{"as_of":"2026-08-07T08:23:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c53b8e10b797e335fd08d5e8f7eab3d0f48b1f558847f38b0e16d7bde9b1a8a9","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T09:43:29.778080Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-05-22T01:50:54.590669Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown","version":2},"cited_work":{"arxiv_id":"1711.00926","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.00926","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"On choosing the start time of binary black hole ringdown","venue":"gr-qc","work_id":"58667dbd-8784-47dc-b06e-e520491fc498","year":2017},"citing_paper":{"arxiv_id":"2010.14529","last_updated":"2025-09-10T17:43:53Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-10-27T18:01:34Z","title":"Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog","version":3},"reference_index":138,"source":"pdf_text","source_observed_at":"2026-05-15T03:47:43.850102Z"},"links":{"cited_paper":"/paper/1711.00926","citing_paper":"/paper/2010.14529"},"observation_digest":"sha256:54eaee2ce85c640a0d4ad14416af121bc296057f0ecca3457dae7b6cd4f6cef4","observation_id":"a9c551fc-51b0-46e9-9041-0c3f4b4e7a0c","resolution":{"observed_at":"2026-05-15T03:47:46.945952Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown","version":2},"cited_work":{"arxiv_id":"1711.00926","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.00926","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"On choosing the start time of binary black hole ringdown","venue":"gr-qc","work_id":"58667dbd-8784-47dc-b06e-e520491fc498","year":2017},"citing_paper":{"arxiv_id":"2506.01035","last_updated":"2026-05-20T00:27:25Z","snapshot_observed_at":"2026-07-06T21:34:34.091508Z","submitted_at":"2025-06-01T14:33:43Z","title":"Finite Curvature Construction of Regular Black Holes and Quasinormal Mode Analysis","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-19T12:07:22.369254Z"},"links":{"cited_paper":"/paper/1711.00926","citing_paper":"/paper/2506.01035"},"observation_digest":"sha256:d0c6fc9903edba761f4921f40f44064ab52ecdfbca2703b0ef6840f9976f6c6c","observation_id":"965c9173-6d70-48a5-9917-dd7a1e830f4f","resolution":{"observed_at":"2026-05-19T12:12:17.020137Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown","version":2},"cited_work":{"arxiv_id":"1711.00926","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.00926","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"On choosing the start time of binary black hole ringdown","venue":"gr-qc","work_id":"58667dbd-8784-47dc-b06e-e520491fc498","year":2017},"citing_paper":{"arxiv_id":"2506.01035","last_updated":"2026-05-20T00:27:25Z","snapshot_observed_at":"2026-07-06T21:34:34.091508Z","submitted_at":"2025-06-01T14:33:43Z","title":"Finite Curvature Construction of Regular Black Holes and Quasinormal Mode Analysis","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-22T01:48:23.292871Z"},"links":{"cited_paper":"/paper/1711.00926","citing_paper":"/paper/2506.01035"},"observation_digest":"sha256:cd590caa7d109020c202a501c594893ba106d0f18f315f09fd753968bc94aa28","observation_id":"34c5d51a-4730-4cb9-ae0a-bade9a4a4981","resolution":{"observed_at":"2026-05-22T01:50:54.593147Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown","version":2},"cited_work":{"arxiv_id":"1711.00926","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.00926","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"On choosing the start time of binary black hole ringdown","venue":"gr-qc","work_id":"58667dbd-8784-47dc-b06e-e520491fc498","year":2017},"citing_paper":{"arxiv_id":"2507.08219","last_updated":"2025-11-10T18:47:56Z","snapshot_observed_at":"2026-07-06T21:55:27.120410Z","submitted_at":"2025-07-10T23:52:46Z","title":"GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\\odot}$","version":3},"reference_index":110,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.00926","citing_paper":"/paper/2507.08219"},"observation_digest":"sha256:5d22fbec7fbf2a078d5eca84280bbaecf4d1ff382305146e940841a527d08fbe","observation_id":"87ef37ac-6dab-4933-83a2-0680cb1a1945","resolution":{"observed_at":"2026-05-16T03:16:34.113827Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00926","snapshot_observed_at":"2026-08-04T09:43:29.778080Z","title":"Bhagwatet al., PRD97, 104065 (2018), arXiv:1711.00926 [gr-qc]","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2510.13954","last_updated":"2026-06-24T11:08:04Z","snapshot_observed_at":"2026-08-05T21:41:34.850791Z","submitted_at":"2025-10-15T18:00:03Z","title":"Quasinormal mode content of binary black hole