{"as_of":"2026-08-23T19:50:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bb7749472bfb8887f623bce31219a9417825de0401e6d48aa77e8978b49e8e21","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:59:44.639035Z","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":"2026-05-16T02:42:10.629406Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2204.03259","last_updated":"2022-08-03T23:23:12Z","snapshot_observed_at":"2026-08-21T16:29:50.040315Z","submitted_at":"2022-04-07T07:12:06Z","title":"Quasinormal modes of self-dual black holes in loop quantum gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.03259","snapshot_observed_at":"2026-08-11T22:07:37.300222Z","title":"Momennia, Quasinormal modes of self-dual black holes in loop quantum gravity , Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03885","last_updated":"2025-03-31T20:18:48Z","snapshot_observed_at":"2026-08-17T07:41:19.479388Z","submitted_at":"2024-12-05T05:35:51Z","title":"Energy Extraction from Loop Quantum Black Holes: The Role of Magnetic Penrose Process and Quantum Gravity Effects with Astrophysical Insights","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T22:07:37.300222Z"},"links":{"cited_paper":"/paper/2204.03259","citing_paper":"/paper/2412.03885"},"observation_digest":"sha256:eee2445105df7c809e1b12156a606fd25a409a9dd3b7188a3f2d1a20d7fac183","observation_id":"f576729d-f6a4-48a1-9302-558cff758864","resolution":{"observed_at":"2026-08-11T22:07:37.300222Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.03259","last_updated":"2022-08-03T23:23:12Z","snapshot_observed_at":"2026-08-21T16:29:50.040315Z","submitted_at":"2022-04-07T07:12:06Z","title":"Quasinormal modes of self-dual black holes in loop quantum gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.03259","snapshot_observed_at":"2026-08-15T21:59:44.639035Z","title":"Momennia, Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.08545","last_updated":"2025-05-13T13:17:23Z","snapshot_observed_at":"2026-08-19T07:10:47.154734Z","submitted_at":"2025-05-13T13:17:23Z","title":"Long-Lived Quasinormal Modes and Quasi-Resonances around Non-Minimal Einstein-Yang-Mills Black Holes","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-15T21:59:44.639035Z"},"links":{"cited_paper":"/paper/2204.03259","citing_paper":"/paper/2505.08545"},"observation_digest":"sha256:49c22fe28210f8abdfbc8a2a79f829fb150506bd2bd6513cfc23a2dc0ce4a0d0","observation_id":"7afa792c-e10b-4952-88b8-6b46fbcf0a88","resolution":{"observed_at":"2026-08-15T21:59:44.639035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.03259","last_updated":"2022-08-03T23:23:12Z","snapshot_observed_at":"2026-08-21T16:29:50.040315Z","submitted_at":"2022-04-07T07:12:06Z","title":"Quasinormal modes of self-dual black holes in loop quantum gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.03259","snapshot_observed_at":"2026-08-03T22:11:08.716261Z","title":"Momennia, Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.12335","last_updated":"2026-05-28T09:58:14Z","snapshot_observed_at":"2026-08-17T14:56:41.731279Z","submitted_at":"2025-11-15T19:28:44Z","title":"Long-lived quasinormal modes and grey-body factors of supermassive black holes with a dark matter halo","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-03T22:11:08.716261Z"},"links":{"cited_paper":"/paper/2204.03259","citing_paper":"/paper/2511.12335"},"observation_digest":"sha256:7b47a94445ca4098db65e68fcd8e46feb958ad3f79e1fc41dbe98c6f63f02095","observation_id":"428c3d8d-fa55-4260-829a-4c798fa62596","resolution":{"observed_at":"2026-08-03T22:11:08.716261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.03259","last_updated":"2022-08-03T23:23:12Z","snapshot_observed_at":"2026-08-21T16:29:50.040315Z","submitted_at":"2022-04-07T07:12:06Z","title":"Quasinormal modes of self-dual black holes in loop quantum