{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:Z2A6XZE65ATNUN7GBUDPURGDTC","short_pith_number":"pith:Z2A6XZE6","schema_version":"1.0","canonical_sha256":"ce81ebe49ee826da37e60d06fa44c3989247fee684c89e6a65c989dccc4afeb9","source":{"kind":"arxiv","id":"1310.3008","version":1},"attestation_state":"computed","paper":{"title":"Is the late near-infrared bump in short-hard GRB 130603B due to the Li-Paczynski kilonova?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Da-Ming Wei, Dong Xu, Xue-Feng Wu, Yi-Zhong Fan, Zhi-Ping Jin","submitted_at":"2013-10-11T02:43:59Z","abstract_excerpt":"Short-hard gamma-ray bursts (GRBs) are widely believed to be produced by the merger of two binary compact objects, specifically by two neutron stars or by a neutron star orbiting a black hole. According to the Li-Paczynski kilonova model, the merger would launch sub-relativistic ejecta and a near-infrared/optical transient would then occur, lasting up to days, which is powered by the radioactive decay of heavy elements synthesized in the ejecta. The detection of a late bump using the {\\em Hubble Space Telescope} ({\\em HST}) in the near-infrared afterglow light curve of the short-hard GRB 13060"},"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":"1310.3008","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-11T02:43:59Z","cross_cats_sorted":[],"title_canon_sha256":"db5594c7cc9cd6349737e603b92661af91c51fe3e18ebeab1bb8073b467a59e7","abstract_canon_sha256":"cb8cf9b420aa11e9017118b05c55bfb23a81c44f2a5f225456a6eab7e9434b29"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:10:45.284359Z","signature_b64":"Hv9DV0n7IIFTxqCHNWDfl4nLSSBPdm44nNacXtEvuDK5IaBlgp92iMC0q1DemvNBbVCCNNu7/f2wD+vJpZWwCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ce81ebe49ee826da37e60d06fa44c3989247fee684c89e6a65c989dccc4afeb9","last_reissued_at":"2026-05-18T03:10:45.283818Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:10:45.283818Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Is the late near-infrared bump in short-hard GRB 130603B due to the Li-Paczynski kilonova?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Da-Ming Wei, Dong Xu, Xue-Feng Wu, Yi-Zhong Fan, Zhi-Ping Jin","submitted_at":"2013-10-11T02:43:59Z","abstract_excerpt":"Short-hard gamma-ray bursts (GRBs) are widely believed to be produced by the merger of two binary compact objects, specifically by two neutron stars or by a neutron star orbiting a black hole. According to the Li-Paczynski kilonova model, the merger would launch sub-relativistic ejecta and a near-infrared/optical transient would then occur, lasting up to days, which is powered by the radioactive decay of heavy elements synthesized in the ejecta. The detection of a late bump using the {\\em Hubble Space Telescope} ({\\em HST}) in the near-infrared afterglow light curve of the short-hard GRB 13060"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.3008","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":""},"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":"1310.3008","created_at":"2026-05-18T03:10:45.283903+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.3008v1","created_at":"2026-05-18T03:10:45.283903+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.3008","created_at":"2026-05-18T03:10:45.283903+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z2A6XZE65ATN","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z2A6XZE65ATNUN7G","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z2A6XZE6","created_at":"2026-05-18T12:28:09.283467+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/Z2A6XZE65ATNUN7GBUDPURGDTC","json":"https://pith.science/pith/Z2A6XZE65ATNUN7GBUDPURGDTC.json","graph_json":"https://pith.science/api/pith-number/Z2A6XZE65ATNUN7GBUDPURGDTC/graph.json","events_json":"https://pith.science/api/pith-number/Z2A6XZE65ATNUN7GBUDPURGDTC/events.json","paper":"https://pith.science/paper/Z2A6XZE6"},"agent_actions":{"view_html":"https://pith.science/pith/Z2A6XZE65ATNUN7GBUDPURGDTC","download_json":"https://pith.science/pith/Z2A6XZE65ATNUN7GBUDPURGDTC.json","view_paper":"https://pith.science/paper/Z2A6XZE6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.3008&json=true","fetch_graph":"https://pith.science/api/pith-number/Z2A6XZE65ATNUN7GBUDPURGDTC/graph.json","fetch_events":"https://pith.science/api/pith-number/Z2A6XZE65ATNUN7GBUDPURGDTC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z2A6XZE65ATNUN7GBUDPURGDTC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z2A6XZE65ATNUN7GBUDPURGDTC/action/storage_attestation","attest_author":"https://pith.science/pith/Z2A6XZE65ATNUN7GBUDPURGDTC/action/author_attestation","sign_citation":"https://pith.science/pith/Z2A6XZE65ATNUN7GBUDPURGDTC/action/citation_signature","submit_replication":"https://pith.science/pith/Z2A6XZE65ATNUN7GBUDPURGDTC/action/replication_record"}},"created_at":"2026-05-18T03:10:45.283903+00:00","updated_at":"2026-05-18T03:10:45.283903+00:00"}