{"as_of":"2026-08-22T20:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b50f8959bef82906eeace8ea0f62e56b840216ade995ebd4d36e03f1c16c9b53","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T22:18:53.870074Z","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":"2026-05-16T12:02:50.796008Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2312.00557","last_updated":"2024-02-12T09:24:43Z","snapshot_observed_at":"2026-08-16T14:38:29.099806Z","submitted_at":"2023-12-01T13:12:41Z","title":"The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.00557","snapshot_observed_at":"2026-08-11T22:18:53.870074Z","title":"Mummery, The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events, Mon","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.03655","last_updated":"2025-04-07T07:25:40Z","snapshot_observed_at":"2026-08-13T07:04:52.428367Z","submitted_at":"2024-12-04T19:00:01Z","title":"Stepping Up Superradiance Constraints on Axions","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T22:18:53.870074Z"},"links":{"cited_paper":"/paper/2312.00557","citing_paper":"/paper/2412.03655"},"observation_digest":"sha256:e39333363412a093ccfa4cd1306310d56536eb1680dbbe6735d7725593a5feac","observation_id":"666ee1af-1144-4f56-a392-39a692580455","resolution":{"observed_at":"2026-08-11T22:18:53.870074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.00557","last_updated":"2024-02-12T09:24:43Z","snapshot_observed_at":"2026-08-16T14:38:29.099806Z","submitted_at":"2023-12-01T13:12:41Z","title":"The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.00557","snapshot_observed_at":"2026-08-07T11:54:00.604813Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.01437","last_updated":"2025-06-02T08:51:54Z","snapshot_observed_at":"2026-08-22T02:34:38.151929Z","submitted_at":"2025-06-02T08:51:54Z","title":"Black hole supercolliders","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T11:54:00.604813Z"},"links":{"cited_paper":"/paper/2312.00557","citing_paper":"/paper/2506.01437"},"observation_digest":"sha256:5c0c79d21b579950a7409b34e58253d96948f3863e77a5f3c22523d4d93b6bc9","observation_id":"0fea6ef7-f1d4-4896-9df5-1f01956dea2a","resolution":{"observed_at":"2026-08-07T11:54:00.604813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.00557","last_updated":"2024-02-12T09:24:43Z","snapshot_observed_at":"2026-08-16T14:38:29.099806Z","submitted_at":"2023-12-01T13:12:41Z","title":"The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.00557","snapshot_observed_at":"2026-08-06T11:21:10.574113Z","title":"Mummery, Mon","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.23161","last_updated":"2025-07-30T23:47:53Z","snapshot_observed_at":"2026-08-20T11:02:03.960516Z","submitted_at":"2025-07-30T23:47:53Z","title":"Mass Determination of Supermassive Black Holes Governing Evolution of Radio Emitters","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T11:21:10.574113Z"},"links":{"cited_paper":"/paper/2312.00557","citing_paper":"/paper/2507.23161"},"observation_digest":"sha256:ab242c1a922aef805522479d83d4cac474f78ad5aa403b5dfdcf4dd4c9c1391a","observation_id":"f08d4c86-a18e-4e17-b75a-ce86633e24f9","resolution":{"observed_at":"2026-08-06T11:21:10.574113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.00557","last_updated":"2024-02-12T09:24:43Z","snapshot_observed_at":"2026-08-16T14:38:29.099806Z","submitted_at":"2023-12-01T13:12:41Z","title":"The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events","version":2},"cited_work":{"arxiv_id":"2312.00557","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2312.00557","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events","venue":null,"work_id":"1328a95a-3bf7-458f-8113-bd9cf784125a","year":2023},"citing_paper":{"arxiv_id":"2601.16082","last_updated":"2026-05-05T14:49:12Z","snapshot_observed_at":"2026-07-06T22:42:43.581560Z","submitted_at":"2026-01-22T16:25:13Z","title":"Roche limit and stellar disruption in the Simpson--Visser spacetime","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-05-16T12:01:27.699618Z"},"links":{"cited_paper":"/paper/2312.00557","citing_paper":"/paper/2601.16082"},"observation_digest":"sha256:5ef7b1d62060b85e2049812655b93d423c59ee82a799f430c6ec8e64056cf5fd","observation_id":"c856db07-4390-450b-a456-10593ec5e6b2","resolution":{"observed_at":"2026-05-16T12:02:50.798189Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.00557","last_updated":"2024-02-12T09:24:43Z","snapshot_observed_at":"2026-08-16T14:38:29.099806Z","submitted_at":"2023-12-01T13:12:41Z","title":"The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.00557","snapshot_observed_at":"2026-08-05T23:39:12.965753Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.03205","last_updated":"2026-08-04T06:47:15Z","snapshot_observed_at":"2026-08-14T02:28:25.228277Z","submitted_at":"2026-08-04T06:47:15Z","title":"One year of broadband radio monitoring of the enigmatic transient GRB 250702B reveals the evolution of the relativistic jet","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-05T23:39:12.965753Z"},"links":{"cited_paper":"/paper/2312.00557","citing_paper":"/paper/2608.03205"},"observation_digest":"sha256:814279f29fedfd88474f77a8d04b9927ad964ce12bc689ba84bef37866c7e7e6","observation_id":"0a793ae8-f22e-4031-91c7-7ee56aee2c68","resolution":{"observed_at":"2026-08-05T23:39:12.965753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2312.00557/citation-record","integrity":"/paper/2312.00557/integrity","json":"/paper/2312.00557/citation-record.json","paper":"/paper/2312.00557"},"outbound":[],"paper":{"arxiv_id":"2312.00557","last_updated":"2024-02-12T09:24:43Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T14:38:29.099806Z","submitted_at":"2023-12-01T13:12:41Z","title":"The maximum mass of a black hole which can tidally disrupt a star: measuring black hole spins with tidal disruption events"},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2312.00557."}