{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:YZR43RDJG3VNBKXEKMORS6L7JU","short_pith_number":"pith:YZR43RDJ","schema_version":"1.0","canonical_sha256":"c663cdc46936ead0aae4531d19797f4d0ac9e9e2f055314ecad9c3ea0e411d26","source":{"kind":"arxiv","id":"2503.02186","version":2},"attestation_state":"computed","paper":{"title":"Residual test to search for microlensing signatures in strongly lensed gravitational wave signals","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Bin Hu, Eungwang Seo, Justin Janquart, Martin A. Hendry, Otto A. Hannuksela, Xikai Shan","submitted_at":"2025-03-04T01:49:27Z","abstract_excerpt":"When a gravitational wave signal encounters a massive object, such as a galaxy or galaxy cluster, it undergoes strong gravitational lensing, producing multiple copies of the original signal. These strongly lensed signals exhibit identical waveform morphology in the frequency domain, allowing analysis without the need for complex lens models. However, stellar fields and dark matter substructures within the galactic lens introduce microlensing effects that alter individual signal morphologies. Identifying these microlensing signatures is computationally challenging within Bayesian frameworks. In"},"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":"2503.02186","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2025-03-04T01:49:27Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"00c0cfb2cd8b31c67871c01f384b009fe5cda471cfef909fd8345513ce6ffe29","abstract_canon_sha256":"d4a82c656b7c33d77d10667d5ae953869f705ac269ef23d073854c054884167d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:25:42.530823Z","signature_b64":"o5rR75u7kHRIlP8NnS5MDkJQ8iEtJxp+7Zma9bP/e2BbOBoplmRE+D4cU6eHc3zz4LbjM7a4E0teobPYYTajAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c663cdc46936ead0aae4531d19797f4d0ac9e9e2f055314ecad9c3ea0e411d26","last_reissued_at":"2026-07-05T11:25:42.530375Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:25:42.530375Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Residual test to search for microlensing signatures in strongly lensed gravitational wave signals","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Bin Hu, Eungwang Seo, Justin Janquart, Martin A. Hendry, Otto A. Hannuksela, Xikai Shan","submitted_at":"2025-03-04T01:49:27Z","abstract_excerpt":"When a gravitational wave signal encounters a massive object, such as a galaxy or galaxy cluster, it undergoes strong gravitational lensing, producing multiple copies of the original signal. These strongly lensed signals exhibit identical waveform morphology in the frequency domain, allowing analysis without the need for complex lens models. However, stellar fields and dark matter substructures within the galactic lens introduce microlensing effects that alter individual signal morphologies. Identifying these microlensing signatures is computationally challenging within Bayesian frameworks. In"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.02186","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/2503.02186/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":"2503.02186","created_at":"2026-07-05T11:25:42.530433+00:00"},{"alias_kind":"arxiv_version","alias_value":"2503.02186v2","created_at":"2026-07-05T11:25:42.530433+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2503.02186","created_at":"2026-07-05T11:25:42.530433+00:00"},{"alias_kind":"pith_short_12","alias_value":"YZR43RDJG3VN","created_at":"2026-07-05T11:25:42.530433+00:00"},{"alias_kind":"pith_short_16","alias_value":"YZR43RDJG3VNBKXE","created_at":"2026-07-05T11:25:42.530433+00:00"},{"alias_kind":"pith_short_8","alias_value":"YZR43RDJ","created_at":"2026-07-05T11:25:42.530433+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.17765","citing_title":"Effective description of lensed gravitational waves diffracted by stellar fields","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2606.03346","citing_title":"Model-Independent Search Discards Faint Lensed-Pairs of Gravitational Wave Events in the Sub-Threshold Candidates of GWTC-4","ref_index":72,"is_internal_anchor":false},{"citing_arxiv_id":"2510.11790","citing_title":"False Alarm Rates in Detecting Gravitational Wave Lensing from Astrophysical Coincidences: Insights with Model-Independent Technique GLANCE","ref_index":36,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YZR43RDJG3VNBKXEKMORS6L7JU","json":"https://pith.science/pith/YZR43RDJG3VNBKXEKMORS6L7JU.json","graph_json":"https://pith.science/api/pith-number/YZR43RDJG3VNBKXEKMORS6L7JU/graph.json","events_json":"https://pith.science/api/pith-number/YZR43RDJG3VNBKXEKMORS6L7JU/events.json","paper":"https://pith.science/paper/YZR43RDJ"},"agent_actions":{"view_html":"https://pith.science/pith/YZR43RDJG3VNBKXEKMORS6L7JU","download_json":"https://pith.science/pith/YZR43RDJG3VNBKXEKMORS6L7JU.json","view_paper":"https://pith.science/paper/YZR43RDJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2503.02186&json=true","fetch_graph":"https://pith.science/api/pith-number/YZR43RDJG3VNBKXEKMORS6L7JU/graph.json","fetch_events":"https://pith.science/api/pith-number/YZR43RDJG3VNBKXEKMORS6L7JU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YZR43RDJG3VNBKXEKMORS6L7JU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YZR43RDJG3VNBKXEKMORS6L7JU/action/storage_attestation","attest_author":"https://pith.science/pith/YZR43RDJG3VNBKXEKMORS6L7JU/action/author_attestation","sign_citation":"https://pith.science/pith/YZR43RDJG3VNBKXEKMORS6L7JU/action/citation_signature","submit_replication":"https://pith.science/pith/YZR43RDJG3VNBKXEKMORS6L7JU/action/replication_record"}},"created_at":"2026-07-05T11:25:42.530433+00:00","updated_at":"2026-07-05T11:25:42.530433+00:00"}