{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:KIEAUKNXWN2NUISGKJCG77NFKE","short_pith_number":"pith:KIEAUKNX","schema_version":"1.0","canonical_sha256":"52080a29b7b374da224652446ffda551127a7d7eb07c16c4d9c30a566fd727e0","source":{"kind":"arxiv","id":"1706.03000","version":2},"attestation_state":"computed","paper":{"title":"Electromagnetic Counterparts to Structured Jets from Gravitational Wave Detected Mergers","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":"2017-06-09T15:34:38Z","abstract_excerpt":"We show the peak magnitude for orphan afterglows from the jets of gravitational wave (GW) detected black-hole/neutron star - neutron star (BH/NS-NS) mergers highly depends on the jet half-opening angle $\\theta_j$. Short $\\gamma$-ray bursts (GRB) with a homogeneous jet structure and $\\theta_j>10^\\circ$, the orphan afterglow viewed at the typical inclination for a GW detected event, 38$^\\circ$, is brighter at optical frequencies than the comparable macronova emission. Structured jets, where the energetics and Lorentz factor $\\Gamma$ vary with angle from the central axis, may have low-$\\Gamma$ co"},"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":"1706.03000","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-06-09T15:34:38Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"a58a2da09b7efe59ececee950fac8398c12e01b13ab1f73befbd665d113cc018","abstract_canon_sha256":"f94cfa7d62cc470525901eea19b0895bd5b998b221e14815096f075fa306cf3f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:32:42.823620Z","signature_b64":"24ksQqIzjdSnMLYT/JbUE73XZBPt9GaT5hSJW7rPq+USBITVBukl7lTL7FbTuIKCVOkU9wlgz8QvzmZpmNdHBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"52080a29b7b374da224652446ffda551127a7d7eb07c16c4d9c30a566fd727e0","last_reissued_at":"2026-05-18T00:32:42.822944Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:32:42.822944Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Electromagnetic Counterparts to Structured Jets from Gravitational Wave Detected Mergers","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":"2017-06-09T15:34:38Z","abstract_excerpt":"We show the peak magnitude for orphan afterglows from the jets of gravitational wave (GW) detected black-hole/neutron star - neutron star (BH/NS-NS) mergers highly depends on the jet half-opening angle $\\theta_j$. Short $\\gamma$-ray bursts (GRB) with a homogeneous jet structure and $\\theta_j>10^\\circ$, the orphan afterglow viewed at the typical inclination for a GW detected event, 38$^\\circ$, is brighter at optical frequencies than the comparable macronova emission. Structured jets, where the energetics and Lorentz factor $\\Gamma$ vary with angle from the central axis, may have low-$\\Gamma$ co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.03000","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":"1706.03000","created_at":"2026-05-18T00:32:42.823043+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.03000v2","created_at":"2026-05-18T00:32:42.823043+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.03000","created_at":"2026-05-18T00:32:42.823043+00:00"},{"alias_kind":"pith_short_12","alias_value":"KIEAUKNXWN2N","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_16","alias_value":"KIEAUKNXWN2NUISG","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_8","alias_value":"KIEAUKNX","created_at":"2026-05-18T12:31:24.725408+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.13719","citing_title":"The Very Late Time Afterglow of GW170817 Favors a Wobbling Jet","ref_index":9,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KIEAUKNXWN2NUISGKJCG77NFKE","json":"https://pith.science/pith/KIEAUKNXWN2NUISGKJCG77NFKE.json","graph_json":"https://pith.science/api/pith-number/KIEAUKNXWN2NUISGKJCG77NFKE/graph.json","events_json":"https://pith.science/api/pith-number/KIEAUKNXWN2NUISGKJCG77NFKE/events.json","paper":"https://pith.science/paper/KIEAUKNX"},"agent_actions":{"view_html":"https://pith.science/pith/KIEAUKNXWN2NUISGKJCG77NFKE","download_json":"https://pith.science/pith/KIEAUKNXWN2NUISGKJCG77NFKE.json","view_paper":"https://pith.science/paper/KIEAUKNX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.03000&json=true","fetch_graph":"https://pith.science/api/pith-number/KIEAUKNXWN2NUISGKJCG77NFKE/graph.json","fetch_events":"https://pith.science/api/pith-number/KIEAUKNXWN2NUISGKJCG77NFKE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KIEAUKNXWN2NUISGKJCG77NFKE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KIEAUKNXWN2NUISGKJCG77NFKE/action/storage_attestation","attest_author":"https://pith.science/pith/KIEAUKNXWN2NUISGKJCG77NFKE/action/author_attestation","sign_citation":"https://pith.science/pith/KIEAUKNXWN2NUISGKJCG77NFKE/action/citation_signature","submit_replication":"https://pith.science/pith/KIEAUKNXWN2NUISGKJCG77NFKE/action/replication_record"}},"created_at":"2026-05-18T00:32:42.823043+00:00","updated_at":"2026-05-18T00:32:42.823043+00:00"}