{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:HYYKZENHZSIJFB2EUOOJQZFZPS","short_pith_number":"pith:HYYKZENH","schema_version":"1.0","canonical_sha256":"3e30ac91a7cc90928744a39c9864b97c988331e722b340ec27b5fe41bd8158ca","source":{"kind":"arxiv","id":"2208.02725","version":2},"attestation_state":"computed","paper":{"title":"GRB 171205A: Hypernova and Newborn Neutron Star","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"C. L. Fryer, J. A. Rueda, L. M. Becerra, R. Ruffini, Yu Wang","submitted_at":"2022-08-04T15:48:34Z","abstract_excerpt":"GRB 171205A is a low-luminosity, long-duration gamma-ray burst (GRB) associated with SN 2017iuk, a broad-line type Ic supernova (SN). It is consistent with being formed in the core-collapse of a widely separated binary, which we have called the binary-driven hypernova (BdHN) of type III. The core-collapse of the CO star forms a newborn NS ($\\nu$NS) and the SN explosion. Fallback accretion transfers mass and angular momentum to the $\\nu$NS, here assumed to be born non-rotating. The accretion energy injected into the expanding stellar layers powers the prompt emission. The multiwavelength power-"},"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":"2208.02725","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-08-04T15:48:34Z","cross_cats_sorted":[],"title_canon_sha256":"d3427f8306bf5c41e37729b591435afad5d9f01cb316fb9b4c5cc13ea2e72645","abstract_canon_sha256":"096d58fafb610fdd91df954703fea3a4fe0ce8ffc9100c05d9a2c16df4e43354"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:50:45.152496Z","signature_b64":"1CuLBO0eSRE0NmT/HHM4p13Bl3ACrjuQDKvo2Jh4aWPpR5COXmcWBXn3Rd8gwHh/QCO5YTGiEggBkKHQe6ShCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3e30ac91a7cc90928744a39c9864b97c988331e722b340ec27b5fe41bd8158ca","last_reissued_at":"2026-07-05T05:50:45.152067Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:50:45.152067Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GRB 171205A: Hypernova and Newborn Neutron Star","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"C. L. Fryer, J. A. Rueda, L. M. Becerra, R. Ruffini, Yu Wang","submitted_at":"2022-08-04T15:48:34Z","abstract_excerpt":"GRB 171205A is a low-luminosity, long-duration gamma-ray burst (GRB) associated with SN 2017iuk, a broad-line type Ic supernova (SN). It is consistent with being formed in the core-collapse of a widely separated binary, which we have called the binary-driven hypernova (BdHN) of type III. The core-collapse of the CO star forms a newborn NS ($\\nu$NS) and the SN explosion. Fallback accretion transfers mass and angular momentum to the $\\nu$NS, here assumed to be born non-rotating. The accretion energy injected into the expanding stellar layers powers the prompt emission. The multiwavelength power-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2208.02725","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/2208.02725/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":"2208.02725","created_at":"2026-07-05T05:50:45.152126+00:00"},{"alias_kind":"arxiv_version","alias_value":"2208.02725v2","created_at":"2026-07-05T05:50:45.152126+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2208.02725","created_at":"2026-07-05T05:50:45.152126+00:00"},{"alias_kind":"pith_short_12","alias_value":"HYYKZENHZSIJ","created_at":"2026-07-05T05:50:45.152126+00:00"},{"alias_kind":"pith_short_16","alias_value":"HYYKZENHZSIJFB2E","created_at":"2026-07-05T05:50:45.152126+00:00"},{"alias_kind":"pith_short_8","alias_value":"HYYKZENH","created_at":"2026-07-05T05:50:45.152126+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HYYKZENHZSIJFB2EUOOJQZFZPS","json":"https://pith.science/pith/HYYKZENHZSIJFB2EUOOJQZFZPS.json","graph_json":"https://pith.science/api/pith-number/HYYKZENHZSIJFB2EUOOJQZFZPS/graph.json","events_json":"https://pith.science/api/pith-number/HYYKZENHZSIJFB2EUOOJQZFZPS/events.json","paper":"https://pith.science/paper/HYYKZENH"},"agent_actions":{"view_html":"https://pith.science/pith/HYYKZENHZSIJFB2EUOOJQZFZPS","download_json":"https://pith.science/pith/HYYKZENHZSIJFB2EUOOJQZFZPS.json","view_paper":"https://pith.science/paper/HYYKZENH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2208.02725&json=true","fetch_graph":"https://pith.science/api/pith-number/HYYKZENHZSIJFB2EUOOJQZFZPS/graph.json","fetch_events":"https://pith.science/api/pith-number/HYYKZENHZSIJFB2EUOOJQZFZPS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HYYKZENHZSIJFB2EUOOJQZFZPS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HYYKZENHZSIJFB2EUOOJQZFZPS/action/storage_attestation","attest_author":"https://pith.science/pith/HYYKZENHZSIJFB2EUOOJQZFZPS/action/author_attestation","sign_citation":"https://pith.science/pith/HYYKZENHZSIJFB2EUOOJQZFZPS/action/citation_signature","submit_replication":"https://pith.science/pith/HYYKZENHZSIJFB2EUOOJQZFZPS/action/replication_record"}},"created_at":"2026-07-05T05:50:45.152126+00:00","updated_at":"2026-07-05T05:50:45.152126+00:00"}