{"as_of":"2026-08-11T01:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2e7e540008a94f5edf96e49efe0b6d212c228b422e3f8df058ee5ba04a403b84","coverage":[{"denominator":107,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T17:37:27.770363Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2502.00844/citation-record","integrity":"/paper/2502.00844/integrity","json":"/paper/2502.00844/citation-record.json","paper":"/paper/2502.00844"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.395573Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.395573Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:89d7951076dd4b6d9fcdf0620f575eff43bad2a1ac0547072932c62ec53f761c","observation_id":"ebbdd965-e464-4efa-8427-fe0672cbd6e5","resolution":{"observed_at":"2026-08-09T17:37:27.395573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.400427Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.400427Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:0c8438407ac5b70c8cb005ff64b32bde75272cee647d330c60a3b44d36a4ab78","observation_id":"ae5851dd-0fe9-4e89-8f6f-17615c0102db","resolution":{"observed_at":"2026-08-09T17:37:27.400427Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.404464Z","title":"at- tached","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.404464Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:0d86f28faab6bfa07c4c73de91335ea41453226c5b9573c271a4bb88ad1a34b0","observation_id":"382b5903-6fca-4957-9076-3da505d09458","resolution":{"observed_at":"2026-08-09T17:37:27.404464Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.409218Z","title":"Dhurandhar, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.409218Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:ace8a4464d47f987c5afda057806ca38205b7fae7cf4edfdca152eada5b8d2e8","observation_id":"3845cb0f-212d-49e4-a49c-f102c6598397","resolution":{"observed_at":"2026-08-09T17:37:27.409218Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1411.4547","last_updated":"2014-11-17T16:55:23Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2014-11-17T16:55:23Z","title":"Advanced LIGO","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1411.4547","snapshot_observed_at":"2026-08-09T17:37:27.412542Z","title":"Aasi et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.412542Z"},"links":{"cited_paper":"/paper/1411.4547","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:66e17f92a939f5df995038863aa41973cc78b1c52d4ef7288ef89f8bd49051f6","observation_id":"98fd32ae-6113-404a-905e-1c8a81f8b93b","resolution":{"observed_at":"2026-08-09T17:37:27.412542Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3978","last_updated":"2014-10-16T13:24:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2014-08-18T11:19:22Z","title":"Advanced Virgo: a 2nd generation interferometric gravitational wave detector","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.3978","snapshot_observed_at":"2026-08-09T17:37:27.416106Z","title":"Acernese et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.416106Z"},"links":{"cited_paper":"/paper/1408.3978","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:07b7d8b5a249fb9fd71bd36da773a24703a7a84cfeba14e76d8f8a935842e394","observation_id":"987a6036-e3ed-4c53-b0f8-48b0104382f8","resolution":{"observed_at":"2026-08-09T17:37:27.416106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03606","last_updated":"2023-10-23T13:37:50Z","snapshot_observed_at":"2026-08-08T16:18:10.684162Z","submitted_at":"2021-11-05T16:43:17Z","title":"GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.03606","snapshot_observed_at":"2026-08-09T17:37:27.420543Z","title":"Abbottet al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.420543Z"},"links":{"cited_paper":"/paper/2111.03606","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:6336ff746d98c281bece535882d9e8813ac796a409a3c6f0df05fe828045380e","observation_id":"4abc19d5-6714-4956-a083-b878cafbf745","resolution":{"observed_at":"2026-08-09T17:37:27.420543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.424689Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.424689Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:0c85c51add5c0cae0f3996950b445d14f6a21cf04f5e2db34b708a1b4af5993f","observation_id":"0622fc39-7b07-4994-948a-14a37f645a7e","resolution":{"observed_at":"2026-08-09T17:37:27.424689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.428567Z","title":"Olsen, T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.428567Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:1fdcc9247db60249082a91e6c652883ce502a1965e7a9351e0f7456b90a6b538","observation_id":"3da1b578-3340-4a26-aeaf-50122ed58a78","resolution":{"observed_at":"2026-08-09T17:37:27.428567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.433683Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.433683Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:d4417e864a7406a87605cf5b2ca4d10794b5c6f51cc73c2c1b85a4c2c8c2a073","observation_id":"6b9e44e6-dfc5-4ad2-b2ae-2dccc3e19b2f","resolution":{"observed_at":"2026-08-09T17:37:27.433683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.06061","last_updated":"2025-01-30T14:00:22Z","snapshot_observed_at":"2026-08-10T02:29:33.040003Z","submitted_at":"2023-11-10T13:50:45Z","title":"New binary black hole mergers in the LIGO-Virgo O3b data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.06061","snapshot_observed_at":"2026-08-09T17:37:27.437421Z","title":"New binary black hole mergers in the ligo- virgo o3b data,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.437421Z"},"links":{"cited_paper":"/paper/2311.06061","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:8aafc50786f562f5cdcee9cd9f7d558dea5c44c64768820796c1c6479b10417e","observation_id":"e4132bdb-1b40-426a-8795-15c9f7a49667","resolution":{"observed_at":"2026-08-09T17:37:27.437421Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.06631","last_updated":"2025-08-16T16:45:41Z","snapshot_observed_at":"2026-08-07T08:00:04.525533Z","submitted_at":"2023-12-11T18:50:10Z","title":"New black hole mergers in the LIGO-Virgo O3 data from a gravitational wave search including higher-order harmonics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.06631","snapshot_observed_at":"2026-08-09T17:37:27.441928Z","title":"New black hole mergers in the ligo-virgo o3 data from a gravitational wave search including higher-order har- monics,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.441928Z"},"links":{"cited_paper":"/paper/2312.06631","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:6bf0dbfecccf40d0e0c1c5fed53a3bfec15dc5ff47c2c52dcaed0649b0c64c5a","observation_id":"14d3ed89-64c4-4470-b8f7-1e8a3c0724f8","resolution":{"observed_at":"2026-08-09T17:37:27.441928Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.445989Z","title":"Vallisneri, J","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.445989Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:4e62b07fb9610b79810b5db410ab0781dcf6c464d8f3c9221aa47417f4236042","observation_id":"3ef6d6a0-ed50-42f8-bfce-efcf2ca85a5c","resolution":{"observed_at":"2026-08-09T17:37:27.445989Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.11716","last_updated":"2021-01-25T16:17:22Z","snapshot_observed_at":"2026-08-08T18:32:33.810582Z","submitted_at":"2019-12-25T21:15:52Z","title":"Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.11716","snapshot_observed_at":"2026-08-09T17:37:27.449618Z","title":"Abbott