{"as_of":"2026-08-14T01:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:97f7b0fc0445a8ca20a26af86f70419ac2063edb346596aeb43e7fe1bc1ac2b0","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T15:58:04.872893Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-10T09:13:30.688991Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2406.03846","last_updated":"2024-06-06T08:24:14Z","snapshot_observed_at":"2026-08-13T19:25:43.319993Z","submitted_at":"2024-06-06T08:24:14Z","title":"Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.03846","snapshot_observed_at":"2026-08-12T15:58:04.872893Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.13897","last_updated":"2024-11-21T07:17:49Z","snapshot_observed_at":"2026-08-13T15:33:55.989016Z","submitted_at":"2024-11-21T07:17:49Z","title":"Observing the eye of the storm I: testing regular black holes with LVK and EHT observations","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-12T15:58:04.872893Z"},"links":{"cited_paper":"/paper/2406.03846","citing_paper":"/paper/2411.13897"},"observation_digest":"sha256:214cae02449b38a6ec77a3d8de4f595ed7ce6a0806dbbd13261c6937b569e160","observation_id":"b1186a98-1e2b-4c57-98bc-30294fdd9259","resolution":{"observed_at":"2026-08-12T15:58:04.872893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03846","last_updated":"2024-06-06T08:24:14Z","snapshot_observed_at":"2026-08-13T19:25:43.319993Z","submitted_at":"2024-06-06T08:24:14Z","title":"Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.03846","snapshot_observed_at":"2026-08-11T18:22:23.738457Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08205","last_updated":"2025-04-17T11:28:01Z","snapshot_observed_at":"2026-08-12T05:14:38.577635Z","submitted_at":"2024-12-11T08:53:12Z","title":"Quasi-normal modes of slowly-rotating Johannsen black holes","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T18:22:23.738457Z"},"links":{"cited_paper":"/paper/2406.03846","citing_paper":"/paper/2412.08205"},"observation_digest":"sha256:e5f5d31109590573e016c977697051b998492a8c196dbad9f16b62e5870734c6","observation_id":"6d55890f-5116-4a7b-a7a0-6cf8ecbcfe62","resolution":{"observed_at":"2026-08-11T18:22:23.738457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03846","last_updated":"2024-06-06T08:24:14Z","snapshot_observed_at":"2026-08-13T19:25:43.319993Z","submitted_at":"2024-06-06T08:24:14Z","title":"Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.03846","snapshot_observed_at":"2026-08-06T15:40:39.541524Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.15270","last_updated":"2025-08-26T12:22:04Z","snapshot_observed_at":"2026-08-06T18:43:34.174277Z","submitted_at":"2025-07-21T06:17:50Z","title":"Stellar-Mass Black Holes","version":2},"reference_index":133,"source":"pdf_text","source_observed_at":"2026-08-06T15:40:39.541524Z"},"links":{"cited_paper":"/paper/2406.03846","citing_paper":"/paper/2507.15270"},"observation_digest":"sha256:aa832863ef18ecdc4aa109fdd07d1e97376d392fda8c3fccd0ce706ba5e1070b","observation_id":"e1a17690-95af-4b41-b986-e97b77d11b63","resolution":{"observed_at":"2026-08-06T15:40:39.541524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03846","last_updated":"2024-06-06T08:24:14Z","snapshot_observed_at":"2026-08-13T19:25:43.319993Z","submitted_at":"2024-06-06T08:24:14Z","title":"Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order","version":1},"cited_work":{"arxiv_id":"2406.03846","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.03846","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"1d24b672-6d32-4ede-8cb0-715ac4ee1d94","year":2024},"citing_paper":{"arxiv_id":"2604.15965","last_updated":"2026-07-06T07:16:38Z","snapshot_observed_at":"2026-08-11T14:22:51.225025Z","submitted_at":"2026-04-17T11:29:10Z","title":"Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-10T08:05:34.078542Z"},"links":{"cited_paper":"/paper/2406.03846","citing_paper":"/paper/2604.15965"},"observation_digest":"sha256:1ab1126f7d0e99bb1af6f10c31f11951232c290604d7f4c2506da2759019b7b3","observation_id":"d0faff33-898c-40f6-bbbe-f0f48a436786","resolution":{"observed_at":"2026-05-10T09:13:30.691046Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2406.03846/citation-record","integrity":"/paper/2406.03846/integrity","json":"/paper/2406.03846/citation-record.json","paper":"/paper/2406.03846"},"outbound":[],"paper":{"arxiv_id":"2406.03846","last_updated":"2024-06-06T08:24:14Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-13T19:25:43.319993Z","submitted_at":"2024-06-06T08:24:14Z","title":"Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2406.03846."}