{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:BOXSREWZRZHN2NQ27HRJ2XKEP4","short_pith_number":"pith:BOXSREWZ","schema_version":"1.0","canonical_sha256":"0baf2892d98e4edd361af9e29d5d447f05aadb7a849cd291e4a44f89ffba52bc","source":{"kind":"arxiv","id":"1603.08072","version":2},"attestation_state":"computed","paper":{"title":"Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Atsushi Nishizawa, Atsushi Taruya, Toshiya Namikawa","submitted_at":"2016-03-26T04:30:15Z","abstract_excerpt":"The first discovery of the gravitational wave (GW) event, GW150914, suggests a higher merger rate of black-hole (BH) binaries. If this is true, a number of BH binaries will be observed via the second-generation GW detectors, and the statistical properties of the observed BH binaries can be scrutinized. A naive but important question to ask is whether the spatial distribution of BH binaries faithfully traces the matter inhomogeneities in the Universe or not. Although the BH binaries are thought to be formed inside the galaxies in most of the scenarios, there is no observational evidence to conf"},"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":"1603.08072","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-03-26T04:30:15Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"c43663cecfee8fa9f3d4171bcf030662f60a2eff6c4ef8d34c118e50772aa0bc","abstract_canon_sha256":"c8dad9a3941107a7f22432fc23703add7b089e5436ced9468c9c280878712593"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:11:12.393433Z","signature_b64":"QLojun8/Gjb9/P96ph8w554bHLWkSlpLOqtPOCK7+DxQB/ARjQGMOk+8ZBY15heabFSXAidaEOW+fXBED36pDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0baf2892d98e4edd361af9e29d5d447f05aadb7a849cd291e4a44f89ffba52bc","last_reissued_at":"2026-05-18T01:11:12.392781Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:11:12.392781Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.CO","authors_text":"Atsushi Nishizawa, Atsushi Taruya, Toshiya Namikawa","submitted_at":"2016-03-26T04:30:15Z","abstract_excerpt":"The first discovery of the gravitational wave (GW) event, GW150914, suggests a higher merger rate of black-hole (BH) binaries. If this is true, a number of BH binaries will be observed via the second-generation GW detectors, and the statistical properties of the observed BH binaries can be scrutinized. A naive but important question to ask is whether the spatial distribution of BH binaries faithfully traces the matter inhomogeneities in the Universe or not. Although the BH binaries are thought to be formed inside the galaxies in most of the scenarios, there is no observational evidence to conf"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.08072","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":"1603.08072","created_at":"2026-05-18T01:11:12.392869+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.08072v2","created_at":"2026-05-18T01:11:12.392869+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.08072","created_at":"2026-05-18T01:11:12.392869+00:00"},{"alias_kind":"pith_short_12","alias_value":"BOXSREWZRZHN","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_16","alias_value":"BOXSREWZRZHN2NQ2","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_8","alias_value":"BOXSREWZ","created_at":"2026-05-18T12:30:07.202191+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2506.10469","citing_title":"Constraining the lensing dispersion from the angular clustering of binary black hole mergers","ref_index":55,"is_internal_anchor":true},{"citing_arxiv_id":"2603.13053","citing_title":"A unified harmonic framework for dark siren cosmology","ref_index":25,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BOXSREWZRZHN2NQ27HRJ2XKEP4","json":"https://pith.science/pith/BOXSREWZRZHN2NQ27HRJ2XKEP4.json","graph_json":"https://pith.science/api/pith-number/BOXSREWZRZHN2NQ27HRJ2XKEP4/graph.json","events_json":"https://pith.science/api/pith-number/BOXSREWZRZHN2NQ27HRJ2XKEP4/events.json","paper":"https://pith.science/paper/BOXSREWZ"},"agent_actions":{"view_html":"https://pith.science/pith/BOXSREWZRZHN2NQ27HRJ2XKEP4","download_json":"https://pith.science/pith/BOXSREWZRZHN2NQ27HRJ2XKEP4.json","view_paper":"https://pith.science/paper/BOXSREWZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.08072&json=true","fetch_graph":"https://pith.science/api/pith-number/BOXSREWZRZHN2NQ27HRJ2XKEP4/graph.json","fetch_events":"https://pith.science/api/pith-number/BOXSREWZRZHN2NQ27HRJ2XKEP4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BOXSREWZRZHN2NQ27HRJ2XKEP4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BOXSREWZRZHN2NQ27HRJ2XKEP4/action/storage_attestation","attest_author":"https://pith.science/pith/BOXSREWZRZHN2NQ27HRJ2XKEP4/action/author_attestation","sign_citation":"https://pith.science/pith/BOXSREWZRZHN2NQ27HRJ2XKEP4/action/citation_signature","submit_replication":"https://pith.science/pith/BOXSREWZRZHN2NQ27HRJ2XKEP4/action/replication_record"}},"created_at":"2026-05-18T01:11:12.392869+00:00","updated_at":"2026-05-18T01:11:12.392869+00:00"}