{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:JTV52YWZRQB5WFN5OGWTZQ2FCM","short_pith_number":"pith:JTV52YWZ","schema_version":"1.0","canonical_sha256":"4cebdd62d98c03db15bd71ad3cc3451333d6770dd3968d9a179388f25cc0aa56","source":{"kind":"arxiv","id":"1809.10727","version":1},"attestation_state":"computed","paper":{"title":"Constraining the Inclination of Binary Mergers from Gravitational-wave Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Joseph C. Mills, Samantha A. Usman, Stephen Fairhurst","submitted_at":"2018-09-27T19:04:28Z","abstract_excerpt":"Much of the information we hope to extract from the gravitational-waves signatures of compact binaries is only obtainable when we can accurately constrain the inclination of the source. In this paper, we discuss in detail a degeneracy between the measurement of the binary distance and inclination which limits our ability to accurately measure the inclination using gravitational waves alone. This degeneracy is exacerbated by the expected distribution of events in the universe, which leads us to prefer face-on systems at a greater distance. We use a simplified model that only considers the binar"},"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":"1809.10727","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-09-27T19:04:28Z","cross_cats_sorted":[],"title_canon_sha256":"82b1e36dc5c0f2b148363009738c37524ca598d90be36aabaa019c1298345aed","abstract_canon_sha256":"3ad8bcd0fb884ac27b28980a30f9179a7cd923a0e6c0946d362c5c5f21dae4a8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:44:22.322417Z","signature_b64":"eSO5y9AdLEmMZ0/jovBMs6Jo/z6jwazIiq+WMylEgdkkk/2+N+htdAfTqO89ZhbBATOpKCFXFWwiZ9LmahSBAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4cebdd62d98c03db15bd71ad3cc3451333d6770dd3968d9a179388f25cc0aa56","last_reissued_at":"2026-05-17T23:44:22.321775Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:44:22.321775Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining the Inclination of Binary Mergers from Gravitational-wave Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Joseph C. Mills, Samantha A. Usman, Stephen Fairhurst","submitted_at":"2018-09-27T19:04:28Z","abstract_excerpt":"Much of the information we hope to extract from the gravitational-waves signatures of compact binaries is only obtainable when we can accurately constrain the inclination of the source. In this paper, we discuss in detail a degeneracy between the measurement of the binary distance and inclination which limits our ability to accurately measure the inclination using gravitational waves alone. This degeneracy is exacerbated by the expected distribution of events in the universe, which leads us to prefer face-on systems at a greater distance. We use a simplified model that only considers the binar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.10727","kind":"arxiv","version":1},"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":"1809.10727","created_at":"2026-05-17T23:44:22.321875+00:00"},{"alias_kind":"arxiv_version","alias_value":"1809.10727v1","created_at":"2026-05-17T23:44:22.321875+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1809.10727","created_at":"2026-05-17T23:44:22.321875+00:00"},{"alias_kind":"pith_short_12","alias_value":"JTV52YWZRQB5","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_16","alias_value":"JTV52YWZRQB5WFN5","created_at":"2026-05-18T12:32:31.084164+00:00"},{"alias_kind":"pith_short_8","alias_value":"JTV52YWZ","created_at":"2026-05-18T12:32:31.084164+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.23554","citing_title":"Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope","ref_index":89,"is_internal_anchor":true},{"citing_arxiv_id":"2605.11703","citing_title":"GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors","ref_index":217,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11903","citing_title":"Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects","ref_index":149,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JTV52YWZRQB5WFN5OGWTZQ2FCM","json":"https://pith.science/pith/JTV52YWZRQB5WFN5OGWTZQ2FCM.json","graph_json":"https://pith.science/api/pith-number/JTV52YWZRQB5WFN5OGWTZQ2FCM/graph.json","events_json":"https://pith.science/api/pith-number/JTV52YWZRQB5WFN5OGWTZQ2FCM/events.json","paper":"https://pith.science/paper/JTV52YWZ"},"agent_actions":{"view_html":"https://pith.science/pith/JTV52YWZRQB5WFN5OGWTZQ2FCM","download_json":"https://pith.science/pith/JTV52YWZRQB5WFN5OGWTZQ2FCM.json","view_paper":"https://pith.science/paper/JTV52YWZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1809.10727&json=true","fetch_graph":"https://pith.science/api/pith-number/JTV52YWZRQB5WFN5OGWTZQ2FCM/graph.json","fetch_events":"https://pith.science/api/pith-number/JTV52YWZRQB5WFN5OGWTZQ2FCM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JTV52YWZRQB5WFN5OGWTZQ2FCM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JTV52YWZRQB5WFN5OGWTZQ2FCM/action/storage_attestation","attest_author":"https://pith.science/pith/JTV52YWZRQB5WFN5OGWTZQ2FCM/action/author_attestation","sign_citation":"https://pith.science/pith/JTV52YWZRQB5WFN5OGWTZQ2FCM/action/citation_signature","submit_replication":"https://pith.science/pith/JTV52YWZRQB5WFN5OGWTZQ2FCM/action/replication_record"}},"created_at":"2026-05-17T23:44:22.321875+00:00","updated_at":"2026-05-17T23:44:22.321875+00:00"}