{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:M523S6W4HMP3UE6BNHGX6RRUVC","short_pith_number":"pith:M523S6W4","schema_version":"1.0","canonical_sha256":"6775b97adc3b1fba13c169cd7f4634a8b47d16b76f29ae5045f6a803f44a5918","source":{"kind":"arxiv","id":"1710.05857","version":4},"attestation_state":"computed","paper":{"title":"GRB 170817A as a jet counterpart to gravitational wave trigger GW 170817","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Gavin P Lamb, Shiho Kobayashi","submitted_at":"2017-10-16T16:58:14Z","abstract_excerpt":"{\\it Fermi}/GBM (Gamma-ray Burst Monitor) and INTEGRAL (the International Gamma-ray Astrophysics Laboratory) reported the detection of the $\\gamma$-ray counterpart, GRB 170817A, to the LIGO (Light Interferometer Gravitational-wave Observatory)/{\\it Virgo} gravitational wave detected binary neutron star merger, GW 170817. GRB 170817A is likely to have an internal jet or another origin such as cocoon emission, shock-breakout, or a flare from a viscous disc. In this paper, we assume that the $\\gamma$-ray emission is caused by energy dissipation within a relativistic jet and we model the afterglow"},"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":"1710.05857","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-16T16:58:14Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"6dcc41e9e7bd05209760a310f15627045cc15122e9ffdf66918a7cee8307dc34","abstract_canon_sha256":"6e3b4e6e710d0cb5b0a65f9f44e0ae3d6d03842d375e2dcee14423e59c39b72a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:15:58.899017Z","signature_b64":"elrtF67nfYWkF8zp2vRYZzE960LWFvPDn+z1z0WS3uDga+8AeTMT5uGFBb0YEo3lacS8zNn8lAOFYUyq2gzTAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6775b97adc3b1fba13c169cd7f4634a8b47d16b76f29ae5045f6a803f44a5918","last_reissued_at":"2026-05-18T00:15:58.898388Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:15:58.898388Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GRB 170817A as a jet counterpart to gravitational wave trigger GW 170817","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Gavin P Lamb, Shiho Kobayashi","submitted_at":"2017-10-16T16:58:14Z","abstract_excerpt":"{\\it Fermi}/GBM (Gamma-ray Burst Monitor) and INTEGRAL (the International Gamma-ray Astrophysics Laboratory) reported the detection of the $\\gamma$-ray counterpart, GRB 170817A, to the LIGO (Light Interferometer Gravitational-wave Observatory)/{\\it Virgo} gravitational wave detected binary neutron star merger, GW 170817. GRB 170817A is likely to have an internal jet or another origin such as cocoon emission, shock-breakout, or a flare from a viscous disc. In this paper, we assume that the $\\gamma$-ray emission is caused by energy dissipation within a relativistic jet and we model the afterglow"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.05857","kind":"arxiv","version":4},"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":"1710.05857","created_at":"2026-05-18T00:15:58.898491+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.05857v4","created_at":"2026-05-18T00:15:58.898491+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.05857","created_at":"2026-05-18T00:15:58.898491+00:00"},{"alias_kind":"pith_short_12","alias_value":"M523S6W4HMP3","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"M523S6W4HMP3UE6B","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"M523S6W4","created_at":"2026-05-18T12:31:28.150371+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/M523S6W4HMP3UE6BNHGX6RRUVC","json":"https://pith.science/pith/M523S6W4HMP3UE6BNHGX6RRUVC.json","graph_json":"https://pith.science/api/pith-number/M523S6W4HMP3UE6BNHGX6RRUVC/graph.json","events_json":"https://pith.science/api/pith-number/M523S6W4HMP3UE6BNHGX6RRUVC/events.json","paper":"https://pith.science/paper/M523S6W4"},"agent_actions":{"view_html":"https://pith.science/pith/M523S6W4HMP3UE6BNHGX6RRUVC","download_json":"https://pith.science/pith/M523S6W4HMP3UE6BNHGX6RRUVC.json","view_paper":"https://pith.science/paper/M523S6W4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.05857&json=true","fetch_graph":"https://pith.science/api/pith-number/M523S6W4HMP3UE6BNHGX6RRUVC/graph.json","fetch_events":"https://pith.science/api/pith-number/M523S6W4HMP3UE6BNHGX6RRUVC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M523S6W4HMP3UE6BNHGX6RRUVC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M523S6W4HMP3UE6BNHGX6RRUVC/action/storage_attestation","attest_author":"https://pith.science/pith/M523S6W4HMP3UE6BNHGX6RRUVC/action/author_attestation","sign_citation":"https://pith.science/pith/M523S6W4HMP3UE6BNHGX6RRUVC/action/citation_signature","submit_replication":"https://pith.science/pith/M523S6W4HMP3UE6BNHGX6RRUVC/action/replication_record"}},"created_at":"2026-05-18T00:15:58.898491+00:00","updated_at":"2026-05-18T00:15:58.898491+00:00"}