gravity","version":2},"cited_work":{"arxiv_id":"2204.03259","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.03259","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Momennia, Phys","venue":null,"work_id":"a308f6e4-4d5a-4bab-8017-3f7fd814d181","year":2022},"citing_paper":{"arxiv_id":"2602.11001","last_updated":"2026-04-17T10:43:09Z","snapshot_observed_at":"2026-08-15T05:19:27.872023Z","submitted_at":"2026-02-11T16:23:23Z","title":"Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-05-16T02:41:01.645151Z"},"links":{"cited_paper":"/paper/2204.03259","citing_paper":"/paper/2602.11001"},"observation_digest":"sha256:4488fba17062ba120bb1f60bf0ded15bd5083b9f70816ccf9c8bac032afbe141","observation_id":"d6e65739-bf5c-47ac-bf28-bff49805e8d2","resolution":{"observed_at":"2026-05-16T02:42:10.632754Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.03259","last_updated":"2022-08-03T23:23:12Z","snapshot_observed_at":"2026-08-21T16:29:50.040315Z","submitted_at":"2022-04-07T07:12:06Z","title":"Quasinormal modes of self-dual black holes in loop quantum gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.03259","snapshot_observed_at":"2026-07-12T01:38:05.217536Z","title":"Momennia, Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-20T21:29:40.209208Z","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":92,"source":"pdf_text","source_observed_at":"2026-07-12T01:38:05.217536Z"},"links":{"cited_paper":"/paper/2204.03259","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:8fb564fdbdb2bb5f595810b54ea1fb027087ae174e90e2d01cc6aa7ba23d4fc2","observation_id":"aac55b81-09f4-4154-a609-da0422ebee68","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":"2204.03259","last_updated":"2022-08-03T23:23:12Z","snapshot_observed_at":"2026-08-21T16:29:50.040315Z","submitted_at":"2022-04-07T07:12:06Z","title":"Quasinormal modes of self-dual black holes in loop quantum gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.03259","snapshot_observed_at":"2026-08-02T08:53:13.538095Z","title":"Momennia, Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.07715","last_updated":"2026-07-28T13:09:16Z","snapshot_observed_at":"2026-08-20T21:29:40.209208Z","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":109,"source":"pdf_text","source_observed_at":"2026-08-02T08:53:13.538095Z"},"links":{"cited_paper":"/paper/2204.03259","citing_paper":"/paper/2607.07715"},"observation_digest":"sha256:0ad38048a75b1f5eb06a55599d5451a09230461ee1b5868954e236bacd766f86","observation_id":"01d9a2b8-3a75-4dc4-8570-02b4ad85d434","resolution":{"observed_at":"2026-08-02T08:53:13.538095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.03259","last_updated":"2022-08-03T23:23:12Z","snapshot_observed_at":"2026-08-21T16:29:50.040315Z","submitted_at":"2022-04-07T07:12:06Z","title":"Quasinormal modes of self-dual black holes in loop quantum gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.03259","snapshot_observed_at":"2026-08-02T01:11:19.484604Z","title":"Quasinormal modes of loop quantum black holes,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.15324","last_updated":"2026-07-16T09:48:22Z","snapshot_observed_at":"2026-08-20T11:15:34.986098Z","submitted_at":"2026-07-16T09:48:22Z","title":"Quasinormal Modes of Self-Dual Loop Quantum Gravity Corrected Kerr Black Holes","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-02T01:11:19.484604Z"},"links":{"cited_paper":"/paper/2204.03259","citing_paper":"/paper/2607.15324"},"observation_digest":"sha256:fa05367fdc9515c9aa890336b98fd144b3a4aba295589f855a202664d40b9d06","observation_id":"c2fbac00-83b7-4329-8f22-4298f1eee859","resolution":{"observed_at":"2026-08-02T01:11:19.484604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2204.03259/citation-record","integrity":"/paper/2204.03259/integrity","json":"/paper/2204.03259/citation-record.json","paper":"/paper/2204.03259"},"outbound":[],"paper":{"arxiv_id":"2204.03259","last_updated":"2022-08-03T23:23:12Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-21T16:29:50.040315Z","submitted_at":"2022-04-07T07:12:06Z","title":"Quasinormal modes of self-dual black holes in loop quantum gravity"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2204.03259."}