et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.449618Z"},"links":{"cited_paper":"/paper/1912.11716","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:e6f00e0d0b5178ee3beffa7e040166778e02fcb4dd87297842d66c0b679d1289","observation_id":"09dbd15e-ebf2-47b6-9794-ea0672e053a0","resolution":{"observed_at":"2026-08-09T17:37:27.449618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-09T17:37:27.453419Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.453419Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:9609a1688af107ac81e6e7eef15ee7f5d77c6916c20b21c68f90e2c0dab56eaf","observation_id":"f66d9bb5-ef4d-4f2f-b324-b68e01923b1e","resolution":{"observed_at":"2026-08-09T17:37:27.453419Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.01761","last_updated":"2020-04-07T09:39:44Z","snapshot_observed_at":"2026-08-10T13:59:44.754944Z","submitted_at":"2020-01-06T19:54:55Z","title":"GW190425: Observation of a Compact Binary Coalescence with Total Mass $\\sim 3.4 M_{\\odot}$","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.01761","snapshot_observed_at":"2026-08-09T17:37:27.457316Z","title":"Abbott et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.457316Z"},"links":{"cited_paper":"/paper/2001.01761","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:c17f4abca3b76f9e266c6b17e2d0cadf85e91265f4b8256094712f94788cef38","observation_id":"866af343-345d-41d9-a532-c1b11d81a481","resolution":{"observed_at":"2026-08-09T17:37:27.457316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.15163","last_updated":"2021-06-29T08:24:35Z","snapshot_observed_at":"2026-08-08T13:26:17.085092Z","submitted_at":"2021-06-29T08:24:35Z","title":"Observation of gravitational waves from two neutron star-black hole coalescences","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.15163","snapshot_observed_at":"2026-08-09T17:37:27.461312Z","title":"Abbottet al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.461312Z"},"links":{"cited_paper":"/paper/2106.15163","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:6578772fa186973e7a5e56b58c2aee89d5b6a681208a0941c4acf7d40459d569","observation_id":"b97d6718-692c-4214-8ff7-d90b9c8e62c4","resolution":{"observed_at":"2026-08-09T17:37:27.461312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06861","last_updated":"2025-11-17T15:05:31Z","snapshot_observed_at":"2026-08-02T22:41:06.793496Z","submitted_at":"2021-12-13T18:19:04Z","title":"Tests of General Relativity with GWTC-3","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06861","snapshot_observed_at":"2026-08-09T17:37:27.464883Z","title":"Abbottet al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.464883Z"},"links":{"cited_paper":"/paper/2112.06861","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:fdf3bdef0f6c6b37425e06fc53344bb8b3becd33d4f4800e9062266a7a812319","observation_id":"f0d75e1e-fdc0-4679-af38-7c4f3c5c30fd","resolution":{"observed_at":"2026-08-09T17:37:27.464883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03841","last_updated":"2018-10-23T15:08:45Z","snapshot_observed_at":"2026-07-06T04:45:55.047976Z","submitted_at":"2016-02-11T19:26:48Z","title":"Tests of general relativity with GW150914","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03841","snapshot_observed_at":"2026-08-09T17:37:27.468101Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.468101Z"},"links":{"cited_paper":"/paper/1602.03841","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:15ac5d630eb16057bbf1d61d1d0290282081ebbbec43d4b3a18ceb8730ad94af","observation_id":"122ee3f6-3b5e-4755-806a-da1a40b4c988","resolution":{"observed_at":"2026-08-09T17:37:27.468101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04467","last_updated":"2019-10-09T09:03:41Z","snapshot_observed_at":"2026-07-06T07:38:28.188454Z","submitted_at":"2019-03-11T17:43:43Z","title":"Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04467","snapshot_observed_at":"2026-08-09T17:37:27.471106Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.471106Z"},"links":{"cited_paper":"/paper/1903.04467","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:c5b8749a6923faa7d2c10019f8464ecfc5aa4930f4a753b4744cb2b9ad5bcc34","observation_id":"463f33bd-9c24-4914-bd3c-6fd00e40d170","resolution":{"observed_at":"2026-08-09T17:37:27.471106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.474292Z","title":"Abbott et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.474292Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:0d61d3b996c7c06e32af3040f2fa31e6e1e8b7ae510c4b46261c6ab36fea53f5","observation_id":"561043bd-91fb-4ab1-ae4e-ede7b48ef4cb","resolution":{"observed_at":"2026-08-09T17:37:27.474292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.02453","last_updated":"2016-09-14T08:32:59Z","snapshot_observed_at":"2026-07-06T04:45:24.152472Z","submitted_at":"2016-02-08T02:57:56Z","title":"Testing general relativity using golden black-hole binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.02453","snapshot_observed_at":"2026-08-09T17:37:27.477200Z","title":"Ghosh et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.477200Z"},"links":{"cited_paper":"/paper/1602.02453","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:c512ec01c9729795c5ee53f08990a5b59a008831407a76b87dfd487ec609492c","observation_id":"db65cd28-9b58-4b2b-bdc8-0a7c3cf68776","resolution":{"observed_at":"2026-08-09T17:37:27.477200Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.06784","last_updated":"2018-04-13T08:05:11Z","snapshot_observed_at":"2026-08-10T07:14:47.108225Z","submitted_at":"2017-04-22T11:45:25Z","title":"Testing general relativity using gravitational wave signals from the inspiral, merger and ringdown of binary black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.06784","snapshot_observed_at":"2026-08-09T17:37:27.480952Z","title":"Ghosh, N","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.480952Z"},"links":{"cited_paper":"/paper/1704.06784","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:4ca90982c1fe8a7516fb3db9f548889542d9a1e860214bfd60e756aaea1c6a5f","observation_id":"d4a9bb1f-917c-44cc-8896-6c2da350e732","resolution":{"observed_at":"2026-08-09T17:37:27.480952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.484683Z","title":"Blanchet and B","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.484683Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:49ad2247935c6d9d7ff8dc57a3cee1d37e72620fd7b14c4558c5ca702d1c1bbb","observation_id":"00df33ef-be93-46ab-8774-cf88d994985b","resolution":{"observed_at":"2026-08-09T17:37:27.484683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.488435Z","title":"Blanchet and B","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.488435Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:afeefeb61cfeb93e22c4b84836c057cdb71d865d826131753dd2071db9ce1392","observation_id":"b9730bc8-de35-496b-87a4-1218ae78e097","resolution":{"observed_at":"2026-08-09T17:37:27.488435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0604067","last_updated":"2006-06-29T09:11:02Z","snapshot_observed_at":"2026-07-07T03:22:24.227721Z","submitted_at":"2006-04-16T09:50:19Z","title":"Probing the non-linear structure of general relativity