues"},"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":"0708.2106","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-08-16T14:45:39Z","cross_cats_sorted":[],"title_canon_sha256":"aada660b4e812df02dde34a80d23973ecfdcd25240dc5f4e5a1f3fb84389740b","abstract_canon_sha256":"91da6e7750e675f6a5422db9a595d9b0f81d3d6b5b3477d7b0fca36b0490b47f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:05:12.302330Z","signature_b64":"5hIioM+5GHJuWqQGFUPNmAe1czLGXMZZMcE6qROuvCUm/WQU0rvih9NjJah/Kws6TTNnpmRD2TYKpyobcWN9Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8406a097884409dccc1384acc988abd57afddd55efb337402b0a5100cc9505e0","last_reissued_at":"2026-07-04T17:05:12.301930Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:05:12.301930Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"How common are long Gamma-Ray Bursts in the Local Universe?","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) University of Leicester, (3) University of Warwick), Andrew J. Levan (3) ((1) University of Hertfordshire, Nial R. Tanvir (2), Robert Chapman (1), Robert S. Priddey (1)","submitted_at":"2007-08-16T14:45:39Z","abstract_excerpt":"The two closest Gamma-Ray Bursts so far detected (GRBs 980425 & 060218) were both under-luminous, spectrally soft, long duration bursts with smooth, single-peaked light curves. Only of the order of 100 GRBs have measured redshifts, and there are, for example, 2704 GRBs in the BATSE catalogue alone. It is therefore plausible that other nearby GRBs have been observed but not identified as relatively nearby. Here we search for statistical correlations between BATSE long duration GRBs and galaxy samples with recession velocities v <= 11,000 km/s (z = 0.0367, ~ 155 Mpc) selected from two catalogues"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0708.2106","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/0708.2106/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"0708.2106","created_at":"2026-07-04T17:05:12.301991+00:00"},{"alias_kind":"arxiv_version","alias_value":"0708.2106v1","created_at":"2026-07-04T17:05:12.301991+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0708.2106","created_at":"2026-07-04T17:05:12.301991+00:00"},{"alias_kind":"pith_short_12","alias_value":"QQDKBF4IIQE5","created_at":"2026-07-04T17:05:12.301991+00:00"},{"alias_kind":"pith_short_16","alias_value":"QQDKBF4IIQE5ZTAT","created_at":"2026-07-04T17:05:12.301991+00:00"},{"alias_kind":"pith_short_8","alias_value":"QQDKBF4I","created_at":"2026-07-04T17:05:12.301991+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07610","citing_title":"Gamma-ray bursts reveal the history and faint contributors of cosmic reionization","ref_index":13,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QQDKBF4IIQE5ZTATQSWMTCFL2V","json":"https://pith.science/pith/QQDKBF4IIQE5ZTATQSWMTCFL2V.json","graph_json":"https://pith.science/api/pith-number/QQDKBF4IIQE5ZTATQSWMTCFL2V/graph.json","events_json":"https://pith.science/api/pith-number/QQDKBF4IIQE5ZTATQSWMTCFL2V/events.json","paper":"https://pith.science/paper/QQDKBF4I"},"agent_actions":{"view_html":"https://pith.science/pith/QQDKBF4IIQE5ZTATQSWMTCFL2V","download_json":"https://pith.science/pith/QQDKBF4IIQE5ZTATQSWMTCFL2V.json","view_paper":"https://pith.science/paper/QQDKBF4I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0708.2106&json=true","fetch_graph":"https://pith.science/api/pith-number/QQDKBF4IIQE5ZTATQSWMTCFL2V/graph.json","fetch_events":"https://pith.science/api/pith-number/QQDKBF4IIQE5ZTATQSWMTCFL2V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QQDKBF4IIQE5ZTATQSWMTCFL2V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QQDKBF4IIQE5ZTATQSWMTCFL2V/action/storage_attestation","attest_author":"https://pith.science/pith/QQDKBF4IIQE5ZTATQSWMTCFL2V/action/author_attestation","sign_citation":"https://pith.science/pith/QQDKBF4IIQE5ZTATQSWMTCFL2V/action/citation_signature","submit_replication":"https://pith.science/pith/QQDKBF4IIQE5ZTATQSWMTCFL2V/action/replication_record"}},"created_at":"2026-07-04T17:05:12.301991+00:00","updated_at":"2026-07-04T17:05:12.301991+00:00"}