{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:6O5F747CLMNXQH2RATV4XIFQHF","short_pith_number":"pith:6O5F747C","schema_version":"1.0","canonical_sha256":"f3ba5ff3e25b1b781f5104ebcba0b03969179267fbcb4b0065d5178294147163","source":{"kind":"arxiv","id":"1806.10624","version":2},"attestation_state":"computed","paper":{"title":"A luminous blue kilonova and an off-axis jet from a compact binary merger at z=0.1341","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Kutyrev, E. Troja, G. Ryan, H. van Eerten, L. Piro, M. Im, P. Gatkine, S. B. Cenko, S.-K. Lee, S. Veilleux, T. Sakamoto, Y. Yoon","submitted_at":"2018-06-27T18:01:08Z","abstract_excerpt":"The recent discovery of a faint gamma-ray burst (GRB) coincident with the gravitational wave (GW) event GW 170817 revealed the existence of a population of low-luminosity short duration gamma-ray transients produced by neutron star mergers in the nearby Universe. These events could be routinely detected by existing gamma-ray monitors, yet previous observations failed to identify them without the aid of GW triggers. Here we show that GRB150101B was an analogue of GRB170817A located at a cosmological distance. GRB 150101B was a faint short duration GRB characterized by a bright optical counterpa"},"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":"1806.10624","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-06-27T18:01:08Z","cross_cats_sorted":[],"title_canon_sha256":"5055383a86644af48d2601b2cc4ff04486464a656b833217561e2f2a9ce67d0b","abstract_canon_sha256":"d0e6a2a1becec7f1e5db4e887a31e25fa03247529a33c1a58db6337181352c51"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:00:19.061415Z","signature_b64":"Bii33arsGRazwfg2vxQNIOoCg7r4QxeejRW/D8PxBsfOCN8l3DC0hnUOEXfZcw6qFry4uQJFVrD4mbZFJF+SAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f3ba5ff3e25b1b781f5104ebcba0b03969179267fbcb4b0065d5178294147163","last_reissued_at":"2026-05-18T00:00:19.060772Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:00:19.060772Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A luminous blue kilonova and an off-axis jet from a compact binary merger at z=0.1341","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Kutyrev, E. Troja, G. Ryan, H. van Eerten, L. Piro, M. Im, P. Gatkine, S. B. Cenko, S.-K. Lee, S. Veilleux, T. Sakamoto, Y. Yoon","submitted_at":"2018-06-27T18:01:08Z","abstract_excerpt":"The recent discovery of a faint gamma-ray burst (GRB) coincident with the gravitational wave (GW) event GW 170817 revealed the existence of a population of low-luminosity short duration gamma-ray transients produced by neutron star mergers in the nearby Universe. These events could be routinely detected by existing gamma-ray monitors, yet previous observations failed to identify them without the aid of GW triggers. Here we show that GRB150101B was an analogue of GRB170817A located at a cosmological distance. GRB 150101B was a faint short duration GRB characterized by a bright optical counterpa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.10624","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":"1806.10624","created_at":"2026-05-18T00:00:19.060854+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.10624v2","created_at":"2026-05-18T00:00:19.060854+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.10624","created_at":"2026-05-18T00:00:19.060854+00:00"},{"alias_kind":"pith_short_12","alias_value":"6O5F747CLMNX","created_at":"2026-05-18T12:32:11.075285+00:00"},{"alias_kind":"pith_short_16","alias_value":"6O5F747CLMNXQH2R","created_at":"2026-05-18T12:32:11.075285+00:00"},{"alias_kind":"pith_short_8","alias_value":"6O5F747C","created_at":"2026-05-18T12:32:11.075285+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.13983","citing_title":"Rapid and robust simulation-based inference for kilonovae","ref_index":113,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6O5F747CLMNXQH2RATV4XIFQHF","json":"https://pith.science/pith/6O5F747CLMNXQH2RATV4XIFQHF.json","graph_json":"https://pith.science/api/pith-number/6O5F747CLMNXQH2RATV4XIFQHF/graph.json","events_json":"https://pith.science/api/pith-number/6O5F747CLMNXQH2RATV4XIFQHF/events.json","paper":"https://pith.science/paper/6O5F747C"},"agent_actions":{"view_html":"https://pith.science/pith/6O5F747CLMNXQH2RATV4XIFQHF","download_json":"https://pith.science/pith/6O5F747CLMNXQH2RATV4XIFQHF.json","view_paper":"https://pith.science/paper/6O5F747C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.10624&json=true","fetch_graph":"https://pith.science/api/pith-number/6O5F747CLMNXQH2RATV4XIFQHF/graph.json","fetch_events":"https://pith.science/api/pith-number/6O5F747CLMNXQH2RATV4XIFQHF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6O5F747CLMNXQH2RATV4XIFQHF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6O5F747CLMNXQH2RATV4XIFQHF/action/storage_attestation","attest_author":"https://pith.science/pith/6O5F747CLMNXQH2RATV4XIFQHF/action/author_attestation","sign_citation":"https://pith.science/pith/6O5F747CLMNXQH2RATV4XIFQHF/action/citation_signature","submit_replication":"https://pith.science/pith/6O5F747CLMNXQH2RATV4XIFQHF/action/replication_record"}},"created_at":"2026-05-18T00:00:19.060854+00:00","updated_at":"2026-05-18T00:00:19.060854+00:00"}