{"as_of":"2026-08-12T11:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:42ebcc457949dae1c3870b98809c48a29a35362bbfdd43be4067310978142acc","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T13:49:13.824058Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-05-18T09:51:13.019192Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1305.5991","last_updated":"2013-09-23T19:36:30Z","snapshot_observed_at":"2026-07-06T03:14:19.762420Z","submitted_at":"2013-05-26T06:33:39Z","title":"Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or anti-aligned spins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.5991","snapshot_observed_at":"2026-08-11T13:49:13.824058Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.12823","last_updated":"2025-08-21T18:54:24Z","snapshot_observed_at":"2026-08-11T13:39:17.730415Z","submitted_at":"2024-12-17T11:42:40Z","title":"Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM","version":2},"reference_index":281,"source":"pdf_text","source_observed_at":"2026-08-11T13:49:13.824058Z"},"links":{"cited_paper":"/paper/1305.5991","citing_paper":"/paper/2412.12823"},"observation_digest":"sha256:31b5d972f08446499d03f242102ba24adaf05aa5642b75aaf4c72a67f537717e","observation_id":"817eeb2c-0d0e-40f4-ae16-212d6fe7f728","resolution":{"observed_at":"2026-08-11T13:49:13.824058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.5991","last_updated":"2013-09-23T19:36:30Z","snapshot_observed_at":"2026-07-06T03:14:19.762420Z","submitted_at":"2013-05-26T06:33:39Z","title":"Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or anti-aligned spins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.5991","snapshot_observed_at":"2026-08-10T21:37:16.024269Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.04495","last_updated":"2025-01-08T13:28:08Z","snapshot_observed_at":"2026-08-11T14:52:09.774215Z","submitted_at":"2025-01-08T13:28:08Z","title":"Eccentricity Effects on Modeling Dynamic Quantities and Their Correlations in Binary Black Hole Mergers","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-10T21:37:16.024269Z"},"links":{"cited_paper":"/paper/1305.5991","citing_paper":"/paper/2501.04495"},"observation_digest":"sha256:7c4d2f370d49ba870219397e1ee7c725ecda8fc39d97c354fc5022974bf4e850","observation_id":"2459f2f5-417f-4b51-b7c8-50b8270f2c4a","resolution":{"observed_at":"2026-08-10T21:37:16.024269Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.5991","last_updated":"2013-09-23T19:36:30Z","snapshot_observed_at":"2026-07-06T03:14:19.762420Z","submitted_at":"2013-05-26T06:33:39Z","title":"Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or anti-aligned spins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.5991","snapshot_observed_at":"2026-08-08T15:41:06.906738Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.06389","last_updated":"2025-08-23T11:45:52Z","snapshot_observed_at":"2026-08-11T21:30:41.309866Z","submitted_at":"2025-02-10T12:18:33Z","title":"Relativistic gas accretion onto supermassive black Hole binaries from inspiral through merger","version":5},"reference_index":158,"source":"pdf_text","source_observed_at":"2026-08-08T15:41:06.906738Z"},"links":{"cited_paper":"/paper/1305.5991","citing_paper":"/paper/2502.06389"},"observation_digest":"sha256:508f2861e57950b87b94b4a785ca7f060fd1a5f0dc4aaeab3ec7f46298931371","observation_id":"18591748-9ab4-4b63-82a0-df817134203b","resolution":{"observed_at":"2026-08-08T15:41:06.906738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.5991","last_updated":"2013-09-23T19:36:30Z","snapshot_observed_at":"2026-07-06T03:14:19.762420Z","submitted_at":"2013-05-26T06:33:39Z","title":"Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or anti-aligned spins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.5991","snapshot_observed_at":"2026-08-06T14:25:06.093478Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.19431","last_updated":"2025-07-25T16:58:30Z","snapshot_observed_at":"2026-08-10T16:27:35.236416Z","submitted_at":"2025-07-25T16:58:30Z","title":"Remnant properties of binary neutron star mergers undergoing prompt collapse","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-06T14:25:06.093478Z"},"links":{"cited_paper":"/paper/1305.5991","citing_paper":"/paper/2507.19431"},"observation_digest":"sha256:76e0d56d8664e1546c8a4bb3bb3079de8af0418b0bcd4a0d36cf76afd6a56ba3","observation_id":"da4adad9-14bc-49bc-a540-40141c008bd6","resolution":{"observed_at":"2026-08-06T14:25:06.093478Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.5991","last_updated":"2013-09-23T19:36:30Z","snapshot_observed_at":"2026-07-06T03:14:19.762420Z","submitted_at":"2013-05-26T06:33:39Z","title":"Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or anti-aligned spins","version":2},"cited_work":{"arxiv_id":"1305.5991","doi":null,"metadata_source":"pith","pith_arxiv_id":"1305.5991","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or anti-aligned spins","venue":"gr-qc","work_id":"b6f8d50f-350a-4760-bd60-49e854a18004","year":2013},"citing_paper":{"arxiv_id":"2510.04332","last_updated":"2026-05-12T13:46:37Z","snapshot_observed_at":"2026-08-07T20:58:26.847096Z","submitted_at":"2025-10-05T19:29:41Z","title":"Biased parameter inference of eccentric, spin-precessing binary black holes","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-05-18T09:50:50.035204Z"},"links":{"cited_paper":"/paper/1305.5991","citing_paper":"/paper/2510.04332"},"observation_digest":"sha256:344611bd9937b764bea44c46296199382438ad9f994e84d74bd9354a2202d63d","observation_id":"37766178-c694-44c2-856b-303c6381a318","resolution":{"observed_at":"2026-05-18T09:51:13.021689Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1305.5991","last_updated":"2013-09-23T19:36:30Z","snapshot_observed_at":"2026-07-06T03:14:19.762420Z","submitted_at":"2013-05-26T06:33:39Z","title":"Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or anti-aligned spins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.5991","snapshot_observed_at":"2026-07-15T14:26:35.666160Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2603.05601","last_updated":"2026-03-05T19:01:03Z","snapshot_observed_at":"2026-08-04T08:29:47.055382Z","submitted_at":"2026-03-05T19:01:03Z","title":"Advancing the Effective-One-Body Framework in the Test-Mass Limit","version":1},"reference_index":126,"source":"pdf_text","source_observed_at":"2026-07-15T14:26:35.666160Z"},"links":{"cited_paper":"/paper/1305.5991","citing_paper":"/paper/2603.05601"},"observation_digest":"sha256:222aac85bfe15a3ed24c0671ce19e46d07bfd49e99de56ab003d3b0893a5b50d","observation_id":"e8191dea-8be1-4e77-a3f5-d4e57c705b1f","resolution":{"observed_at":"2026-07-15T14:26:35.666160Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1305.5991/citation-record","integrity":"/paper/1305.5991/integrity","json":"/paper/1305.5991/citation-record.json","paper":"/paper/1305.5991"},"outbound":[],"paper":{"arxiv_id":"1305.5991","last_updated":"2013-09-23T19:36:30Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T03:14:19.762420Z","submitted_at":"2013-05-26T06:33:39Z","title":"Final spin and radiated energy in numerical simulations of binary black holes with equal masses and equal, aligned or anti-aligned spins"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1305.5991."}