{"as_of":"2026-08-08T07:40:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:558cdeadbf7243edb66d3561431a95db09017a4d3ef16684e98e66196d9a2bef","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":11,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":11,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":11,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":11,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T13:46:34.112181Z","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":"2026-05-23T06:12:38.861240Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":"2211.04263","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"7df5ff45-030f-46e1-b434-4145decd5a73","year":2023},"citing_paper":{"arxiv_id":"2501.07029","last_updated":"2025-01-20T07:28:31Z","snapshot_observed_at":"2026-07-06T20:20:05.443672Z","submitted_at":"2025-01-13T03:00:02Z","title":"Shadow of the Scalar Hairy Black Hole with Inverted Higgs Potential","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-23T06:09:14.669705Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2501.07029"},"observation_digest":"sha256:1b8eaec4dc8553ee2ba6592d1fc51bd0c9f61f280b12b1647d388d20360fd321","observation_id":"cc676630-3041-4ab9-bb87-42aea69810a1","resolution":{"observed_at":"2026-05-23T06:12:38.863734Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-08-07T13:46:34.112181Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.21314","last_updated":"2025-05-27T15:12:56Z","snapshot_observed_at":"2026-08-07T20:32:33.662872Z","submitted_at":"2025-05-27T15:12:56Z","title":"Testing Extended Theories of Gravity via Black Hole Photon Rings","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-07T13:46:34.112181Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2505.21314"},"observation_digest":"sha256:e07348a93219062e69813dd66f999663d3cb3163caf7df63f910a83edbf75250","observation_id":"fd29b46c-6cad-49c7-a6a6-3909c2485de9","resolution":{"observed_at":"2026-08-07T13:46:34.112181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-08-07T11:26:26.581440Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.02653","last_updated":"2025-06-03T09:06:31Z","snapshot_observed_at":"2026-08-07T15:39:27.466751Z","submitted_at":"2025-06-03T09:06:31Z","title":"Thermodynamics and Shadows of Kerr black holes endowed with a global monopole charge","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-07T11:26:26.581440Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2506.02653"},"observation_digest":"sha256:a2cd7479716b610ecca11a8ff8c56e7185ba169c629bfb409a66c8b4e30b88bf","observation_id":"a98ca486-0f4e-4451-9702-5c81bda40764","resolution":{"observed_at":"2026-08-07T11:26:26.581440Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-08-06T14:09:33.285642Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-06T14:09:32.264748Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.285642Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:ca57d1581ee019a065d21707ed8afb51e825a541454126957a5e715b29ded672","observation_id":"d6ab7bda-4590-4ac5-acc7-99d553c8f8f9","resolution":{"observed_at":"2026-08-06T14:09:33.285642Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-08-04T10:39:00.141982Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.09956","last_updated":"2026-05-24T09:34:07Z","snapshot_observed_at":"2026-08-07T13:23:38.196297Z","submitted_at":"2025-10-11T02:03:25Z","title":"Image of a quantum-corrected black hole without Cauchy horizons illuminated by a static thin accretion disk","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-04T10:39:00.141982Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2510.09956"},"observation_digest":"sha256:0a5a687c6bf0f44c4bb4575974353a55ae017c1e05b831f5b897fe0803a8fe34","observation_id":"f0f3659c-c372-47be-981c-056215328a4f","resolution":{"observed_at":"2026-08-04T10:39:00.141982Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":"2211.04263","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"7df5ff45-030f-46e1-b434-4145decd5a73","year":2023},"citing_paper":{"arxiv_id":"2510.27320","last_updated":"2026-04-06T06:53:03Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-31T09:47:10Z","title":"The quasinormal modes of the rotating quantum corrected black