{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:YJOVJR3AKA7RKEHNP2UQ2UH6MR","short_pith_number":"pith:YJOVJR3A","schema_version":"1.0","canonical_sha256":"c25d54c760503f1510ed7ea90d50fe646118d8ee44939bf9ca155937920aea9b","source":{"kind":"arxiv","id":"2410.06995","version":2},"attestation_state":"computed","paper":{"title":"$\\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Aniruddha Chakraborty, Suvodip Mukherjee","submitted_at":"2024-10-09T15:43:31Z","abstract_excerpt":"Gravitational microlensing in the wave-optics (WO) regime occurs when the Schwarzschild radius of a lensing object is comparable to or smaller than the wavelength of incoming gravitational waves (GWs), producing chromatic amplitude and phase modulations. In contrary, geometric optics effects happen when wavelength is much smaller than the lensing object leading to frequency independent amplifications and phase shifts. GWs can undergo both effects of lensing due to interactions with objects of different scales. To detect and characterize the wave-optics features from a lensed GW, we have develo"},"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":"2410.06995","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"gr-qc","submitted_at":"2024-10-09T15:43:31Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE","astro-ph.IM"],"title_canon_sha256":"c93360c862438369d943e7b52ece41b00e671c346ad2076eda14e5018ce14aeb","abstract_canon_sha256":"bcb7227072c9098abaae1a977021d9e69736121129763ee7969c02a69ee5f40c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:05:35.412850Z","signature_b64":"lSwUTdBSrw9MxURrCusGV4kVxYzWOVqB9GlhdnwnrgsYonsy3lNQxeKHI3q7roH7GXz6Qoq2OtMajxpEqOnhBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c25d54c760503f1510ed7ea90d50fe646118d8ee44939bf9ca155937920aea9b","last_reissued_at":"2026-07-05T11:05:35.412391Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:05:35.412391Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"$\\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Aniruddha Chakraborty, Suvodip Mukherjee","submitted_at":"2024-10-09T15:43:31Z","abstract_excerpt":"Gravitational microlensing in the wave-optics (WO) regime occurs when the Schwarzschild radius of a lensing object is comparable to or smaller than the wavelength of incoming gravitational waves (GWs), producing chromatic amplitude and phase modulations. In contrary, geometric optics effects happen when wavelength is much smaller than the lensing object leading to frequency independent amplifications and phase shifts. GWs can undergo both effects of lensing due to interactions with objects of different scales. To detect and characterize the wave-optics features from a lensed GW, we have develo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.06995","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/2410.06995/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":"2410.06995","created_at":"2026-07-05T11:05:35.412449+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.06995v2","created_at":"2026-07-05T11:05:35.412449+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.06995","created_at":"2026-07-05T11:05:35.412449+00:00"},{"alias_kind":"pith_short_12","alias_value":"YJOVJR3AKA7R","created_at":"2026-07-05T11:05:35.412449+00:00"},{"alias_kind":"pith_short_16","alias_value":"YJOVJR3AKA7RKEHN","created_at":"2026-07-05T11:05:35.412449+00:00"},{"alias_kind":"pith_short_8","alias_value":"YJOVJR3A","created_at":"2026-07-05T11:05:35.412449+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.17765","citing_title":"Effective description of lensed gravitational waves diffracted by stellar fields","ref_index":52,"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":71,"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":25,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22441","citing_title":"How lonely are the Binary Compact Objects Detected by the LIGO-Virgo-KAGRA Collaboration?","ref_index":104,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YJOVJR3AKA7RKEHNP2UQ2UH6MR","json":"https://pith.science/pith/YJOVJR3AKA7RKEHNP2UQ2UH6MR.json","graph_json":"https://pith.science/api/pith-number/YJOVJR3AKA7RKEHNP2UQ2UH6MR/graph.json","events_json":"https://pith.science/api/pith-number/YJOVJR3AKA7RKEHNP2UQ2UH6MR/events.json","paper":"https://pith.science/paper/YJOVJR3A"},"agent_actions":{"view_html":"https://pith.science/pith/YJOVJR3AKA7RKEHNP2UQ2UH6MR","download_json":"https://pith.science/pith/YJOVJR3AKA7RKEHNP2UQ2UH6MR.json","view_paper":"https://pith.science/paper/YJOVJR3A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.06995&json=true","fetch_graph":"https://pith.science/api/pith-number/YJOVJR3AKA7RKEHNP2UQ2UH6MR/graph.json","fetch_events":"https://pith.science/api/pith-number/YJOVJR3AKA7RKEHNP2UQ2UH6MR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YJOVJR3AKA7RKEHNP2UQ2UH6MR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YJOVJR3AKA7RKEHNP2UQ2UH6MR/action/storage_attestation","attest_author":"https://pith.science/pith/YJOVJR3AKA7RKEHNP2UQ2UH6MR/action/author_attestation","sign_citation":"https://pith.science/pith/YJOVJR3AKA7RKEHNP2UQ2UH6MR/action/citation_signature","submit_replication":"https://pith.science/pith/YJOVJR3AKA7RKEHNP2UQ2UH6MR/action/replication_record"}},"created_at":"2026-07-05T11:05:35.412449+00:00","updated_at":"2026-07-05T11:05:35.412449+00:00"}