with black hole binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0604067","snapshot_observed_at":"2026-08-09T17:37:27.492311Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.492311Z"},"links":{"cited_paper":"/paper/gr-qc/0604067","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:21b80710c03e9d976eb8908c7433f75cd6aa9907ce6e5ae0c1ae72608d28db76","observation_id":"06bd71f9-7eea-400f-b0fa-db0790a15ee4","resolution":{"observed_at":"2026-08-09T17:37:27.492311Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0604018","last_updated":"2006-04-05T12:23:02Z","snapshot_observed_at":"2026-07-07T03:22:24.227721Z","submitted_at":"2006-04-05T12:23:02Z","title":"Testing post-Newtonian theory with gravitational wave observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0604018","snapshot_observed_at":"2026-08-09T17:37:27.496264Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.496264Z"},"links":{"cited_paper":"/paper/gr-qc/0604018","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:906d8c9a53550127c06914cf14e93a0badab4deb7a64c24cb13a5feffe5a7f35","observation_id":"aa9f8437-07c2-420f-9259-340a52159e2d","resolution":{"observed_at":"2026-08-09T17:37:27.496264Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.3328","last_updated":"2009-12-07T17:14:47Z","snapshot_observed_at":"2026-07-06T01:57:40.790524Z","submitted_at":"2009-09-17T22:16:20Z","title":"Fundamental Theoretical Bias in Gravitational Wave Astrophysics and the Parameterized Post-Einsteinian Framework","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.3328","snapshot_observed_at":"2026-08-09T17:37:27.500103Z","title":"Yunes and F","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.500103Z"},"links":{"cited_paper":"/paper/0909.3328","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:88141d7a60084d0af8b0a4fe486d7b1f5cb71312b8b32426984b6df6e097f902","observation_id":"d24397b7-2428-4853-9b54-2940d8db1b52","resolution":{"observed_at":"2026-08-09T17:37:27.500103Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1005.0304","last_updated":"2010-09-08T08:20:32Z","snapshot_observed_at":"2026-08-10T10:27:28.531073Z","submitted_at":"2010-05-03T14:12:10Z","title":"Parametrized tests of post-Newtonian theory using Advanced LIGO and Einstein Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.0304","snapshot_observed_at":"2026-08-09T17:37:27.504113Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.504113Z"},"links":{"cited_paper":"/paper/1005.0304","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:ebb8fc3c461bd1b8761374f2826a9d9cf44c9a0b6c05f89f75661c4050cb6246","observation_id":"0644e3d8-032d-43bb-aaa9-2b022b11a05c","resolution":{"observed_at":"2026-08-09T17:37:27.504113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.0530","last_updated":"2012-03-04T12:28:05Z","snapshot_observed_at":"2026-07-06T02:35:06.752411Z","submitted_at":"2011-10-03T22:06:11Z","title":"Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.0530","snapshot_observed_at":"2026-08-09T17:37:27.507935Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.507935Z"},"links":{"cited_paper":"/paper/1110.0530","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:579800ff5d341b63e63b868e9e7033fb9fbcd4b0b8b87d3e0acfd584dd7ec514","observation_id":"dbf78fbd-e7fa-419f-a4b0-41564b0d1c72","resolution":{"observed_at":"2026-08-09T17:37:27.507935Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.5274","last_updated":"2012-05-03T22:05:16Z","snapshot_observed_at":"2026-07-06T02:38:02.298612Z","submitted_at":"2011-11-22T18:29:40Z","title":"Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence: Further investigations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.5274","snapshot_observed_at":"2026-08-09T17:37:27.512374Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.512374Z"},"links":{"cited_paper":"/paper/1111.5274","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:83b74cca500081d37e8cf0e1a14da65613b7a65050f658a159c1c4e1ac6a3165","observation_id":"b64d26f4-3c6a-43a4-b612-19fa73370ad5","resolution":{"observed_at":"2026-08-09T17:37:27.512374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.00364","last_updated":"2019-07-29T15:54:28Z","snapshot_observed_at":"2026-08-07T23:27:34.485522Z","submitted_at":"2018-11-01T13:23:52Z","title":"Tests of General Relativity with GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.00364","snapshot_observed_at":"2026-08-09T17:37:27.516643Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.516643Z"},"links":{"cited_paper":"/paper/1811.00364","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:1015ee11206059dccca279e410eb7c09d109e06a978fa7f289edea59dc741c36","observation_id":"1ed70e90-0dbd-4f19-af0a-25d563c78eae","resolution":{"observed_at":"2026-08-09T17:37:27.516643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.521055Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.521055Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:1dcf31bcc34060763af5c92b636606ade49fdfa05182d1b9e77759c6fdde34ee","observation_id":"b9bed366-f2b0-403c-8b22-556c4ba13af8","resolution":{"observed_at":"2026-08-09T17:37:27.521055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.524873Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.524873Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:bae18e354fbcf1e6940490267aee0d7424af78a27002335b009586335e45472e","observation_id":"2bccf573-48eb-428d-a0ed-b77e0468ea3b","resolution":{"observed_at":"2026-08-09T17:37:27.524873Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.528010Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.528010Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:6aa566555bf386a00e17eeb358ec6f59dce65f0693d04e8b3072fcb3cada1ae7","observation_id":"cac40099-0a09-4459-b11c-fe6a56b27491","resolution":{"observed_at":"2026-08-09T17:37:27.528010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.531225Z","title":"Oguri, Monthly Notices of the Royal Astronomical Society 480, 3842 (2018)","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.531225Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:7efac699a79e29f0546119082ef640340b4ac9c471de859944f9ddf6e9b1e574","observation_id":"2c753180-a7dd-4dce-8039-42efefd0d905","resolution":{"observed_at":"2026-08-09T17:37:27.531225Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.534542Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.534542Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:355cd80248367e355cc7d3d98fd523a21151e105d4632b3930c4087dc5c5a333","observation_id":"01d36070-8789-40d0-be57-431cff59b806","resolution":{"observed_at":"2026-08-09T17:37:27.534542Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.537957Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.537957Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:b6f70a6e3de50ebd5d42239849e3b20123b4c15879dfe5f2d953494d237b4452","observation_id":"0c599f68-61fb-4fd8-af2e-590e4bb44bea","resolution":{"observed_at":"2026-08-09T17:37:27.537957Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.05140","last_updated":"2019-02-13T21:47:30Z","snapshot_observed_at":"2026-08-10T23:32:05.263985Z","submitted_at":"2019-02-13T21:47:30Z","title":"Discovery of Strongly-lensed Gravitational Waves - Implications for the LSST Observing