ringdowns","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-04T09:43:29.778080Z"},"links":{"cited_paper":"/paper/1711.00926","citing_paper":"/paper/2510.13954"},"observation_digest":"sha256:21714b8a84b789b6f74990075196479d5bcbd0e3831b010fd172ecaa3ea8e388","observation_id":"687c5e6b-c2a3-40fb-85c2-507a5fadf06e","resolution":{"observed_at":"2026-08-04T09:43:29.778080Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown","version":2},"cited_work":{"arxiv_id":"1711.00926","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.00926","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"On choosing the start time of binary black hole ringdown","venue":"gr-qc","work_id":"58667dbd-8784-47dc-b06e-e520491fc498","year":2017},"citing_paper":{"arxiv_id":"2601.23019","last_updated":"2026-05-05T14:01:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-01-30T14:27:25Z","title":"Toward claiming a detection of gravitational memory","version":2},"reference_index":139,"source":"pdf_text","source_observed_at":"2026-05-16T09:18:23.702726Z"},"links":{"cited_paper":"/paper/1711.00926","citing_paper":"/paper/2601.23019"},"observation_digest":"sha256:82edd1181dea59fd7d2619bbfdb91cbc6e63000b0828ed19cd80702ce7800d7d","observation_id":"93fe3457-9f49-47ec-addb-57ef1cee9410","resolution":{"observed_at":"2026-05-16T09:20:47.933452Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown","version":2},"cited_work":{"arxiv_id":"1711.00926","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.00926","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"On choosing the start time of binary black hole ringdown","venue":"gr-qc","work_id":"58667dbd-8784-47dc-b06e-e520491fc498","year":2017},"citing_paper":{"arxiv_id":"2604.15431","last_updated":"2026-04-16T18:00:02Z","snapshot_observed_at":"2026-08-02T05:54:54.327009Z","submitted_at":"2026-04-16T18:00:02Z","title":"Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms","version":1},"reference_index":197,"source":"pdf_text","source_observed_at":"2026-05-10T10:16:15.923894Z"},"links":{"cited_paper":"/paper/1711.00926","citing_paper":"/paper/2604.15431"},"observation_digest":"sha256:342453e40f32091e48df607e6bdc39a683140c9ba712cc6343ed159b93bd7172","observation_id":"276daece-ace1-44cb-836c-09575a3c316e","resolution":{"observed_at":"2026-05-10T10:19:21.057357Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown","version":2},"cited_work":{"arxiv_id":"1711.00926","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.00926","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"On choosing the start time of binary black hole ringdown","venue":"gr-qc","work_id":"58667dbd-8784-47dc-b06e-e520491fc498","year":2017},"citing_paper":{"arxiv_id":"2605.18249","last_updated":"2026-05-18T11:50:45Z","snapshot_observed_at":"2026-07-06T23:29:09.538843Z","submitted_at":"2026-05-18T11:50:45Z","title":"Quasinormal modes of a rotating loop quantum black hole","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-20T09:22:46.533112Z"},"links":{"cited_paper":"/paper/1711.00926","citing_paper":"/paper/2605.18249"},"observation_digest":"sha256:698f8650722fde8047ab41ae58bcdb94df2e232eb93a9bb73ddd971c4b814df0","observation_id":"6c1e5101-a890-4f16-b281-0dc1c078d4ee","resolution":{"observed_at":"2026-05-20T09:23:10.385395Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00926","snapshot_observed_at":"2026-08-01T09:07:05.037809Z","title":"On choosing the start time of binary black hole ringdowns,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.27343","last_updated":"2026-07-29T18:01:42Z","snapshot_observed_at":"2026-08-06T04:38:09.721746Z","submitted_at":"2026-07-29T18:01:42Z","title":"Nonlinear Dynamics near the Threshold of Gravitational Collapse","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-01T09:07:05.037809Z"},"links":{"cited_paper":"/paper/1711.00926","citing_paper":"/paper/2607.27343"},"observation_digest":"sha256:e3597f2cff1297516f7b5b263b70ad612a0cb9def8046438e6167a13fa7bd0c0","observation_id":"d3a23c8c-574c-4845-a6d5-308cb39164e2","resolution":{"observed_at":"2026-08-01T09:07:05.037809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1711.00926/citation-record","integrity":"/paper/1711.00926/integrity","json":"/paper/1711.00926/citation-record.json","paper":"/paper/1711.00926"},"outbound":[],"paper":{"arxiv_id":"1711.00926","last_updated":"2017-11-06T23:08:16Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T06:07:28.704181Z","submitted_at":"2017-11-02T20:39:43Z","title":"On choosing the start time of binary black hole ringdown"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1711.00926."}