{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:TBMG43ZPRRWVZXWKX3W5KKMH2K","short_pith_number":"pith:TBMG43ZP","schema_version":"1.0","canonical_sha256":"98586e6f2f8c6d5cdecabeedd52987d285f1accc248b03c620d99c398fa6c350","source":{"kind":"arxiv","id":"1004.5267","version":2},"attestation_state":"computed","paper":{"title":"XRF 100316D/SN 2010bh: clue to the diverse origin of nearby supernova-associated GRBs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Bin-Bin Zhang, Bing Zhang, Dong Xu, En-Wei Liang, Yi-Zhong Fan","submitted_at":"2010-04-29T12:40:26Z","abstract_excerpt":"X-ray Flash (XRF) 100316D, a nearby super-long under-luminous burst with a peak energy E_p \\sim 20 keV, was detected by Swift and was found to be associated with an energetic supernova SN 2010bh. Both the spectral and the temporal behavior of this burst are rather similar to that of XRF 060218, except that the latter was associated with a \"less energetic\" SN 2006aj and had a prominent soft thermal emission component in the spectrum. We analyze the spectral and temporal properties of this burst, and interpret the prompt gamma-ray emission and the early X-ray plateau emission as synchrotron emis"},"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":"1004.5267","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-04-29T12:40:26Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"f61fcd3cb63c4c8e5d476b6a56d7c54a1936b06e8a1dde6913b8ebf3419c9887","abstract_canon_sha256":"9a8866e7dbca1a1f09ed633e48092debdf40eca239ff6bc7ad98ab51772c9739"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:36:16.411892Z","signature_b64":"EOk5i6+zD8LTQOXEEH/udQTeF1JL+uaYZ4BBnnDdwY9UCKLcXRjKP/45QVlW4Uk60wMKugAv3Qg7rwUxpVQGAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"98586e6f2f8c6d5cdecabeedd52987d285f1accc248b03c620d99c398fa6c350","last_reissued_at":"2026-05-18T03:36:16.411288Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:36:16.411288Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"XRF 100316D/SN 2010bh: clue to the diverse origin of nearby supernova-associated GRBs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Bin-Bin Zhang, Bing Zhang, Dong Xu, En-Wei Liang, Yi-Zhong Fan","submitted_at":"2010-04-29T12:40:26Z","abstract_excerpt":"X-ray Flash (XRF) 100316D, a nearby super-long under-luminous burst with a peak energy E_p \\sim 20 keV, was detected by Swift and was found to be associated with an energetic supernova SN 2010bh. Both the spectral and the temporal behavior of this burst are rather similar to that of XRF 060218, except that the latter was associated with a \"less energetic\" SN 2006aj and had a prominent soft thermal emission component in the spectrum. We analyze the spectral and temporal properties of this burst, and interpret the prompt gamma-ray emission and the early X-ray plateau emission as synchrotron emis"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1004.5267","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":""},"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":"1004.5267","created_at":"2026-05-18T03:36:16.411387+00:00"},{"alias_kind":"arxiv_version","alias_value":"1004.5267v2","created_at":"2026-05-18T03:36:16.411387+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1004.5267","created_at":"2026-05-18T03:36:16.411387+00:00"},{"alias_kind":"pith_short_12","alias_value":"TBMG43ZPRRWV","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_16","alias_value":"TBMG43ZPRRWVZXWK","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_8","alias_value":"TBMG43ZP","created_at":"2026-05-18T12:26:13.927090+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/TBMG43ZPRRWVZXWKX3W5KKMH2K","json":"https://pith.science/pith/TBMG43ZPRRWVZXWKX3W5KKMH2K.json","graph_json":"https://pith.science/api/pith-number/TBMG43ZPRRWVZXWKX3W5KKMH2K/graph.json","events_json":"https://pith.science/api/pith-number/TBMG43ZPRRWVZXWKX3W5KKMH2K/events.json","paper":"https://pith.science/paper/TBMG43ZP"},"agent_actions":{"view_html":"https://pith.science/pith/TBMG43ZPRRWVZXWKX3W5KKMH2K","download_json":"https://pith.science/pith/TBMG43ZPRRWVZXWKX3W5KKMH2K.json","view_paper":"https://pith.science/paper/TBMG43ZP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1004.5267&json=true","fetch_graph":"https://pith.science/api/pith-number/TBMG43ZPRRWVZXWKX3W5KKMH2K/graph.json","fetch_events":"https://pith.science/api/pith-number/TBMG43ZPRRWVZXWKX3W5KKMH2K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TBMG43ZPRRWVZXWKX3W5KKMH2K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TBMG43ZPRRWVZXWKX3W5KKMH2K/action/storage_attestation","attest_author":"https://pith.science/pith/TBMG43ZPRRWVZXWKX3W5KKMH2K/action/author_attestation","sign_citation":"https://pith.science/pith/TBMG43ZPRRWVZXWKX3W5KKMH2K/action/citation_signature","submit_replication":"https://pith.science/pith/TBMG43ZPRRWVZXWKX3W5KKMH2K/action/replication_record"}},"created_at":"2026-05-18T03:36:16.411387+00:00","updated_at":"2026-05-18T03:36:16.411387+00:00"}