{"as_of":"2026-08-07T01:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c3faf693f8398e82874a1b0eaf9269fb8aef457abd4ef6daa847216da2cca6e2","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T09:50:04.043579Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":119,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1205.6348","last_updated":"2012-09-11T15:24:47Z","snapshot_observed_at":"2026-08-03T18:44:22.394846Z","submitted_at":"2012-05-29T12:44:19Z","title":"Probing the space-time geometry around black hole candidates with the resonance models for high-frequency QPOs and comparison with the continuum-fitting method","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.6348","snapshot_observed_at":"2026-08-04T09:50:04.043579Z","title":"Probing the space-time geometry around blac k hole candidates with the resonance models for high-freque ncy QPOs and comparison with the continuum-ﬁtting method,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2510.13552","last_updated":"2026-07-12T04:46:12Z","snapshot_observed_at":"2026-08-06T21:07:25.125422Z","submitted_at":"2025-10-15T13:49:01Z","title":"Mapping Quasi-Periodic Oscillations to Lyapunov Exponent across Black Hole Thermodynamic Phase Transitions","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-04T09:50:04.043579Z"},"links":{"cited_paper":"/paper/1205.6348","citing_paper":"/paper/2510.13552"},"observation_digest":"sha256:95b5c98f29593ce66c404cc9883db1c81fbef0e5cd721a9b64ee95f7b5dcb21d","observation_id":"a19f2381-1f30-43f5-9c15-e206db838ec9","resolution":{"observed_at":"2026-08-04T09:50:04.043579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.6348","last_updated":"2012-09-11T15:24:47Z","snapshot_observed_at":"2026-08-03T18:44:22.394846Z","submitted_at":"2012-05-29T12:44:19Z","title":"Probing the space-time geometry around black hole candidates with the resonance models for high-frequency QPOs and comparison with the continuum-fitting method","version":2},"cited_work":{"arxiv_id":"1205.6348","doi":"10.1088/1475-7516/2012/09/014","metadata_source":"pith","pith_arxiv_id":"1205.6348","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Probing the space-time geometry around black hole candidates with the resonance models for high-frequency QPOs and comparison with the continuum-fitting method","venue":"gr-qc","work_id":"b9467093-5932-4224-aa89-cf8bfcc6d930","year":2012},"citing_paper":{"arxiv_id":"2606.10964","last_updated":"2026-06-09T15:03:52Z","snapshot_observed_at":"2026-08-02T21:12:49.567331Z","submitted_at":"2026-06-09T15:03:52Z","title":"The link between obscured accretion and mildly relativistic precessing jets","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1205.6348","citing_paper":"/paper/2606.10964"},"observation_digest":"sha256:40c9fd46d2dfa0a3797a80f56258c0c09701ad11b2c0db459f834513dc31ffe8","observation_id":"0fc8066a-0cf9-43c8-8c6f-08d19d645a67","resolution":{"observed_at":"2026-06-27T14:01:00.613243Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-07-13T10:19:36.708513+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T10:19:36.708513+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.6348","last_updated":"2012-09-11T15:24:47Z","snapshot_observed_at":"2026-08-03T18:44:22.394846Z","submitted_at":"2012-05-29T12:44:19Z","title":"Probing the space-time geometry around black hole candidates with the resonance models for high-frequency QPOs and comparison with the continuum-fitting method","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.6348","snapshot_observed_at":"2026-07-13T05:19:16.347394Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.09112","last_updated":"2026-07-10T05:50:09Z","snapshot_observed_at":"2026-08-05T12:36:28.197886Z","submitted_at":"2026-07-10T05:50:09Z","title":"Physics and Astrophysics of Black Holes with eXTP","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-13T05:19:16.347394Z"},"links":{"cited_paper":"/paper/1205.6348","citing_paper":"/paper/2607.09112"},"observation_digest":"sha256:a65398d2ab61d11fab1d03b817e625ce492a7432dee82ca7dabe6c2421933a9e","observation_id":"6920c7e6-a135-40ab-bbfd-6d78c3232d99","resolution":{"observed_at":"2026-07-13T05:19:16.347394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1205.6348/citation-record","integrity":"/paper/1205.6348/integrity","json":"/paper/1205.6348/citation-record.json","paper":"/paper/1205.6348"},"outbound":[],"paper":{"arxiv_id":"1205.6348","last_updated":"2012-09-11T15:24:47Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-03T18:44:22.394846Z","submitted_at":"2012-05-29T12:44:19Z","title":"Probing the space-time geometry around black hole candidates with the resonance models for high-frequency QPOs and comparison with the continuum-fitting method"},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1205.6348."}