{"as_of":"2026-08-09T04:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:95e9f8ef45c9d32678236d01555c6732b5a60f547aa4012b6a5c3b53705f3150","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T16:12:04.315733Z","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":"2026-07-03T11:48:05.118013Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2302.14722","last_updated":"2023-02-28T16:32:32Z","snapshot_observed_at":"2026-07-06T14:56:54.731501Z","submitted_at":"2023-02-28T16:32:32Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.14722","snapshot_observed_at":"2026-08-07T15:00:33.563198Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.16883","last_updated":"2025-05-29T16:46:47Z","snapshot_observed_at":"2026-08-07T16:30:52.556811Z","submitted_at":"2025-05-22T16:36:53Z","title":"Test-Field vs Physical Quasi-Normal Modes in Scalar-Tensor Theories","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-07T15:00:33.563198Z"},"links":{"cited_paper":"/paper/2302.14722","citing_paper":"/paper/2505.16883"},"observation_digest":"sha256:9f7ab8f6a25102a8aff8ad12db8f2c503d0d86b809472e449bdf2f3aaa06c15b","observation_id":"bafde0a2-4b76-4f12-b596-ea62b87aa0a7","resolution":{"observed_at":"2026-08-07T15:00:33.563198Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.14722","last_updated":"2023-02-28T16:32:32Z","snapshot_observed_at":"2026-07-06T14:56:54.731501Z","submitted_at":"2023-02-28T16:32:32Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":"2302.14722","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.14722","snapshot_observed_at":"2026-07-03T11:48:05.118013Z","title":null,"venue":null,"work_id":"8301920c-d8e2-47b3-b39e-7770013ad198","year":2023},"citing_paper":{"arxiv_id":"2506.16217","last_updated":"2026-04-06T09:35:14Z","snapshot_observed_at":"2026-07-06T21:44:42.748650Z","submitted_at":"2025-06-19T11:09:00Z","title":"Quasinormal modes and grey-body factors of axial gravitational perturbations of regular black holes in asymptotically safe gravity","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-19T09:05:31.241151Z"},"links":{"cited_paper":"/paper/2302.14722","citing_paper":"/paper/2506.16217"},"observation_digest":"sha256:49af6069256f274c1bb472aabe362a26b6a11435644b05b1e876f9d4d0d7f360","observation_id":"4b01089c-412a-413b-8c26-4b23051b0a9d","resolution":{"observed_at":"2026-05-19T09:07:14.393753Z","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":"2302.14722","last_updated":"2023-02-28T16:32:32Z","snapshot_observed_at":"2026-07-06T14:56:54.731501Z","submitted_at":"2023-02-28T16:32:32Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.14722","snapshot_observed_at":"2026-08-04T11:09:50.793684Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.06689","last_updated":"2026-05-28T09:50:09Z","snapshot_observed_at":"2026-08-04T11:09:41.169992Z","submitted_at":"2025-10-08T06:25:32Z","title":"Bonanno-Reuter regular black hole: quasi-resonances, grey-body factors and absorption cross-sections of a massive scalar field","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-04T11:09:50.793684Z"},"links":{"cited_paper":"/paper/2302.14722","citing_paper":"/paper/2510.06689"},"observation_digest":"sha256:4fc9a55ace87221834140f3f713ac399f151dbf71787b56dfc9e78ae8f1ec091","observation_id":"8ba8c742-6666-43da-88a4-d4eb310d06ce","resolution":{"observed_at":"2026-08-04T11:09:50.793684Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.14722","last_updated":"2023-02-28T16:32:32Z","snapshot_observed_at":"2026-07-06T14:56:54.731501Z","submitted_at":"2023-02-28T16:32:32Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":"2302.14722","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.14722","snapshot_observed_at":"2026-07-03T11:48:05.118013Z","title":null,"venue":null,"work_id":"8301920c-d8e2-47b3-b39e-7770013ad198","year":2023},"citing_paper":{"arxiv_id":"2601.17906","last_updated":"2026-04-02T18:11:47Z","snapshot_observed_at":"2026-07-06T22:42:57.796038Z","submitted_at":"2026-01-25T16:54:41Z","title":"Telling tails and quasi-resonances in the vicinity of Dymnikova regular black