Strategy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.05140","snapshot_observed_at":"2026-08-09T17:37:27.541422Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.541422Z"},"links":{"cited_paper":"/paper/1902.05140","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:76781d44ddb2f88d57f4681e58c8b31811e1423065039a3ee92167b4c4caba9e","observation_id":"4a91653d-b0a9-4429-bdea-b1dd4e7945f7","resolution":{"observed_at":"2026-08-09T17:37:27.541422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.545955Z","title":"Robertson, G","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.545955Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:c062af9d740325fb15b49c91a2bf1b16429b4edceee9aae03a18174cacd1c3a1","observation_id":"b32cbb0d-fff8-46c3-8756-9ff0326ded49","resolution":{"observed_at":"2026-08-09T17:37:27.545955Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.549935Z","title":"Ryczanowski, G","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.549935Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:bdf3bce964d04cfa1b8ff70890d11df1088b2ae43c50cd5ee19ded3fb296bcc1","observation_id":"9453ddeb-6db7-4140-9f45-d78c8ea78b83","resolution":{"observed_at":"2026-08-09T17:37:27.549935Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.554380Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.554380Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:85503d6e54a62d85a37aef3acfad05569929cfbb4bd1211e40c893d94ed6cf4f","observation_id":"bbc1f65b-3e8e-4c9e-9fe5-fcffe2d0cac5","resolution":{"observed_at":"2026-08-09T17:37:27.554380Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.04724","last_updated":"2017-02-15T19:00:01Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2017-02-15T19:00:01Z","title":"On the waveforms of gravitationally lensed gravitational waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.04724","snapshot_observed_at":"2026-08-09T17:37:27.557871Z","title":"Dai and T","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.557871Z"},"links":{"cited_paper":"/paper/1702.04724","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:698497fe935b9b8d43c76eea097a6f5616bb661d817bf4ab1ec8775e382e8b99","observation_id":"91546371-5dd7-4170-8da7-18a9beab75ff","resolution":{"observed_at":"2026-08-09T17:37:27.557871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.561584Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.561584Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:7a2db4e22521b2dc1541846d6b5258ad76965fc26be65477a6de6795c559ab5b","observation_id":"f6a2a843-0a7c-446d-95f2-c41310c6c710","resolution":{"observed_at":"2026-08-09T17:37:27.561584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.564936Z","title":"Deguchi and W","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.564936Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:5b0cfc65064d7db710f2c68fb51cce6a250019cccdb41908dc1f60c8fcaad585","observation_id":"b5c993cd-9822-4236-9a65-a2a337b8a1e7","resolution":{"observed_at":"2026-08-09T17:37:27.564936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.568449Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.568449Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:0e08285cc9dad1b8a543c294377d5ecf609411a8b9c18f55f1e5708d1528a528","observation_id":"afba9a61-7c3b-4758-907a-cea54ab5a2a2","resolution":{"observed_at":"2026-08-09T17:37:27.568449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.571743Z","title":"Takahashi and T","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.571743Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:e76892927a841fcead0902f0eca78530c7d6226be5497b5c70ac406852ea9591","observation_id":"1903a3e2-c5d8-4079-a828-a51945ce2b8b","resolution":{"observed_at":"2026-08-09T17:37:27.571743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.575164Z","title":"Cao, L.-F","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.575164Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:e1d49fbd2afe39b2efe81a99bc90bb5fa5cd190b882252ee21344459a68710a4","observation_id":"e134e5ab-23b5-4a66-93c6-59f778f51a0d","resolution":{"observed_at":"2026-08-09T17:37:27.575164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.578843Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.578843Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:4ab39919a8df595d653377148f2b0539b39aadc7493c86705ef94755bb7fae1a","observation_id":"c3854b08-98e8-4963-a287-7f4994f387ae","resolution":{"observed_at":"2026-08-09T17:37:27.578843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.582340Z","title":"Christian, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.582340Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:5a67c977dfb281e1ddf6ce969df2a2357f880285a20deac1830456c0578b0a84","observation_id":"a85b4b81-63b0-4d81-bae4-61c91012852a","resolution":{"observed_at":"2026-08-09T17:37:27.582340Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.586030Z","title":"Dai, S.-S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.586030Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:2b80404bd6427061abde6f5f87230efaf68a3776447f14d39b98f5312440a19f","observation_id":"e30a790a-da11-4a38-b7bb-3fc5f7f66ef9","resolution":{"observed_at":"2026-08-09T17:37:27.586030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.589207Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.589207Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:8181531a46c210d47c841f8d42a02d9ffb1f4cd26f765c65db00e96fa63989b8","observation_id":"3152b900-2a89-48ef-8a9f-631e88651799","resolution":{"observed_at":"2026-08-09T17:37:27.589207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.962346Z","title":"Baker and M","venue":null,"work_id":"7c78331d-83b1-49c4-85ee-d90f74587d51","year":2017},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.592825Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:8e6bc32b6c9e7fe40cf52edd6eb29409c005d3bf0cf9e98cef4737e2edae903b","observation_id":"d37bdf46-6789-4ae9-9bbe-a46455dc3db1","resolution":{"observed_at":"2026-08-09T17:37:28.965839Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.952129Z","title":null,"venue":null,"work_id":"58113bac-5722-48d1-b7d4-5f78b8e55908","year":2017},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.596085Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:88219e88612453e453ebe4884145f3267271edd8fee9bbb9334da938b32bdb24","observation_id":"e9ea48d3-d432-494a-ada4-d60ae9fdf35f","resolution":{"observed_at":"2026-08-09T17:37:28.955743Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.941388Z","title":null,"venue":null,"work_id":"6845994d-9a9e-47a8-83e9-846af6838eef","year":2017},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.599025Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:9c8093e51b46bef34b1727418c9cf92c9d39f412e9f4250d2d152e8e42e81194","observation_id":"568fb0c3-cd40-4e55-a2ea-756e8818f27a","resolution":{"observed_at":"2026-08-09T17:37:28.944907Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.931159Z","title":"Goyal, K","venue":null,"work_id":"d05adbe7-a2ff-43fe-a8de-e72b1d91b8c6","year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.602079Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:f299ee6fde589a2e03930ee3a70a292716054536539fed1b733ffeaa2645435c","observation_id":"aacc0c19-0e29-4a3a-a963-d136d824b40b","resolution":{"observed_at":"2026-08-09T17:37:28.934868Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.920476Z","title":null,"venue":null,"work_id":"ea6bda63-e297-4d7e-aef9-1a0466c310e5","year":2020},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.606178Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:47cc187b41cd34de6b696fb0c88de6436e26ecf57cb8b28827f65be5c53d2a44","observation_id":"8146ba69-be3b-4186-813b-3c1060690999","resolution":{"observed_at":"2026-08-09T17:37:28.924013Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.910881Z","title":"Sereno, P","venue":null,"work_id":"0e409750-67d1-49e6-9b7c-65809eadb03e","year":2011},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.609677Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:dd2d3eb714ca639ec1a3ea0b445c5a11ab7108771e0c1877c492b76fe0e2199d","observation_id":"4753dbe4-d84c-436f-b05e-f3425934727b","resolution":{"observed_at":"2026-08-09T17:37:28.913930Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.901575Z","title":"Liao, X.