{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:OWBSKOZMEF3ATISQLQQ3IMLWJM","short_pith_number":"pith:OWBSKOZM","schema_version":"1.0","canonical_sha256":"7583253b2c217609a2505c21b431764b0de670d8c147f3b378e299df79a1011e","source":{"kind":"arxiv","id":"1307.3562","version":2},"attestation_state":"computed","paper":{"title":"Investigating the effect of precession on searches for neutron-star-black-hole binaries with Advanced LIGO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"A. H. Nitz, A. Lundgren, D. Keppel, Duncan A. Brown, Evan Ochsner, I. W. Harry","submitted_at":"2013-07-12T20:00:57Z","abstract_excerpt":"The first direct detection of neutron-star-black-hole binaries will likely be made with gravitational-wave observatories. Advanced LIGO and Advanced Virgo will be able to observe neutron-star-black-hole mergers at a maximum distance of 900Mpc. To acheive this sensitivity, gravitational-wave searches will rely on using a bank of filter waveforms that accurately model the expected gravitational-wave signal. The angular momentum of the black hole is expected to be comparable to the orbital angular momentum. This angular momentum will affect the dynamics of the inspiralling system and alter the ph"},"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":"1307.3562","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2013-07-12T20:00:57Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"a994178a1dc29a9b0b2a1e207a57d1a1f3b62bae51364e2125f6dba66790d3fd","abstract_canon_sha256":"e84a18d3437a53b475edd2d0a1221fd05d89ebed8a58bb47d42e45dd6af332e0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:51:34.145604Z","signature_b64":"kBSX/XjaWRI75kwSqPu5714aIeZnDlxcPaMBLFPriyFbD1ELAmO/OXSQjh/WOikR40h7XJ3LeQnSVehkEVYQAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7583253b2c217609a2505c21b431764b0de670d8c147f3b378e299df79a1011e","last_reissued_at":"2026-05-18T02:51:34.145035Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:51:34.145035Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigating the effect of precession on searches for neutron-star-black-hole binaries with Advanced LIGO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"A. H. Nitz, A. Lundgren, D. Keppel, Duncan A. Brown, Evan Ochsner, I. W. Harry","submitted_at":"2013-07-12T20:00:57Z","abstract_excerpt":"The first direct detection of neutron-star-black-hole binaries will likely be made with gravitational-wave observatories. Advanced LIGO and Advanced Virgo will be able to observe neutron-star-black-hole mergers at a maximum distance of 900Mpc. To acheive this sensitivity, gravitational-wave searches will rely on using a bank of filter waveforms that accurately model the expected gravitational-wave signal. The angular momentum of the black hole is expected to be comparable to the orbital angular momentum. This angular momentum will affect the dynamics of the inspiralling system and alter the ph"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.3562","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":"1307.3562","created_at":"2026-05-18T02:51:34.145121+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.3562v2","created_at":"2026-05-18T02:51:34.145121+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.3562","created_at":"2026-05-18T02:51:34.145121+00:00"},{"alias_kind":"pith_short_12","alias_value":"OWBSKOZMEF3A","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_16","alias_value":"OWBSKOZMEF3ATISQ","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_8","alias_value":"OWBSKOZM","created_at":"2026-05-18T12:27:54.935989+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.10803","citing_title":"Detection of GW200105 with a targeted eccentric search","ref_index":56,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OWBSKOZMEF3ATISQLQQ3IMLWJM","json":"https://pith.science/pith/OWBSKOZMEF3ATISQLQQ3IMLWJM.json","graph_json":"https://pith.science/api/pith-number/OWBSKOZMEF3ATISQLQQ3IMLWJM/graph.json","events_json":"https://pith.science/api/pith-number/OWBSKOZMEF3ATISQLQQ3IMLWJM/events.json","paper":"https://pith.science/paper/OWBSKOZM"},"agent_actions":{"view_html":"https://pith.science/pith/OWBSKOZMEF3ATISQLQQ3IMLWJM","download_json":"https://pith.science/pith/OWBSKOZMEF3ATISQLQQ3IMLWJM.json","view_paper":"https://pith.science/paper/OWBSKOZM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.3562&json=true","fetch_graph":"https://pith.science/api/pith-number/OWBSKOZMEF3ATISQLQQ3IMLWJM/graph.json","fetch_events":"https://pith.science/api/pith-number/OWBSKOZMEF3ATISQLQQ3IMLWJM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OWBSKOZMEF3ATISQLQQ3IMLWJM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OWBSKOZMEF3ATISQLQQ3IMLWJM/action/storage_attestation","attest_author":"https://pith.science/pith/OWBSKOZMEF3ATISQLQQ3IMLWJM/action/author_attestation","sign_citation":"https://pith.science/pith/OWBSKOZMEF3ATISQLQQ3IMLWJM/action/citation_signature","submit_replication":"https://pith.science/pith/OWBSKOZMEF3ATISQLQQ3IMLWJM/action/replication_record"}},"created_at":"2026-05-18T02:51:34.145121+00:00","updated_at":"2026-05-18T02:51:34.145121+00:00"}