{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:QI7KX2Z65LRFDNYAHKCGWAMOOY","short_pith_number":"pith:QI7KX2Z6","schema_version":"1.0","canonical_sha256":"823eabeb3eeae251b7003a846b018e7625bdca7f9e508f92fc5832e35eb6d433","source":{"kind":"arxiv","id":"2304.06581","version":2},"attestation_state":"computed","paper":{"title":"GRB 211211A-like Events and How Gravitational Waves May Tell Their Origins","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Bin-Bin Zhang, Bing Zhang, Hui Sun, Jun Yang, Lijing Shao, Yacheng Kang, Yi-Han Iris Yin, Yu-Han Yang","submitted_at":"2023-04-13T14:44:21Z","abstract_excerpt":"GRB 211211A is a rare burst with a genuinely long duration, yet its prominent kilonova association provides compelling evidence that this peculiar burst was the result of a compact binary merger. However, the exact nature of the merging objects, whether they were neutron star pairs, neutron star--black hole systems, or neutron star--white dwarf systems, remains unsettled. This {\\it Letter} delves into the rarity of this event and the possibility of using current and next-generation gravitational wave detectors to distinguish between the various types of binary systems. Our research reveals an "},"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":"2304.06581","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-04-13T14:44:21Z","cross_cats_sorted":[],"title_canon_sha256":"8c70d5f160c5e4ba8ff910bec3447da826a4ee493d0050cdd32d1ada0b9db97f","abstract_canon_sha256":"f004b15b7001acd2c6f563ca0aa33dfc242571f7081267a50ca53abec9be0750"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:46:32.116656Z","signature_b64":"8duacC760x+IVHc4cS9bHB2VuO//amIsVTvPK2STAMomGTuJ9LMhLoFQfXjSOsUnUsotrlQVHKqCTgot99KaBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"823eabeb3eeae251b7003a846b018e7625bdca7f9e508f92fc5832e35eb6d433","last_reissued_at":"2026-07-05T06:46:32.116158Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:46:32.116158Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GRB 211211A-like Events and How Gravitational Waves May Tell Their Origins","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Bin-Bin Zhang, Bing Zhang, Hui Sun, Jun Yang, Lijing Shao, Yacheng Kang, Yi-Han Iris Yin, Yu-Han Yang","submitted_at":"2023-04-13T14:44:21Z","abstract_excerpt":"GRB 211211A is a rare burst with a genuinely long duration, yet its prominent kilonova association provides compelling evidence that this peculiar burst was the result of a compact binary merger. However, the exact nature of the merging objects, whether they were neutron star pairs, neutron star--black hole systems, or neutron star--white dwarf systems, remains unsettled. This {\\it Letter} delves into the rarity of this event and the possibility of using current and next-generation gravitational wave detectors to distinguish between the various types of binary systems. Our research reveals an "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2304.06581","kind":"arxiv","version":2},"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/2304.06581/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":"2304.06581","created_at":"2026-07-05T06:46:32.116210+00:00"},{"alias_kind":"arxiv_version","alias_value":"2304.06581v2","created_at":"2026-07-05T06:46:32.116210+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2304.06581","created_at":"2026-07-05T06:46:32.116210+00:00"},{"alias_kind":"pith_short_12","alias_value":"QI7KX2Z65LRF","created_at":"2026-07-05T06:46:32.116210+00:00"},{"alias_kind":"pith_short_16","alias_value":"QI7KX2Z65LRFDNYA","created_at":"2026-07-05T06:46:32.116210+00:00"},{"alias_kind":"pith_short_8","alias_value":"QI7KX2Z6","created_at":"2026-07-05T06:46:32.116210+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.00239","citing_title":"On the Duration of Gamma-Ray Bursts","ref_index":81,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QI7KX2Z65LRFDNYAHKCGWAMOOY","json":"https://pith.science/pith/QI7KX2Z65LRFDNYAHKCGWAMOOY.json","graph_json":"https://pith.science/api/pith-number/QI7KX2Z65LRFDNYAHKCGWAMOOY/graph.json","events_json":"https://pith.science/api/pith-number/QI7KX2Z65LRFDNYAHKCGWAMOOY/events.json","paper":"https://pith.science/paper/QI7KX2Z6"},"agent_actions":{"view_html":"https://pith.science/pith/QI7KX2Z65LRFDNYAHKCGWAMOOY","download_json":"https://pith.science/pith/QI7KX2Z65LRFDNYAHKCGWAMOOY.json","view_paper":"https://pith.science/paper/QI7KX2Z6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2304.06581&json=true","fetch_graph":"https://pith.science/api/pith-number/QI7KX2Z65LRFDNYAHKCGWAMOOY/graph.json","fetch_events":"https://pith.science/api/pith-number/QI7KX2Z65LRFDNYAHKCGWAMOOY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QI7KX2Z65LRFDNYAHKCGWAMOOY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QI7KX2Z65LRFDNYAHKCGWAMOOY/action/storage_attestation","attest_author":"https://pith.science/pith/QI7KX2Z65LRFDNYAHKCGWAMOOY/action/author_attestation","sign_citation":"https://pith.science/pith/QI7KX2Z65LRFDNYAHKCGWAMOOY/action/citation_signature","submit_replication":"https://pith.science/pith/QI7KX2Z65LRFDNYAHKCGWAMOOY/action/replication_record"}},"created_at":"2026-07-05T06:46:32.116210+00:00","updated_at":"2026-07-05T06:46:32.116210+00:00"}