-L","venue":null,"work_id":"d10791cb-57bd-49d9-8a6d-9ee4e6b07811","year":2017},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.613279Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:261f5efc454da18a8d157cae64cff202f1413066ecba29c1cf0b48f612569348","observation_id":"a698f0fb-e68e-4c5c-99aa-8dd53c92d8ab","resolution":{"observed_at":"2026-08-09T17:37:28.904678Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.892095Z","title":null,"venue":null,"work_id":"c173d599-5cb1-4fc7-829b-f733c1531a39","year":2019},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.616762Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:4c0d8311ab8a6ec8ff862de45693de0cfb955568a52966613d902c97b8cce040","observation_id":"709e7463-bb6c-4733-88d4-c37c01781d50","resolution":{"observed_at":"2026-08-09T17:37:28.895393Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.882100Z","title":null,"venue":null,"work_id":"78599363-5e04-49e1-a526-d251d6dc7e10","year":2019},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.620404Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:36ffd0c35ea9821d20ec7ce8529644950aa3a96abe2ef022aa5d08dd792f4d69","observation_id":"1d74cddc-063f-494a-9ec6-a0f3189f2cc8","resolution":{"observed_at":"2026-08-09T17:37:28.885471Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.872116Z","title":null,"venue":null,"work_id":"1c210edb-20dd-4414-a377-6138f44902db","year":2020},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.624971Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:41e55941608e4a9760959d9e055fdacbfdb315c649e18c664954c3a9899958b6","observation_id":"18dca436-416c-44a3-89b4-ef397ed93421","resolution":{"observed_at":"2026-08-09T17:37:28.875587Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.861503Z","title":null,"venue":null,"work_id":"828b08f8-7aef-4263-82db-a0294250cde3","year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.628490Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:a87b54e091c8933fe1f330ea12988890014bda47477bce54a050abffd48461b5","observation_id":"94200c09-4b7b-41d8-a25c-e62cad03711c","resolution":{"observed_at":"2026-08-09T17:37:28.864892Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.05290","last_updated":"2024-08-09T18:21:26Z","snapshot_observed_at":"2026-07-06T18:59:00.983278Z","submitted_at":"2024-08-09T18:21:26Z","title":"Probing the nature of dark matter using strongly lensed gravitational waves from binary black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.05290","snapshot_observed_at":"2026-08-09T17:37:27.632119Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.632119Z"},"links":{"cited_paper":"/paper/2408.05290","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:67543408fedfafb23461919f1092c42ed8ed6231492e2b6c59e7693da14acb62","observation_id":"697aea88-3728-4693-a37c-109fadaa515a","resolution":{"observed_at":"2026-08-09T17:37:27.632119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.02916","last_updated":"2023-02-06T16:40:51Z","snapshot_observed_at":"2026-08-06T18:55:18.880385Z","submitted_at":"2023-02-06T16:40:51Z","title":"Gear-up for the Action Replay: Leveraging Lensing for Enhanced Gravitational-Wave Early-Warning","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.02916","snapshot_observed_at":"2026-08-09T17:37:27.636077Z","title":"Magare, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.636077Z"},"links":{"cited_paper":"/paper/2302.02916","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:68d2323ba9717a90d004a14e33c7b94f7fa0988d4bcc1f1c240818fd18afa9eb","observation_id":"68784723-dd61-4ecc-aa93-04a747eea16f","resolution":{"observed_at":"2026-08-09T17:37:27.636077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.06456","last_updated":"2022-02-23T04:17:52Z","snapshot_observed_at":"2026-07-06T11:47:27.474428Z","submitted_at":"2021-09-14T05:52:55Z","title":"Constraints on compact dark matter from gravitational wave microlensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.06456","snapshot_observed_at":"2026-08-09T17:37:27.639845Z","title":"Basak, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.639845Z"},"links":{"cited_paper":"/paper/2109.06456","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:45b214e72c261c416f03afaabe3d6e028a14d467c189804950482a56bce2fb9a","observation_id":"2c7bd431-4deb-4576-b41e-c45ee5d96220","resolution":{"observed_at":"2026-08-09T17:37:27.639845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.15878","last_updated":"2024-05-24T18:42:23Z","snapshot_observed_at":"2026-08-06T19:36:07.530495Z","submitted_at":"2024-05-24T18:42:23Z","title":"Constraints on compact dark matter from the non-observation of gravitational-wave strong lensing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.15878","snapshot_observed_at":"2026-08-09T17:37:27.643350Z","title":"Barsode, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.643350Z"},"links":{"cited_paper":"/paper/2405.15878","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:08c18cf8cee1bacb3e23be4155a73bab2b61256a6b49dc84ee9b7915caf55cd5","observation_id":"3bf50213-05d8-4336-aa66-7d541fc68d54","resolution":{"observed_at":"2026-08-09T17:37:27.643350Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.17805","last_updated":"2024-11-19T08:04:25Z","snapshot_observed_at":"2026-08-05T23:09:39.008359Z","submitted_at":"2024-05-28T04:08:01Z","title":"Strong-lensing cosmography using third-generation gravitational-wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.17805","snapshot_observed_at":"2026-08-09T17:37:27.646984Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.646984Z"},"links":{"cited_paper":"/paper/2405.17805","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:d01eab506879194091eef358e42c917333a64e1d97c4f8281c83de8726c0cdf0","observation_id":"e158a4ab-faad-4668-9cee-2453f61c6b3a","resolution":{"observed_at":"2026-08-09T17:37:27.646984Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.06553","last_updated":"2025-01-09T17:01:40Z","snapshot_observed_at":"2026-08-06T16:51:43.422003Z","submitted_at":"2024-01-12T12:58:53Z","title":"Probing charge of compact objects with gravitational microlensing of gravitational waves","version":2},"cited_work":{"arxiv_id":"2401.06553","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.06553","snapshot_observed_at":"2026-08-09T17:37:28.247970Z","title":"Probing