{"as_of":"2026-08-10T23:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:510dbc578e4c1f8cefdb0071b4784a889186535d18105daf67e9f986e786d7ec","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":"2026-08-10T06:31:04.303077+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":"2026-08-09T18:51:41.427184Z","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":"2026-05-16T12:02:50.978105Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2203.04965","last_updated":"2022-04-25T22:30:40Z","snapshot_observed_at":"2026-07-06T12:46:08.838773Z","submitted_at":"2022-03-09T17:21:15Z","title":"Bardeen-Kiselev black hole with cosmological constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.04965","snapshot_observed_at":"2026-08-09T18:51:41.427184Z","title":"Bardeen-Kiselev black hole with a cosmological constant,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.00502","last_updated":"2025-02-10T14:04:04Z","snapshot_observed_at":"2026-08-10T17:55:55.055645Z","submitted_at":"2025-02-01T17:49:07Z","title":"Spherically symmetric and static black bounces with multiple horizons, throats, and anti-throats in four dimensions","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-09T18:51:41.427184Z"},"links":{"cited_paper":"/paper/2203.04965","citing_paper":"/paper/2502.00502"},"observation_digest":"sha256:76fe06024c7aa5f151a76e8955a8d538835937f3e2615e7c2d8416068080e76c","observation_id":"ce418a93-d0ca-4ebe-8816-de0f61d96eba","resolution":{"observed_at":"2026-08-09T18:51:41.427184Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04965","last_updated":"2022-04-25T22:30:40Z","snapshot_observed_at":"2026-07-06T12:46:08.838773Z","submitted_at":"2022-03-09T17:21:15Z","title":"Bardeen-Kiselev black hole with cosmological constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.04965","snapshot_observed_at":"2026-08-06T14:09:33.362896Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-09T21:51:28.473483Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.362896Z"},"links":{"cited_paper":"/paper/2203.04965","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:66beb241746ecbc90675b2c62ca73a681a1b5fb2805a465896b882b64c3b2a34","observation_id":"e529aa7d-74b9-4111-b9a4-eae855b72964","resolution":{"observed_at":"2026-08-06T14:09:33.362896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04965","last_updated":"2022-04-25T22:30:40Z","snapshot_observed_at":"2026-07-06T12:46:08.838773Z","submitted_at":"2022-03-09T17:21:15Z","title":"Bardeen-Kiselev black hole with cosmological constant","version":2},"cited_work":{"arxiv_id":"2203.04965","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2203.04965","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bardeen-Kiselev black hole with a cos- mological constant","venue":null,"work_id":"9348ab34-58fb-4c76-b7fe-7fb9bbff23be","year":2022},"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":35,"source":"pdf_text","source_observed_at":"2026-05-16T12:01:27.699618Z"},"links":{"cited_paper":"/paper/2203.04965","citing_paper":"/paper/2601.16082"},"observation_digest":"sha256:73dd4d59aaeef63c58d9ff9d9c51851e9e7f99b0314401c1e432871dd4577201","observation_id":"31c0764d-6edf-4b75-9240-66feba67d2e8","resolution":{"observed_at":"2026-05-16T12:02:50.980369Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04965","last_updated":"2022-04-25T22:30:40Z","snapshot_observed_at":"2026-07-06T12:46:08.838773Z","submitted_at":"2022-03-09T17:21:15Z","title":"Bardeen-Kiselev black hole with cosmological constant","version":2},"cited_work":{"arxiv_id":"2203.04965","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2203.04965","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bardeen-Kiselev black hole with a cos- mological constant","venue":null,"work_id":"9348ab34-58fb-4c76-b7fe-7fb9bbff23be","year":2022},"citing_paper":{"arxiv_id":"2603.23556","last_updated":"2026-07-17T20:08:50Z","snapshot_observed_at":"2026-08-10T10:15:32.150173Z","submitted_at":"2026-03-23T18:55:24Z","title":"On regular black string spacetimes in nonlinear electrodynamics","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-15T00:26:19.378889Z"},"links":{"cited_paper":"/paper/2203.04965","citing_paper":"/paper/2603.23556"},"observation_digest":"sha256:ede996c27fda0644c190177a453cb2f15e50af87205a1c468fe231860a5b210b","observation_id":"ea991a55-eac3-4f2a-af9d-a88feec12125","resolution":{"observed_at":"2026-05-15T00:28:23.308973Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04965","last_updated":"2022-04-25T22:30:40Z","snapshot_observed_at":"2026-07-06T12:46:08.838773Z","submitted_at":"2022-03-09T17:21:15Z","title":"Bardeen-Kiselev black hole with cosmological constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.04965","snapshot_observed_at":"2026-08-02T17:53:11.090410Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.23556","last_updated":"2026-07-17T20:08:50Z","snapshot_observed_at":"2026-08-10T10:15:32.150173Z","submitted_at":"2026-03-23T18:55:24Z","title":"On regular black string spacetimes in nonlinear electrodynamics","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-02T17:53:11.090410Z"},"links":{"cited_paper":"/paper/2203.04965","citing_paper":"/paper/2603.23556"},"observation_digest":"sha256:3159e9b19d6667491e1445dc4511d4e7e1d46800c801cce229ce3d689b4cd866","observation_id":"96b00b33-9a09-41fc-a99e-349e7dac1952","resolution":{"observed_at":"2026-08-02T17:53:11.090410Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2203.04965/citation-record","integrity":"/paper/2203.04965/integrity","json":"/paper/2203.04965/citation-record.json","paper":"/paper/2203.04965"},"outbound":[],"paper":{"arxiv_id":"2203.04965","last_updated":"2022-04-25T22:30:40Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T12:46:08.838773Z","submitted_at":"2022-03-09T17:21:15Z","title":"Bardeen-Kiselev black hole with cosmological constant"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2203.04965."}