{"as_of":"2026-08-18T04:49:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f03db8d6d4f9d006b3587e093fd8835dbce7f8ab1ce4941f0597417fef4e4b01","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":"2026-08-17T06:30:58.91139+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":"2026-08-07T14:46:39.002363Z","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":"2026-08-05T18:35:42.690858Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1904.10847","last_updated":"2019-05-22T16:44:32Z","snapshot_observed_at":"2026-08-16T08:52:56.095714Z","submitted_at":"2019-04-24T14:37:41Z","title":"Quasinormal modes of regular black holes with non linear-Electrodynamical sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.10847","snapshot_observed_at":"2026-08-07T14:46:39.002363Z","title":"Quasinormal modes of regular black holes with non linear-Electrodynamical sources,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.17947","last_updated":"2025-05-23T14:24:05Z","snapshot_observed_at":"2026-08-15T14:44:37.755732Z","submitted_at":"2025-05-23T14:24:05Z","title":"Charged black holes in Kalb-Ramond gravity: Weak Deflection Angle, Shadow cast, Quasinormal Modes and Neutrino annihilation","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-07T14:46:39.002363Z"},"links":{"cited_paper":"/paper/1904.10847","citing_paper":"/paper/2505.17947"},"observation_digest":"sha256:6baf4525ad7690ebeb6ad2becbac1a99485a828cba06bc139b025d67f96fc9ab","observation_id":"a08c747f-b0fc-4bb9-9033-01fef4993d51","resolution":{"observed_at":"2026-08-07T14:46:39.002363Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.10847","last_updated":"2019-05-22T16:44:32Z","snapshot_observed_at":"2026-08-16T08:52:56.095714Z","submitted_at":"2019-04-24T14:37:41Z","title":"Quasinormal modes of regular black holes with non linear-Electrodynamical sources","version":2},"cited_work":{"arxiv_id":"1904.10847","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.10847","snapshot_observed_at":"2026-08-05T18:35:42.690858Z","title":"Quasinormal modes of regular black holes with non linear-Electrodynamical sources","venue":"gr-qc","work_id":"ad869389-6b0c-4951-9ebe-2abec03f0c41","year":2019},"citing_paper":{"arxiv_id":"2508.14489","last_updated":"2025-08-20T07:27:01Z","snapshot_observed_at":"2026-08-15T00:23:13.916013Z","submitted_at":"2025-08-20T07:27:01Z","title":"Energy Extraction and Evolution of Regular Black Holes: The Case of Bardeen Spacetime","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-05T18:35:36.367347Z"},"links":{"cited_paper":"/paper/1904.10847","citing_paper":"/paper/2508.14489"},"observation_digest":"sha256:30590891523377f1dfd88617236bbe34cf93ff84a3d91aa08026a52321047671","observation_id":"6fec7b29-26e5-45f4-93c3-ce3b6bed3906","resolution":{"observed_at":"2026-08-05T18:35:42.809188Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.10847","last_updated":"2019-05-22T16:44:32Z","snapshot_observed_at":"2026-08-16T08:52:56.095714Z","submitted_at":"2019-04-24T14:37:41Z","title":"Quasinormal modes of regular black holes with non linear-Electrodynamical sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.10847","snapshot_observed_at":"2026-07-12T01:38:05.217536Z","title":"Panotopoulos and Á","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-15T23:09:32.785590Z","submitted_at":"2026-07-03T18:43:45Z","title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-12T01:38:05.217536Z"},"links":{"cited_paper":"/paper/1904.10847","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:dea403ee5c79f6c190e9eb74647c5a332faf8e1fd3f236e75d25ce6292a69ee4","observation_id":"9b8dd0c4-9993-429f-98d5-3b5ed4f2fedc","resolution":{"observed_at":"2026-07-12T01:38:05.217536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.10847","last_updated":"2019-05-22T16:44:32Z","snapshot_observed_at":"2026-08-16T08:52:56.095714Z","submitted_at":"2019-04-24T14:37:41Z","title":"Quasinormal modes of regular black holes with non linear-Electrodynamical sources","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.10847","snapshot_observed_at":"2026-08-02T08:53:13.229963Z","title":"Panotopoulos and Á","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-15T23:09:32.785590Z","submitted_at":"2026-07-03T18:43:45Z","title":"Gravitational perturbations of a regular T-duality inspired black hole: Quasinormal modes, excitation factors, and time-domain evolution","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-02T08:53:13.229963Z"},"links":{"cited_paper":"/paper/1904.10847","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:26cc391424502b07140f104dab6803f64fd8fb55d591ec7e73c5e6e4179665b9","observation_id":"02f389ad-14b5-4f58-b195-a5e910059b46","resolution":{"observed_at":"2026-08-02T08:53:13.229963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1904.10847/citation-record","integrity":"/paper/1904.10847/integrity","json":"/paper/1904.10847/citation-record.json","paper":"/paper/1904.10847"},"outbound":[],"paper":{"arxiv_id":"1904.10847","last_updated":"2019-05-22T16:44:32Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T08:52:56.095714Z","submitted_at":"2019-04-24T14:37:41Z","title":"Quasinormal modes of regular black holes with non linear-Electrodynamical sources"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1904.10847."}