{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:DOQIJCSGJFI3W7JVVGU35MXHOF","short_pith_number":"pith:DOQIJCSG","schema_version":"1.0","canonical_sha256":"1ba0848a464951bb7d35a9a9beb2e77153a0373555e7220a6bb05d143267c01e","source":{"kind":"arxiv","id":"2105.07011","version":2},"attestation_state":"computed","paper":{"title":"Event rate predictions of strongly lensed gravitational waves with detector networks and more realistic templates","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Kai Liao, Lilan Yang, Marek Biesiada, Shichao Wu, Xuheng Ding, Zhiqiang You, Zhoujian Cao, Zong-Hong Zhu","submitted_at":"2021-05-14T18:00:41Z","abstract_excerpt":"Strong lensing of gravitational waves (GWs) is attracting growing attention of the community. The event rates of lensed GWs by galaxies were predicted in numerous papers, which used some approximations to evaluate the GW strains detectable by a single detector. The joint-detection of GW signals by a network of instruments will increase the detecting ability of fainter and farther GW signals, which could increase the detection rate of the lensed GWs, especially for the 3rd generation detectors, e.g., Einstein Telescope (ET) and Cosmic Explorer (CE). Moreover, realistic GW templates will improve"},"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":"2105.07011","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2021-05-14T18:00:41Z","cross_cats_sorted":[],"title_canon_sha256":"fcab5fcd566c9979edd1bf19e019a6533dac5e0abe156bb8a18eed2f35a2a91e","abstract_canon_sha256":"5ec25c32e97f711d37dd8d5b868c9ec4ea07e0818391ec17b522e57aa317dd58"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:34:25.492540Z","signature_b64":"3Vi2YUT9/O3kizDAlu0aeTVGu86iN8d2gOcWS4ELa9IWgraDjp5Wh75h6M7sYyLKX23jKQUm3nPRAzxim0vdDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1ba0848a464951bb7d35a9a9beb2e77153a0373555e7220a6bb05d143267c01e","last_reissued_at":"2026-07-05T03:34:25.492031Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:34:25.492031Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Event rate predictions of strongly lensed gravitational waves with detector networks and more realistic templates","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Kai Liao, Lilan Yang, Marek Biesiada, Shichao Wu, Xuheng Ding, Zhiqiang You, Zhoujian Cao, Zong-Hong Zhu","submitted_at":"2021-05-14T18:00:41Z","abstract_excerpt":"Strong lensing of gravitational waves (GWs) is attracting growing attention of the community. The event rates of lensed GWs by galaxies were predicted in numerous papers, which used some approximations to evaluate the GW strains detectable by a single detector. The joint-detection of GW signals by a network of instruments will increase the detecting ability of fainter and farther GW signals, which could increase the detection rate of the lensed GWs, especially for the 3rd generation detectors, e.g., Einstein Telescope (ET) and Cosmic Explorer (CE). Moreover, realistic GW templates will improve"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.07011","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/2105.07011/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":"2105.07011","created_at":"2026-07-05T03:34:25.492097+00:00"},{"alias_kind":"arxiv_version","alias_value":"2105.07011v2","created_at":"2026-07-05T03:34:25.492097+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2105.07011","created_at":"2026-07-05T03:34:25.492097+00:00"},{"alias_kind":"pith_short_12","alias_value":"DOQIJCSGJFI3","created_at":"2026-07-05T03:34:25.492097+00:00"},{"alias_kind":"pith_short_16","alias_value":"DOQIJCSGJFI3W7JV","created_at":"2026-07-05T03:34:25.492097+00:00"},{"alias_kind":"pith_short_8","alias_value":"DOQIJCSG","created_at":"2026-07-05T03:34:25.492097+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07120","citing_title":"Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers","ref_index":78,"is_internal_anchor":true},{"citing_arxiv_id":"2606.31531","citing_title":"Probing globular clusters parameters through gravitational wave lensing with stellar-mass black hole binaries","ref_index":12,"is_internal_anchor":false},{"citing_arxiv_id":"2512.10344","citing_title":"Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations","ref_index":16,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DOQIJCSGJFI3W7JVVGU35MXHOF","json":"https://pith.science/pith/DOQIJCSGJFI3W7JVVGU35MXHOF.json","graph_json":"https://pith.science/api/pith-number/DOQIJCSGJFI3W7JVVGU35MXHOF/graph.json","events_json":"https://pith.science/api/pith-number/DOQIJCSGJFI3W7JVVGU35MXHOF/events.json","paper":"https://pith.science/paper/DOQIJCSG"},"agent_actions":{"view_html":"https://pith.science/pith/DOQIJCSGJFI3W7JVVGU35MXHOF","download_json":"https://pith.science/pith/DOQIJCSGJFI3W7JVVGU35MXHOF.json","view_paper":"https://pith.science/paper/DOQIJCSG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2105.07011&json=true","fetch_graph":"https://pith.science/api/pith-number/DOQIJCSGJFI3W7JVVGU35MXHOF/graph.json","fetch_events":"https://pith.science/api/pith-number/DOQIJCSGJFI3W7JVVGU35MXHOF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DOQIJCSGJFI3W7JVVGU35MXHOF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DOQIJCSGJFI3W7JVVGU35MXHOF/action/storage_attestation","attest_author":"https://pith.science/pith/DOQIJCSGJFI3W7JVVGU35MXHOF/action/author_attestation","sign_citation":"https://pith.science/pith/DOQIJCSGJFI3W7JVVGU35MXHOF/action/citation_signature","submit_replication":"https://pith.science/pith/DOQIJCSGJFI3W7JVVGU35MXHOF/action/replication_record"}},"created_at":"2026-07-05T03:34:25.492097+00:00","updated_at":"2026-07-05T03:34:25.492097+00:00"}