charge of compact objects with gravitational microlensing of gravitational waves","venue":"gr-qc","work_id":"cee81bcf-acfe-41c3-8017-8f0aae9b7da9","year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.650388Z"},"links":{"cited_paper":"/paper/2401.06553","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:1c9557874c8cd1699d15d10315e95b889da6765151f8eab4b1d0180b519376bb","observation_id":"9ecb8b32-65f7-499c-af24-e64cac6b1ff5","resolution":{"observed_at":"2026-08-09T17:37:28.252067Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.00022","last_updated":"2023-01-04T06:04:23Z","snapshot_observed_at":"2026-07-06T13:05:16.090823Z","submitted_at":"2022-04-29T18:01:11Z","title":"Prospects for the observation of continuous gravitational waves from spinning neutron stars lensed by the galactic supermassive black hole","version":3},"cited_work":{"arxiv_id":"2205.00022","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.00022","snapshot_observed_at":"2026-08-09T17:37:28.232721Z","title":"Prospects for the observation of continuous gravitational waves from spinning neutron stars lensed by the galactic supermassive black hole","venue":"gr-qc","work_id":"e3c4c72c-527c-446b-9adf-55d63d3f1188","year":2022},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.653886Z"},"links":{"cited_paper":"/paper/2205.00022","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:198bbfafaf227cb58ca0da891d117ad8d55c04a3bd8ae111e755be2333f4f08c","observation_id":"75d9c559-6fef-40a5-9cf5-66cd22410f22","resolution":{"observed_at":"2026-08-09T17:37:28.236995Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.02674","last_updated":"2019-01-29T12:07:22Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2019-01-09T11:00:38Z","title":"Search for gravitational lensing signatures in LIGO-Virgo binary black hole events","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.02674","snapshot_observed_at":"2026-08-09T17:37:27.657030Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.657030Z"},"links":{"cited_paper":"/paper/1901.02674","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:f49e3725ca8efb7947fe1cc6e5168fa211d60fb35e53bb54bdeee54b9b940129","observation_id":"070f32cc-f27e-46f3-b67d-029ee33ddc80","resolution":{"observed_at":"2026-08-09T17:37:27.657030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.06384","last_updated":"2021-11-30T17:55:25Z","snapshot_observed_at":"2026-08-08T11:55:42.486548Z","submitted_at":"2021-05-13T16:12:18Z","title":"Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.06384","snapshot_observed_at":"2026-08-09T17:37:27.660097Z","title":"Abbott et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.660097Z"},"links":{"cited_paper":"/paper/2105.06384","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:382fae17adce64affdac9ffb0dcd41fb98824a67cbd8739ab1be6c77b672d3e0","observation_id":"4a52eb8b-7861-404c-bac6-5e242b693a0c","resolution":{"observed_at":"2026-08-09T17:37:27.660097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.08393","last_updated":"2023-04-17T15:59:33Z","snapshot_observed_at":"2026-08-07T21:19:49.102106Z","submitted_at":"2023-04-17T15:59:33Z","title":"Search for gravitational-lensing signatures in the full third observing run of the LIGO-Virgo network","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.08393","snapshot_observed_at":"2026-08-09T17:37:27.664780Z","title":"Abbottet al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.664780Z"},"links":{"cited_paper":"/paper/2304.08393","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:c1a208f2386cfcac54035a48d8efb6329f21470b3c56fc0f21f926461b87563b","observation_id":"5d6166c2-76d4-417f-b14a-54861ae5d2fd","resolution":{"observed_at":"2026-08-09T17:37:27.664780Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.850511Z","title":null,"venue":null,"work_id":"25dc600c-69ea-4afc-b72d-4ff546bf5b0a","year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.668489Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:f4380f0735fda798f6f98947fed31170d1d32e48b39eda53d9ca7e0f6685d64d","observation_id":"aac40247-6c54-4dcc-a5c1-c6a94dee1777","resolution":{"observed_at":"2026-08-09T17:37:28.853997Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.14390","last_updated":"2021-07-30T01:56:49Z","snapshot_observed_at":"2026-08-09T05:01:24.532153Z","submitted_at":"2021-05-29T23:53:09Z","title":"Please repeat: Strong lensing of gravitational waves as a probe of compact binary and galaxy populations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.14390","snapshot_observed_at":"2026-08-09T17:37:27.672064Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.672064Z"},"links":{"cited_paper":"/paper/2105.14390","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:e067d0e26eb19bad7b188fc9d9d25d12928faf807e5a02895c090558e1f0d065","observation_id":"d26aa0d1-3adc-4b77-af0a-3260bbf6aa4e","resolution":{"observed_at":"2026-08-09T17:37:27.672064Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.07062","last_updated":"2018-07-18T17:56:20Z","snapshot_observed_at":"2026-08-10T01:13:32.754380Z","submitted_at":"2018-07-18T17:56:20Z","title":"Identifying strongly lensed gravitational wave signals from binary black hole mergers","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.07062","snapshot_observed_at":"2026-08-09T17:37:27.676748Z","title":"Haris, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.676748Z"},"links":{"cited_paper":"/paper/1807.07062","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:39fe17fdeb851079121c4430b99059db152582874891031e49c77838e92000f5","observation_id":"a98e0b24-2f55-4de7-ae98-7c828fcd5185","resolution":{"observed_at":"2026-08-09T17:37:27.676748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.12466","last_updated":"2021-06-23T15:27:28Z","snapshot_observed_at":"2026-08-06T06:30:47.353185Z","submitted_at":"2021-06-23T15:27:28Z","title":"Rapid Identification of Strongly Lensed Gravitational-Wave Events with Machine Learning","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.12466","snapshot_observed_at":"2026-08-09T17:37:27.685023Z","title":"Goyal, H","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.685023Z"},"links":{"cited_paper":"/paper/2106.12466","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:3ab2d7a14697b2a77305ec2de6561e40df8b402fddbf7562b8a335c6fbdfe5c6","observation_id":"ab6d9921-1cff-4f46-9f57-171fd43b2ecd","resolution":{"observed_at":"2026-08-09T17:37:27.685023Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.02994","last_updated":"2024-03-05T14:20:24Z","snapshot_observed_at":"2026-08-11T01:29:31.236364Z","submitted_at":"2024-03-05T14:20:24Z","title":"SLICK: Strong Lensing Identification of Candidates Kindred in gravitational wave data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.02994","snapshot_observed_at":"2026-08-09T17:37:27.688688Z","title":"Magare, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.688688Z"},"links":{"cited_paper":"/paper/2403.02994","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:d850aabd5142e54663fff28fcf588de70d2ea4b45e2e9b179657a4babaa26495","observation_id":"72a94552-e035-41ab-bfaf-70991890a48c","resolution":{"observed_at":"2026-08-09T17:37:27.688688Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.04397","last_updated":"2023-06-07T12:57:32Z","snapshot_observed_at":"2026-07-06T15:39:41.431581Z","submitted_at":"2023-06-07T12:57:32Z","title":"A