{"as_of":"2026-08-15T23:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:706eb3a178dcabe8bc77271b7cd085ac874b471104f9fc3aea380f291477667e","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":"2026-08-15T06:32:42.880941+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":"2026-08-15T19:54:50.578422Z","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":"2026-07-03T15:08:32.927547Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.09796","last_updated":"2025-05-03T00:56:00Z","snapshot_observed_at":"2026-08-12T22:24:29.461241Z","submitted_at":"2024-10-13T10:51:33Z","title":"Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.09796","snapshot_observed_at":"2026-08-15T19:54:50.578422Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.14868","last_updated":"2025-06-25T18:00:00Z","snapshot_observed_at":"2026-08-15T19:44:53.730002Z","submitted_at":"2025-06-17T18:00:00Z","title":"Gravitational waves from b-EMRIs: Doppler shift and beaming, resonant excitation, helicity oscillations and self-lensing","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T19:54:50.578422Z"},"links":{"cited_paper":"/paper/2410.09796","citing_paper":"/paper/2506.14868"},"observation_digest":"sha256:f0347cc0427b9f35907cf244ce1e4a9546bbf638106c6fbee9bc924891c29ef1","observation_id":"ee336969-e4db-4264-96ff-62e2da0aa1ca","resolution":{"observed_at":"2026-08-15T19:54:50.578422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09796","last_updated":"2025-05-03T00:56:00Z","snapshot_observed_at":"2026-08-12T22:24:29.461241Z","submitted_at":"2024-10-13T10:51:33Z","title":"Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation","version":2},"cited_work":{"arxiv_id":"2410.09796","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.09796","snapshot_observed_at":"2026-07-03T15:08:32.927547Z","title":"Relativistic model of binary extreme-mass- ratio inspiral systems and their gravitational radiation","venue":null,"work_id":"9453cda7-9498-4b28-b243-b9c8c8fbaf83","year":2025},"citing_paper":{"arxiv_id":"2510.16113","last_updated":"2026-04-26T06:30:13Z","snapshot_observed_at":"2026-08-15T04:11:11.854374Z","submitted_at":"2025-10-17T18:00:38Z","title":"Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-05-18T05:52:48.547252Z"},"links":{"cited_paper":"/paper/2410.09796","citing_paper":"/paper/2510.16113"},"observation_digest":"sha256:fc73642a3817c3d6fecd0e5b83ba62ac925bb75b3b244c020bf0260f2b230fe1","observation_id":"1f321c2a-5a73-450d-a096-bc52af9ae1ff","resolution":{"observed_at":"2026-05-18T05:55:57.225495Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09796","last_updated":"2025-05-03T00:56:00Z","snapshot_observed_at":"2026-08-12T22:24:29.461241Z","submitted_at":"2024-10-13T10:51:33Z","title":"Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.09796","snapshot_observed_at":"2026-08-04T07:44:07.386270Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.24897","last_updated":"2026-07-20T13:33:40Z","snapshot_observed_at":"2026-08-15T11:57:23.695028Z","submitted_at":"2025-10-28T19:00:01Z","title":"Observable signature of magnetic tidal coupling in hierarchical triple systems","version":3},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-04T07:44:07.386270Z"},"links":{"cited_paper":"/paper/2410.09796","citing_paper":"/paper/2510.24897"},"observation_digest":"sha256:8be653a0699237769747ed854902de5373cdccd7d42c10feb3a51026b18a750a","observation_id":"580e25ab-6479-4076-bbd8-75c01ab18bb4","resolution":{"observed_at":"2026-08-04T07:44:07.386270Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09796","last_updated":"2025-05-03T00:56:00Z","snapshot_observed_at":"2026-08-12T22:24:29.461241Z","submitted_at":"2024-10-13T10:51:33Z","title":"Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation","version":2},"cited_work":{"arxiv_id":"2410.09796","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.09796","snapshot_observed_at":"2026-07-03T15:08:32.927547Z","title":"Relativistic model of binary extreme-mass- ratio inspiral systems and their gravitational radiation","venue":null,"work_id":"9453cda7-9498-4b28-b243-b9c8c8fbaf83","year":2025},"citing_paper":{"arxiv_id":"2604.24413","last_updated":"2026-04-27T12:40:35Z","snapshot_observed_at":"2026-07-06T23:10:29.508602Z","submitted_at":"2026-04-27T12:40:35Z","title":"Gravitational waves of extreme-mass-ratio inspirals in a rotating black hole with Dehnen dark matter halo","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-08T02:13:24.333816Z"},"links":{"cited_paper":"/paper/2410.09796","citing_paper":"/paper/2604.24413"},"observation_digest":"sha256:24357736da77ae311daa95875e7291a54c830443534bc351730ab0460a574cbb","observation_id":"32eb5f47-38b8-498d-98f2-365fc38e8ab1","resolution":{"observed_at":"2026-05-11T22:56:16.500274Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09796","last_updated":"2025-05-03T00:56:00Z","snapshot_observed_at":"2026-08-12T22:24:29.461241Z","submitted_at":"2024-10-13T10:51:33Z","title":"Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation","version":2},"cited_work":{"arxiv_id":"2410.09796","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.09796","snapshot_observed_at":"2026-07-03T15:08:32.927547Z","title":"Relativistic