holes","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-18T03:07:46.828770Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2510.27320"},"observation_digest":"sha256:f61208d3a93171f2230c143b3181e6311fce55d34472040bb8eadb0f2a765419","observation_id":"e745814d-87e6-47be-8b0d-8f757bff4e40","resolution":{"observed_at":"2026-05-18T03:10:49.257700Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":"2211.04263","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"7df5ff45-030f-46e1-b434-4145decd5a73","year":2023},"citing_paper":{"arxiv_id":"2604.04441","last_updated":"2026-04-06T05:39:36Z","snapshot_observed_at":"2026-07-06T22:53:24.585766Z","submitted_at":"2026-04-06T05:39:36Z","title":"Gravity/thermodynamics correspondence via black hole shadows","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-10T20:27:30.544350Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2604.04441"},"observation_digest":"sha256:2039a2e54c4f853fa11a6c92e868e6cdc127e5c7ce858ea96fce149f2bf5231a","observation_id":"01f1f468-13a9-4037-b1a0-9cb52b65f64e","resolution":{"observed_at":"2026-05-10T21:55:51.411107Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":"2211.04263","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"7df5ff45-030f-46e1-b434-4145decd5a73","year":2023},"citing_paper":{"arxiv_id":"2604.11866","last_updated":"2026-04-13T17:07:50Z","snapshot_observed_at":"2026-08-02T23:16:52.582741Z","submitted_at":"2026-04-13T17:07:50Z","title":"Equatorial periodic orbits and gravitational wave signatures in Euler-Heisenberg black holes surrounded by perfect fluid dark matter","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-10T15:39:57.103611Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2604.11866"},"observation_digest":"sha256:756dd0c5cbfde7e563948815369f1ca58cb59b102dd977b71e72dc8b5ead9b8e","observation_id":"494f6f6f-098d-477d-a2c4-20f8c11dda50","resolution":{"observed_at":"2026-05-11T10:06:02.081164Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":"2211.04263","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"7df5ff45-030f-46e1-b434-4145decd5a73","year":2023},"citing_paper":{"arxiv_id":"2604.13494","last_updated":"2026-04-15T05:26:59Z","snapshot_observed_at":"2026-08-02T11:34:31.411572Z","submitted_at":"2026-04-15T05:26:59Z","title":"Probing Kalb-Ramond gravity with charged rotating black holes: constraints from EHT observations","version":1},"reference_index":114,"source":"pdf_text","source_observed_at":"2026-05-10T13:14:45.286559Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2604.13494"},"observation_digest":"sha256:b655bdd9ebd519263ef2950b7d40259ec9a9ff582b9e3f22268bd342dc72b281","observation_id":"06cf18c2-2768-4e49-942e-ebeff9be6044","resolution":{"observed_at":"2026-05-10T13:15:26.449727Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":"2211.04263","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"7df5ff45-030f-46e1-b434-4145decd5a73","year":2023},"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":18,"source":"pdf_text","source_observed_at":"2026-05-20T09:22:46.533112Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2605.18249"},"observation_digest":"sha256:fc616f5d54b7c4b008bc0d37924dcdb4131068eeb51694b7a35fc99f482a499d","observation_id":"95ecfe85-4d5c-4db8-bf0c-ba37e1680e5d","resolution":{"observed_at":"2026-05-20T09:23:10.449619Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-08-01T01:43:18.235362Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.25738","last_updated":"2026-07-28T14:03:36Z","snapshot_observed_at":"2026-08-07T17:07:23.134741Z","submitted_at":"2026-07-28T14:03:36Z","title":"Echoes and quasinormal modes for static loop quantum black bounces","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-01T01:43:18.235362Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2607.25738"},"observation_digest":"sha256:72ef250e48a2d34daf995465acaca9088884d00ea0a9877289f2c4be6b652132","observation_id":"a9125e03-d9a5-4cf4-bb74-149411121c01","resolution":{"observed_at":"2026-08-01T01:43:18.235362Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2211.04263/citation-record","integrity":"/paper/2211.04263/integrity","json":"/paper/2211.04263/citation-record.json","paper":"/paper/2211.04263"},"outbound":[],"paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T14:15:44.460161Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2211.04263."}