rapid method for preliminary identification of subthreshold strongly lensed counterparts to superthreshold gravitational-wave events","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.04397","snapshot_observed_at":"2026-08-09T17:37:27.692455Z","title":"Goyal, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.692455Z"},"links":{"cited_paper":"/paper/2306.04397","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:e7c5ba04a5a12ea6881457b9354742e70b8d1043b3e3aa974ae7c28e92ed4903","observation_id":"0cf5318e-bcd5-4916-a336-93245c2fd90b","resolution":{"observed_at":"2026-08-09T17:37:27.692455Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.06616","last_updated":"2023-10-23T22:30:11Z","snapshot_observed_at":"2026-07-06T16:05:35.645037Z","submitted_at":"2023-08-12T17:13:14Z","title":"Identifying strongly lensed gravitational waves through their phase consistency","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.06616","snapshot_observed_at":"2026-08-09T17:37:27.696342Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.696342Z"},"links":{"cited_paper":"/paper/2308.06616","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:102ff330439c32d1ab4ac5a50b540a3666ca1c7728caf7a66ab727dbef908053","observation_id":"ec1d1558-ea1c-41a1-bc05-bf10ff118d87","resolution":{"observed_at":"2026-08-09T17:37:27.696342Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03982","last_updated":"2024-08-17T11:21:10Z","snapshot_observed_at":"2026-08-06T05:18:27.997341Z","submitted_at":"2024-03-06T19:00:10Z","title":"GLANCE -- Gravitational Lensing Authenticator using Non-Modelled Cross-Correlation Exploration of Gravitational Wave Signals","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03982","snapshot_observed_at":"2026-08-09T17:37:27.700320Z","title":"Chakraborty and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.700320Z"},"links":{"cited_paper":"/paper/2403.03982","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:69d228242fd30f7da517bf7d1e8393592d1c2bd73727b5bd1a1b2ec8d04343dc","observation_id":"4a58b067-f291-4a3c-98b1-680f36099c27","resolution":{"observed_at":"2026-08-09T17:37:27.700320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.839571Z","title":null,"venue":null,"work_id":"097dd5fe-ccc2-447a-8ec5-4adb6d145b17","year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.704009Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:cba01fc46d7662dfcc80a0f10e674664150d21a8e6cf10fea97c3402a138b9f9","observation_id":"a4804eb9-9495-4553-877e-413994ecc107","resolution":{"observed_at":"2026-08-09T17:37:28.843449Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06444","last_updated":"2022-03-15T10:20:07Z","snapshot_observed_at":"2026-08-06T12:04:00.914013Z","submitted_at":"2022-03-12T14:32:18Z","title":"GOLUM: A fast and precise methodology to search for, and analyze, strongly lensed gravitational-wave events","version":2},"cited_work":{"arxiv_id":"2203.06444","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.06444","snapshot_observed_at":"2026-08-09T17:37:28.111316Z","title":"GOLUM: A fast and precise methodology to search for, and analyze, strongly lensed gravitational-wave events","venue":"gr-qc","work_id":"8838b0f1-8476-4c6e-b19b-12ba39e959c4","year":2022},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.707128Z"},"links":{"cited_paper":"/paper/2203.06444","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:d5b1ea266fc094e28eff709c8105e894a3b0eb368d26fc64e4e8bd3de685579c","observation_id":"903c5482-b450-4f33-bde7-732031f3c7b5","resolution":{"observed_at":"2026-08-09T17:37:28.115746Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.12148","last_updated":"2023-04-24T14:58:10Z","snapshot_observed_at":"2026-07-06T15:19:21.255953Z","submitted_at":"2023-04-24T14:58:10Z","title":"The Return of GOLUM: Improving Distributed Joint Parameter Estimation for Strongly-Lensed Gravitational Waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.12148","snapshot_observed_at":"2026-08-09T17:37:27.710692Z","title":"Janquart, K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.710692Z"},"links":{"cited_paper":"/paper/2304.12148","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:3cd765414a084f1840f3b785cce57e6ee01f1f1acdbe8d1f1a771b4d484a156a","observation_id":"5a0f5fc0-bb49-4f67-8cc5-0157e1b52215","resolution":{"observed_at":"2026-08-09T17:37:27.710692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.828426Z","title":null,"venue":null,"work_id":"dddf32f1-a502-449e-8e49-b2f528c8d413","year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.714240Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:9c333f00679218b40f09a2913c0de96845776ea86e9d5dba33fc9b1984b4487f","observation_id":"bfae77ca-e96b-472b-b8e8-c3eab63fb36b","resolution":{"observed_at":"2026-08-09T17:37:28.832352Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.01278","last_updated":"2024-12-02T08:46:44Z","snapshot_observed_at":"2026-07-06T20:00:00.800207Z","submitted_at":"2024-12-02T08:46:44Z","title":"Fast and efficient Bayesian method to search for strongly lensed gravitational waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.01278","snapshot_observed_at":"2026-08-09T17:37:27.717789Z","title":"Barsode, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.717789Z"},"links":{"cited_paper":"/paper/2412.01278","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:1830b7ba5a2f154b1e03deac4c4b4118189f5fbbeae4ccb26638f0d8cb9f3e31","observation_id":"f9271885-38df-4dca-b078-b9e12d926d44","resolution":{"observed_at":"2026-08-09T17:37:27.717789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.12901","last_updated":"2020-06-23T11:12:04Z","snapshot_observed_at":"2026-08-10T17:49:11.430525Z","submitted_at":"2020-06-23T11:12:04Z","title":"An optimal $\\chi^2$ discriminator against modelled noise-transients in interferometric data in searches for binary black-hole mergers","version":1},"cited_work":{"arxiv_id":"2006.12901","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.12901","snapshot_observed_at":"2026-08-09T17:37:28.080033Z","title":"An optimal $\\chi^2$ discriminator against modelled noise-transients in interferometric data in searches for binary black-hole mergers","venue":"gr-qc","work_id":"21553ec0-594c-4aa1-91e2-36a17103098d","year":2020},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.721304Z"},"links":{"cited_paper":"/paper/2006.12901","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:d8d78609c6f8407f48eb3bddba28dff2b7a8c76965704d7d240529f323b0e119","observation_id":"d4733de6-f305-4964-97b9-f4fcd803bb31","resolution":{"observed_at":"2026-08-09T17:37:28.084744Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.817404Z","title":null,"venue":null,"work_id":"0bffa966-c67e-48b1-a12d-f3b06ff19081","year":2011},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.725783Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:7a9bb2998d44c8f44b78a38cd518d06c07432db98a37085367ee3c5cdd7f5176","observation_id":"258782aa-5fac-471c-8682-a3815df31aab","resolution":{"observed_at":"2026-08-09T17:37:28.821042Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.729599Z","title":"Allen, Phys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.729599Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:b7a341d0a246ba0d8d628e022eee59afa2c812618d2638a8530a6aa18833b9ab","observation_id":"55cfe33d-4160-4207-b0e9-cd24198032d3","resolution":{"observed_at":"2026-08-09T17:37:27.729599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.806398Z","title":"Babak, R","venue":null,"work_id":"6d690836-323e-4097-bd9c-3c1a295b3938","year":2006},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.733117Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:f9b880dea4abe849750d5d48e3315a56ad8dd620c8ba467ef4911548b4fbd729","observation_id":"da3fa38b-3e92-4a53-a4df-d989d86463c4","resolution":{"observed_at":"2026-08-09T17:37:28.809926Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.795686Z","title":"gwastro/pycbc: