{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:JHT25O5DT6AA4LO7VYXLQD5MA5","short_pith_number":"pith:JHT25O5D","schema_version":"1.0","canonical_sha256":"49e7aebba39f800e2ddfae2eb80fac076cc42ef8b0fb99b5eb8e1ef1006cdebb","source":{"kind":"arxiv","id":"2411.13058","version":2},"attestation_state":"computed","paper":{"title":"Detectability of lensed gravitational waves in matched-filtering searches","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alvin K. Y. Li, Eungwang Seo, Heather Fong, Jose M. Ezquiaga, Juno C. L. Chan","submitted_at":"2024-11-20T06:15:06Z","abstract_excerpt":"Gravitational lensing by compact, small-scale intervening masses causes frequency-dependent distortions to gravitational-wave events. The optimal signal-to-noise ratio (SNR) is often used as a proxy for the detectability of exotic signals in gravitational-wave searches. In reality, the detectability of such signals in a matched-filtering search requires comprehensive consideration of match-filtered SNR, signal-consistency test value, and other factors. In this work, we investigate for the first time the detectability of lensed gravitational waves from compact binary coalescences with a match-f"},"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":"2411.13058","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-11-20T06:15:06Z","cross_cats_sorted":[],"title_canon_sha256":"6b53fb0b04facea0b859e6dd8c455af77e48e683ab5a6371059a79b9f4a9b572","abstract_canon_sha256":"d22707ec942cc3cebb109e29f2a8450842584f6c78a29ee3bf77549f16c3870b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:47:33.522049Z","signature_b64":"GYtw78rp8FUryMUJhIP/rm3r4oP0/iiShfpRCNIgsw1jxtNdqqSXbIuFPQeOzSnhbMM4koy99+gOQvA8Q0LzDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"49e7aebba39f800e2ddfae2eb80fac076cc42ef8b0fb99b5eb8e1ef1006cdebb","last_reissued_at":"2026-07-05T10:47:33.521482Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:47:33.521482Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detectability of lensed gravitational waves in matched-filtering searches","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alvin K. Y. Li, Eungwang Seo, Heather Fong, Jose M. Ezquiaga, Juno C. L. Chan","submitted_at":"2024-11-20T06:15:06Z","abstract_excerpt":"Gravitational lensing by compact, small-scale intervening masses causes frequency-dependent distortions to gravitational-wave events. The optimal signal-to-noise ratio (SNR) is often used as a proxy for the detectability of exotic signals in gravitational-wave searches. In reality, the detectability of such signals in a matched-filtering search requires comprehensive consideration of match-filtered SNR, signal-consistency test value, and other factors. In this work, we investigate for the first time the detectability of lensed gravitational waves from compact binary coalescences with a match-f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.13058","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2411.13058/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2411.13058","created_at":"2026-07-05T10:47:33.521558+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.13058v2","created_at":"2026-07-05T10:47:33.521558+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.13058","created_at":"2026-07-05T10:47:33.521558+00:00"},{"alias_kind":"pith_short_12","alias_value":"JHT25O5DT6AA","created_at":"2026-07-05T10:47:33.521558+00:00"},{"alias_kind":"pith_short_16","alias_value":"JHT25O5DT6AA4LO7","created_at":"2026-07-05T10:47:33.521558+00:00"},{"alias_kind":"pith_short_8","alias_value":"JHT25O5D","created_at":"2026-07-05T10:47:33.521558+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.17765","citing_title":"Effective description of lensed gravitational waves diffracted by stellar fields","ref_index":85,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JHT25O5DT6AA4LO7VYXLQD5MA5","json":"https://pith.science/pith/JHT25O5DT6AA4LO7VYXLQD5MA5.json","graph_json":"https://pith.science/api/pith-number/JHT25O5DT6AA4LO7VYXLQD5MA5/graph.json","events_json":"https://pith.science/api/pith-number/JHT25O5DT6AA4LO7VYXLQD5MA5/events.json","paper":"https://pith.science/paper/JHT25O5D"},"agent_actions":{"view_html":"https://pith.science/pith/JHT25O5DT6AA4LO7VYXLQD5MA5","download_json":"https://pith.science/pith/JHT25O5DT6AA4LO7VYXLQD5MA5.json","view_paper":"https://pith.science/paper/JHT25O5D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.13058&json=true","fetch_graph":"https://pith.science/api/pith-number/JHT25O5DT6AA4LO7VYXLQD5MA5/graph.json","fetch_events":"https://pith.science/api/pith-number/JHT25O5DT6AA4LO7VYXLQD5MA5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JHT25O5DT6AA4LO7VYXLQD5MA5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JHT25O5DT6AA4LO7VYXLQD5MA5/action/storage_attestation","attest_author":"https://pith.science/pith/JHT25O5DT6AA4LO7VYXLQD5MA5/action/author_attestation","sign_citation":"https://pith.science/pith/JHT25O5DT6AA4LO7VYXLQD5MA5/action/citation_signature","submit_replication":"https://pith.science/pith/JHT25O5DT6AA4LO7VYXLQD5MA5/action/replication_record"}},"created_at":"2026-07-05T10:47:33.521558+00:00","updated_at":"2026-07-05T10:47:33.521558+00:00"}