model of binary extreme-mass- ratio inspiral systems and their gravitational radiation","venue":null,"work_id":"9453cda7-9498-4b28-b243-b9c8c8fbaf83","year":2025},"citing_paper":{"arxiv_id":"2605.15160","last_updated":"2026-05-14T17:53:26Z","snapshot_observed_at":"2026-08-11T15:15:38.373630Z","submitted_at":"2026-05-14T17:53:26Z","title":"N-body next-to-leading order gravitational spin-orbit interaction via effective field theory","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-05-15T03:03:16.273348Z"},"links":{"cited_paper":"/paper/2410.09796","citing_paper":"/paper/2605.15160"},"observation_digest":"sha256:4c7b660471dbc5290f0adf8b28763ffe31fac1a01c4ac973aec96bed9463b874","observation_id":"00e4631a-0160-4677-912b-0dacf16281e2","resolution":{"observed_at":"2026-05-15T03:03:56.925688Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09796","last_updated":"2025-05-03T00:56:00Z","snapshot_observed_at":"2026-08-12T22:24:29.461241Z","submitted_at":"2024-10-13T10:51:33Z","title":"Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation","version":2},"cited_work":{"arxiv_id":"2410.09796","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.09796","snapshot_observed_at":"2026-07-03T15:08:32.927547Z","title":"Relativistic model of binary extreme-mass- ratio inspiral systems and their gravitational radiation","venue":null,"work_id":"9453cda7-9498-4b28-b243-b9c8c8fbaf83","year":2025},"citing_paper":{"arxiv_id":"2605.20320","last_updated":"2026-07-17T11:50:21Z","snapshot_observed_at":"2026-08-14T15:22:02.323739Z","submitted_at":"2026-05-19T18:00:00Z","title":"Ringdown and lensing of triple systems","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-21T01:56:09.110305Z"},"links":{"cited_paper":"/paper/2410.09796","citing_paper":"/paper/2605.20320"},"observation_digest":"sha256:2521aaabe7660534bbf60c582cf02897ca83f7ada4b28b2eb71684336619ab1b","observation_id":"541c241f-f2ac-4bdb-ae2a-773461adaaba","resolution":{"observed_at":"2026-05-21T01:59:23.284495Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09796","last_updated":"2025-05-03T00:56:00Z","snapshot_observed_at":"2026-08-12T22:24:29.461241Z","submitted_at":"2024-10-13T10:51:33Z","title":"Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.09796","snapshot_observed_at":"2026-08-02T13:41:03.932227Z","title":"Relativistic model of binary extreme-mass- ratio inspiral systems and their gravitational radiation,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.20320","last_updated":"2026-07-17T11:50:21Z","snapshot_observed_at":"2026-08-14T15:22:02.323739Z","submitted_at":"2026-05-19T18:00:00Z","title":"Ringdown and lensing of triple systems","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-02T13:41:03.932227Z"},"links":{"cited_paper":"/paper/2410.09796","citing_paper":"/paper/2605.20320"},"observation_digest":"sha256:d08711c2041ac196a48cc1fa328ac90a8c23e10a1fb6865e15bd63d33cbd5a2e","observation_id":"fdcd8ea1-6342-4132-97d4-0f78597b5562","resolution":{"observed_at":"2026-08-02T13:41:03.932227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09796","last_updated":"2025-05-03T00:56:00Z","snapshot_observed_at":"2026-08-12T22:24:29.461241Z","submitted_at":"2024-10-13T10:51:33Z","title":"Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation","version":2},"cited_work":{"arxiv_id":"2410.09796","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.09796","snapshot_observed_at":"2026-07-03T15:08:32.927547Z","title":"Relativistic model of binary extreme-mass- ratio inspiral systems and their gravitational radiation","venue":null,"work_id":"9453cda7-9498-4b28-b243-b9c8c8fbaf83","year":2025},"citing_paper":{"arxiv_id":"2606.12784","last_updated":"2026-06-11T00:57:08Z","snapshot_observed_at":"2026-07-29T21:06:51.687638Z","submitted_at":"2026-06-11T00:57:08Z","title":"Constraining Kerr supermassive black hole properties using gravitational waves from inspiraling stellar-mass binary black holes","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-06-27T06:41:50.946674Z"},"links":{"cited_paper":"/paper/2410.09796","citing_paper":"/paper/2606.12784"},"observation_digest":"sha256:ffee64f07846694923d353457b09bbef31ea66256e3bb69285cc8abd2ee6225b","observation_id":"59f079f8-52a9-49c2-ba10-b70090ae1ebc","resolution":{"observed_at":"2026-07-03T15:08:32.928970Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2410.09796/citation-record","integrity":"/paper/2410.09796/integrity","json":"/paper/2410.09796/citation-record.json","paper":"/paper/2410.09796"},"outbound":[],"paper":{"arxiv_id":"2410.09796","last_updated":"2025-05-03T00:56:00Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-12T22:24:29.461241Z","submitted_at":"2024-10-13T10:51:33Z","title":"Relativistic model of binary extreme-mass-ratio inspiral systems and their gravitational radiation"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2410.09796."}