v2.0.4 release of pycbc,","venue":null,"work_id":"283ce6d2-7329-4c1b-929b-acee93a66a8b","year":2022},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.736593Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:4251add1763abe0f9ff35238df30d72fc7c84425c31125b2efaaab30202db3df","observation_id":"71da20f8-83ff-49f7-9a3b-ad39b418c97d","resolution":{"observed_at":"2026-08-09T17:37:28.799243Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.785682Z","title":null,"venue":null,"work_id":"db4fd423-5a66-4ec8-8e75-2401b1a14a38","year":2016},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.740129Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:af84a339281d4bde7fe6ed071c2b68bf6e24d607fc94e08bd7ca44b1c1183ca5","observation_id":"86611f97-405b-4126-a00c-7998ca7a7b19","resolution":{"observed_at":"2026-08-09T17:37:28.789132Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.774005Z","title":null,"venue":null,"work_id":"786e3c97-ecc1-4721-8acd-332c257d7193","year":2016},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.744239Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:dc41b8dd57d837aa852213e7a8b2835809be7e39ab2a9a4eda0d8a5884440c8f","observation_id":"8d660220-f795-45ab-b72b-376fdbc9bc3e","resolution":{"observed_at":"2026-08-09T17:37:28.778301Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.06020","last_updated":"2023-06-14T01:03:20Z","snapshot_observed_at":"2026-08-07T01:21:06.727493Z","submitted_at":"2019-04-12T03:07:42Z","title":"Targeted Sub-threshold Search for Strongly-lensed Gravitational-wave Events","version":7},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.06020","snapshot_observed_at":"2026-08-09T17:37:27.747752Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.747752Z"},"links":{"cited_paper":"/paper/1904.06020","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:5ee421cde3dd45d1cf42659d6870b5e06e74cf4ead67497204713ffd23b0c4d1","observation_id":"554c4d0d-7ac5-4f13-acc6-096428b160c8","resolution":{"observed_at":"2026-08-09T17:37:27.747752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:27.751987Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.751987Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:e2d18d3eadaf3aa5822fc1e8f9b960cf7e58cf6902fa9fdc4ac18762a8d71738","observation_id":"a75469e8-c315-4722-8bf3-fa97020c8c6d","resolution":{"observed_at":"2026-08-09T17:37:27.751987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.762770Z","title":null,"venue":null,"work_id":"6ee04704-5345-4193-8be5-a1de5f0d2aee","year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.755550Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:78072088ec2dbf1d8d9d4c1864853cb6a260f12a3f5a1243ac65809e9fb0fa93","observation_id":"f7cf9ded-518b-4622-888a-004e3915d302","resolution":{"observed_at":"2026-08-09T17:37:28.766047Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-09T17:37:28.752499Z","title":"Janquart, E","venue":null,"work_id":"76b851b2-ef0b-4d53-b00f-a8709614450d","year":2021},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.759529Z"},"links":{"citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:a78b76306b54a5275aa3a1ed1eb03595fa275f8b5e48a5ad0d2f44c8d7a4672a","observation_id":"d31ae81d-19f9-410f-b288-1f2d9ba4bc23","resolution":{"observed_at":"2026-08-09T17:37:28.755766Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2202.06334","last_updated":"2023-08-07T08:20:59Z","snapshot_observed_at":"2026-08-10T01:03:04.399574Z","submitted_at":"2022-02-13T14:51:51Z","title":"Detection and parameter estimation challenges of Type-II lensed binary black hole signals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.06334","snapshot_observed_at":"2026-08-09T17:37:27.763140Z","title":"Vijaykumar, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.763140Z"},"links":{"cited_paper":"/paper/2202.06334","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:4a6ab55fdfc6b2d15eb46f6bc23fe71a60ae403e9167a8fc2cc9c515d7da81d0","observation_id":"2cd44dd1-c430-4a46-ab70-7ff0d622b76c","resolution":{"observed_at":"2026-08-09T17:37:27.763140Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.15148","last_updated":"2025-07-24T01:24:23Z","snapshot_observed_at":"2026-08-09T11:25:24.338997Z","submitted_at":"2024-12-19T18:27:47Z","title":"Phase consistency test to identify type II strongly lensed gravitational wave signals using a single event","version":3},"cited_work":{"arxiv_id":"2412.15148","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.15148","snapshot_observed_at":"2026-08-09T17:37:27.865138Z","title":"Phase consistency test to identify type II strongly lensed gravitational wave signals using a single event","venue":"gr-qc","work_id":"5e6f6c07-f284-4eec-a215-3812cac02564","year":2024},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.766966Z"},"links":{"cited_paper":"/paper/2412.15148","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:2d097071f722a7b33f80dc2d5f8ac7dd0bb686c4c076cb807cee35a90b088e14","observation_id":"ee85182d-cd14-4956-b95b-c44920a73436","resolution":{"observed_at":"2026-08-09T17:37:27.871337Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2201.04619","last_updated":"2023-05-29T20:52:11Z","snapshot_observed_at":"2026-08-05T17:23:21.853187Z","submitted_at":"2022-01-12T18:56:01Z","title":"Lensing or luck? False alarm probabilities for gravitational lensing of gravitational waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.04619","snapshot_observed_at":"2026-08-09T17:37:27.770363Z","title":"Çalışkan, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences","version":2},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-08-09T17:37:27.770363Z"},"links":{"cited_paper":"/paper/2201.04619","citing_paper":"/paper/2502.00844"},"observation_digest":"sha256:2e2a18806c0ddeff7315453abc6e15f4a40eb349c8325b6f4699f1b0fe2dae94","observation_id":"8d237ad5-7506-4719-9389-8ed8512e79f1","resolution":{"observed_at":"2026-08-09T17:37:27.770363Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2502.00844","last_updated":"2026-07-22T19:09:30Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-10T22:06:57.226209Z","submitted_at":"2025-02-02T16:32:58Z","title":"A $\\chi^2$ statistic for the identification of strongly lensed gravitational waves from compact binary coalescences"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":87,"verified_exact":5,"verified_fuzzy":7},"total_outbound_references":107},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 100 of 107 outbound references and 0 inbound Pith citation observations for arXiv:2502.00844."}