hole","version":2},"reference_index":126,"source":"pdf_text","source_observed_at":"2026-05-16T11:06:54.209646Z"},"links":{"cited_paper":"/paper/2302.14722","citing_paper":"/paper/2601.17906"},"observation_digest":"sha256:9dbe00c31226f2dc64d59facda68b297db1f0563ea0532e9c3747fd555e94560","observation_id":"71b31aa1-2c41-420f-aabf-83813f099c3c","resolution":{"observed_at":"2026-05-16T11:07:47.356031Z","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":"2302.14722","last_updated":"2023-02-28T16:32:32Z","snapshot_observed_at":"2026-07-06T14:56:54.731501Z","submitted_at":"2023-02-28T16:32:32Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":"2302.14722","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.14722","snapshot_observed_at":"2026-07-03T11:48:05.118013Z","title":null,"venue":null,"work_id":"8301920c-d8e2-47b3-b39e-7770013ad198","year":2023},"citing_paper":{"arxiv_id":"2603.25084","last_updated":"2026-04-23T10:20:59Z","snapshot_observed_at":"2026-07-06T22:50:37.468743Z","submitted_at":"2026-03-26T06:38:36Z","title":"Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-15T00:56:02.789832Z"},"links":{"cited_paper":"/paper/2302.14722","citing_paper":"/paper/2603.25084"},"observation_digest":"sha256:220f0db71ca9a52529944dcd338a5ad8a5a32eebfc20fc78b11a1bbd86ab5a94","observation_id":"487fe847-6a4e-4a9f-871a-ff441a3e111f","resolution":{"observed_at":"2026-05-15T00:58:25.826651Z","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":"2302.14722","last_updated":"2023-02-28T16:32:32Z","snapshot_observed_at":"2026-07-06T14:56:54.731501Z","submitted_at":"2023-02-28T16:32:32Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":"2302.14722","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.14722","snapshot_observed_at":"2026-07-03T11:48:05.118013Z","title":null,"venue":null,"work_id":"8301920c-d8e2-47b3-b39e-7770013ad198","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":52,"source":"pdf_text","source_observed_at":"2026-05-20T09:22:46.533112Z"},"links":{"cited_paper":"/paper/2302.14722","citing_paper":"/paper/2605.18249"},"observation_digest":"sha256:fcb87d7effe99f91ef340e7925e01e8705862e355fd90cfe19e389eaefc914cb","observation_id":"8ca912dc-24cf-4bf0-bcb8-fafb5502e18f","resolution":{"observed_at":"2026-05-20T09:23:10.480707Z","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":"2302.14722","last_updated":"2023-02-28T16:32:32Z","snapshot_observed_at":"2026-07-06T14:56:54.731501Z","submitted_at":"2023-02-28T16:32:32Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":"2302.14722","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.14722","snapshot_observed_at":"2026-07-03T11:48:05.118013Z","title":null,"venue":null,"work_id":"8301920c-d8e2-47b3-b39e-7770013ad198","year":2023},"citing_paper":{"arxiv_id":"2606.11728","last_updated":"2026-06-10T07:06:19Z","snapshot_observed_at":"2026-08-02T11:15:29.805470Z","submitted_at":"2026-06-10T07:06:19Z","title":"Periodic orbits as probes of charged loop quantum gravity black holes through gravitational waves","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-06-27T09:21:09.169388Z"},"links":{"cited_paper":"/paper/2302.14722","citing_paper":"/paper/2606.11728"},"observation_digest":"sha256:831ea12610d5a416c8e7e9101c028e3be4aa1f11f12b20f9c2ae5deb2094d0ea","observation_id":"bf20b3cc-6126-4657-af82-0dc343a773c8","resolution":{"observed_at":"2026-07-03T11:48:05.119564Z","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":"2302.14722","last_updated":"2023-02-28T16:32:32Z","snapshot_observed_at":"2026-07-06T14:56:54.731501Z","submitted_at":"2023-02-28T16:32:32Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.14722","snapshot_observed_at":"2026-08-08T16:12:04.315733Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.05292","last_updated":"2026-08-05T18:00:05Z","snapshot_observed_at":"2026-08-09T04:10:39.851461Z","submitted_at":"2026-08-05T18:00:05Z","title":"Absorption spectrum and greybody factors of charged black holes in loop quantum gravity","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-08T16:12:04.315733Z"},"links":{"cited_paper":"/paper/2302.14722","citing_paper":"/paper/2608.05292"},"observation_digest":"sha256:3714601d897534f1ab1907e3dedd44d9621006224657fdfa0a88652870ec32f0","observation_id":"0d8c2bca-bb62-4d60-a2cd-0cb01009488a","resolution":{"observed_at":"2026-08-08T16:12:04.315733Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2302.14722/citation-record","integrity":"/paper/2302.14722/integrity","json":"/paper/2302.14722/citation-record.json","paper":"/paper/2302.14722"},"outbound":[],"paper":{"arxiv_id":"2302.14722","last_updated":"2023-02-28T16:32:32Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T14:56:54.731501Z","submitted_at":"2023-02-28T16:32:32Z","title":"Quasinormal modes of a holonomy corrected Schwarzschild black hole"},"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 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2302.14722."}