{"as_of":"2026-08-21T04:23:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3c6e27c4a435d1118a01bc69552837ce8eb094f83170b7dc1d71342147fbdf01","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":"2026-08-20T06:33:59.587034+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":"2026-08-15T21:07:26.779341Z","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":"2026-05-19T09:07:14.474428Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.21597","last_updated":"2025-03-27T15:16:02Z","snapshot_observed_at":"2026-08-21T03:59:14.891482Z","submitted_at":"2025-03-27T15:16:02Z","title":"Correspondence between grey-body factors and quasinormal modes for regular black holes with sub-Planckian curvature","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.21597","snapshot_observed_at":"2026-08-15T21:07:26.779341Z","title":"Correspondence between grey-body fac- tors and quasinormal modes for regular black holes with sub-Planckian curvature,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.11073","last_updated":"2025-05-16T10:06:57Z","snapshot_observed_at":"2026-08-16T21:02:01.842510Z","submitted_at":"2025-05-16T10:06:57Z","title":"Can we distinguish whether black holes have singularities or not through echoes and light rings?","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T21:07:26.779341Z"},"links":{"cited_paper":"/paper/2503.21597","citing_paper":"/paper/2505.11073"},"observation_digest":"sha256:67a4815872d2b7f3d0afa069a85bb147da473282759dc792064c714c64fd6080","observation_id":"f30885ea-fff9-487b-9e5c-7455f45dc03a","resolution":{"observed_at":"2026-08-15T21:07:26.779341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.21597","last_updated":"2025-03-27T15:16:02Z","snapshot_observed_at":"2026-08-21T03:59:14.891482Z","submitted_at":"2025-03-27T15:16:02Z","title":"Correspondence between grey-body factors and quasinormal modes for regular black holes with sub-Planckian curvature","version":1},"cited_work":{"arxiv_id":"2503.21597","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.21597","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"eaed8ca4-0012-449e-88a1-0c2d1f1d51e2","year":2025},"citing_paper":{"arxiv_id":"2506.16217","last_updated":"2026-04-06T09:35:14Z","snapshot_observed_at":"2026-08-14T12:14:59.835806Z","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":57,"source":"pdf_text","source_observed_at":"2026-05-19T09:05:31.241151Z"},"links":{"cited_paper":"/paper/2503.21597","citing_paper":"/paper/2506.16217"},"observation_digest":"sha256:f6155b5e1d8886f56cae3ea23a28d733523adf2561cdf7309e5ed030478e2ca4","observation_id":"1c531e1a-2dab-4970-bae8-df1821c19094","resolution":{"observed_at":"2026-05-19T09:07:14.477682Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.21597","last_updated":"2025-03-27T15:16:02Z","snapshot_observed_at":"2026-08-21T03:59:14.891482Z","submitted_at":"2025-03-27T15:16:02Z","title":"Correspondence between grey-body factors and quasinormal modes for regular black holes with sub-Planckian curvature","version":1},"cited_work":{"arxiv_id":"2503.21597","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.21597","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"eaed8ca4-0012-449e-88a1-0c2d1f1d51e2","year":2025},"citing_paper":{"arxiv_id":"2512.23510","last_updated":"2026-04-08T06:40:48Z","snapshot_observed_at":"2026-08-14T07:35:11.401242Z","submitted_at":"2025-12-29T14:47:19Z","title":"Quasinormal mode/grey-body factor correspondence for Kerr black holes","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-16T19:26:13.414782Z"},"links":{"cited_paper":"/paper/2503.21597","citing_paper":"/paper/2512.23510"},"observation_digest":"sha256:a3adb4420144797983b3d7bc573c41774d8723b3487ee41ee8ef48e28bbe3f00","observation_id":"b66d6078-0876-48e3-8541-d21144386b77","resolution":{"observed_at":"2026-05-16T19:28:20.258987Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.21597","last_updated":"2025-03-27T15:16:02Z","snapshot_observed_at":"2026-08-21T03:59:14.891482Z","submitted_at":"2025-03-27T15:16:02Z","title":"Correspondence between grey-body factors and quasinormal modes for regular black holes with sub-Planckian curvature","version":1},"cited_work":{"arxiv_id":"2503.21597","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.21597","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"eaed8ca4-0012-449e-88a1-0c2d1f1d51e2","year":2025},"citing_paper":{"arxiv_id":"2601.18613","last_updated":"2026-01-26T15:53:33Z","snapshot_observed_at":"2026-08-14T16:24:18.356843Z","submitted_at":"2026-01-26T15:53:33Z","title":"Correspondence between quasinormal modes and grey-body factors of Schwarzschild--Tangherlini black holes","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-16T10:39:53.182650Z"},"links":{"cited_paper":"/paper/2503.21597","citing_paper":"/paper/2601.18613"},"observation_digest":"sha256:c630e1dddf55fc9c7ede729f900946f0761dd82bd45b26c7ec491739a0c1f205","observation_id":"e97ec3ec-75fb-4d71-b31d-158d229bec81","resolution":{"observed_at":"2026-05-16T10:40:51.138977Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.21597","last_updated":"2025-03-27T15:16:02Z","snapshot_observed_at":"2026-08-21T03:59:14.891482Z","submitted_at":"2025-03-27T15:16:02Z","title":"Correspondence between grey-body factors and quasinormal modes for regular black holes with sub-Planckian curvature","version":1},"cited_work":{"arxiv_id":"2503.21597","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2503.21597","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"eaed8ca4-0012-449e-88a1-0c2d1f1d51e2","year":2025},"citing_paper":{"arxiv_id":"2604.05084","last_updated":"2026-04-06T18:37:06Z","snapshot_observed_at":"2026-08-20T01:48:42.044459Z","submitted_at":"2026-04-06T18:37:06Z","title":"Parametrized quasinormal modes, greybody factors and their correspondence","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-10T18:56:32.433489Z"},"links":{"cited_paper":"/paper/2503.21597","citing_paper":"/paper/2604.05084"},"observation_digest":"sha256:aec4b0f08eb943ef17258e0a4b6118fd54b3441484f2d84735afea307f6c1554","observation_id":"89d1b036-0642-45ba-86c3-ed95902b6c69","resolution":{"observed_at":"2026-05-10T23:40:52.689147Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2503.21597/citation-record","integrity":"/paper/2503.21597/integrity","json":"/paper/2503.21597/citation-record.json","paper":"/paper/2503.21597"},"outbound":[],"paper":{"arxiv_id":"2503.21597","last_updated":"2025-03-27T15:16:02Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-21T03:59:14.891482Z","submitted_at":"2025-03-27T15:16:02Z","title":"Correspondence between grey-body factors and quasinormal modes for regular black holes with sub-Planckian curvature"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2503.21597."}